On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
On August 17, 1996, the Japanese Space Agency (NASDA - National Space Development Agency)
launched the Advanced Earth Observing Satellite (ADEOS). ADEOS was in a descending, Sun
synchronous orbit with a nominal equatorial crossing time of 10:30 a.m. Amoung the
instruments carried aboard the ADEOS spacecraft was the Ocean Color and Temperature
Scanner (OCTS). OCTS is an optical radiometer with 12 bands covering the visible, near
infrared and thermal infrared regions. (Eight of the bands are in the VIS/NIR. These are
the only bands calibrated and processed by the OBPG) OCTS has a swath width of
approximately 1400 km, and a nominal nadir resolution of 700 m. The instrument operated
at three tilt states (20 degrees aft, nadir and 20 degrees fore), similar to SeaWiFS.
TEMPLATE_PRODDESCRIPTION
TEMPLATE_PRODDESCRIPTION
TEMPLATE_PRODDESCRIPTION
TEMPLATE_PRODDESCRIPTION
TEMPLATE_PRODDESCRIPTION
TEMPLATE_PRODDESCRIPTION
TEMPLATE_PRODDESCRIPTION
TEMPLATE_PRODDESCRIPTION
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
The SeaWiFS instrument was launched by Orbital Sciences Corporation on the OrbView-2
(a.k.a. SeaStar) satellite in August 1997, and collected data from September 1997 until
the end of mission in December 2010. SeaWiFS had 8 spectral bands from 412 to 865 nm.
It collected global data at 4 km resolution, and local data (limited onboard storage
and direct broadcast) at 1 km. The mission and sensor were optimized for ocean color
measurements, with a local noon (descending) equator crossing time orbit, fore-and-aft
tilt capability, full dynamic range, and low polarization sensitivity.
This dataset represents multiple products archived at the Land Processes DAAC for ASTER (Advanced Spaceborne Thermal Emission and Reflection Radiometer) aboard the Terra satellite. This dataset is provided by NASA EOSDIS as a single point of entry for this suite of products. The provided access URL is link to EOSDIS's Earthdata Search tool with a pre-populated query that will bring up all products archived by EOSDIS with imagery provided by the ASTER instrument.
This dataset represents multiple products archived at the multiple archive centers for the MODIS (Moderate Resolution Imaging Spectroradiometer) instrument aboard the Aqua Satellite. This dataset is provided by NASA EOSDIS as a single point of entry for this suite of products. The provided access URL is link to EOSDIS's Earthdata Search tool with a pre-populated query that will bring up all products archived by EOSDIS with imagery provided by the MODIS instrument on Aqua.
This dataset represents multiple products archived at the multiple archive centers for the MODIS (Moderate Resolution Imaging Spectroradiometer) instrument aboard the Terra Satellite. This dataset is provided by NASA EOSDIS as a single point of entry for this suite of products. The provided access URL is link to EOSDIS's Earthdata Search tool with a pre-populated query that will bring up all products archived by EOSDIS with imagery provided by the MODIS instrument on Aqua.
EDI Redaction letter
Each agency is expected to post a JSON file for their Bureau IT Leadership Directory. Each dataset should include one record for each agency employee with the title of “chief information officer” or who performs the duties and responsibilities of a CIO but does not necessarily have the title of CIO.
Each agency is expected to post a JSON file for their CIO Governance Board Membership List.
CIO defines IT processes and policies. The CIO defines the development processes, milestones, review gates, and the overall policies for all capital planning, enterprise architecture, and project management and reporting for IT resources. At a minimum, these processes shall ensure that the CIO certifies that IT resources are adequately implementing incremental development (as defined in the below definitions). The CIO should ensure that such processes and policies address each category of IT resources appropriately—for example, it may not be appropriate to apply the same process or policy to highly customized mission-specific applications and back office enterprise IT systems depending on the agency environment.
The documents contained in this dataset reflect NASA's comprehensive IT policy in compliance with Federal Government laws and regulations.
The documents contained in this dataset reflect NASA's comprehensive IT policy in compliance with Federal Government laws and regulations.
The documents contained in this dataset reflect NASA's comprehensive IT policy in compliance with Federal Government laws and regulations.
The documents contained in this dataset reflect NASA's comprehensive IT policy in compliance with Federal Government laws and regulations.
The documents contained in this dataset reflect NASA's comprehensive IT policy in compliance with Federal Government laws and regulations.
The documents contained in this dataset reflect NASA's comprehensive IT policy in compliance with Federal Government laws and regulations.
The documents contained in this dataset reflect NASA's comprehensive IT policy in compliance with Federal Government laws and regulations.
The documents contained in this dataset reflect NASA's comprehensive IT policy in compliance with Federal Government laws and regulations.
The documents contained in this dataset reflect NASA's comprehensive IT policy in compliance with Federal Government laws and regulations.
Press kit for ISS mission Expedition 01 from 10/2000-03/2001. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 02 from 03/2001-08/2001. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 03 from 08/2001-12/2001. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 04 from 12/2001-06/2002. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 05 from 06/2002-12/2002. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 06 from 11/2002-05/2003. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 07 from 04/2003-10/2003. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 08 from 10/2003-04/2004. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 09 from 04/2004-10/2004. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 10 from 10/2004-04/2005. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 11 from 04/2005-10/2005. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 12 from 10/2005-04/2006. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 13 from 03/2006-09/2006. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 14 from 09/2006-04/2007. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 15 from 04/2007-10/2007. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 16 from 10/2007-04/2008. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 17 from 04/2008-10/2008. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 18 from 10/2008-04/2009. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 19 from 03/2009-05/2009. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 20 from 05/2009-10/2009. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 21/22 from 10/2009-03/2010. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 23 from 12/2009-09/2010. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 24 from 04/2010-11/2010. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 25 from 06/2010-03/2011. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 26 from 10/2010-05/2011. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 27 from 12/2010-09/2011. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 28 from 04/2011-11/2011. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 30 from 11/2011-07/2012. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 31 from 12/2011-07/2012. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 32 from 05/2012-09/2012. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 33 from 07/2012-11/2012. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 34 from 12/2012-03/2013. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 35 from 03/2013-09/2013. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 36 from 03/2013-09/2013. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 37 from 05/2013-11/2013. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 38 from 09/2013-03/2014. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 39 from 11/2013-05/2014. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 40 from 03/2014-11/2014. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 41 from 05/2014-11/2014. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 42 from 09/2014-03/2015. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
Press kit for ISS mission Expedition 43 from 11/2014-06/2015. Press kits contain information about each mission overview, crew, mission timeline, benefits, and media contact information.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2016.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2016.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2016.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2016.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2016.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2015.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2015.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2014.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2014.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2014.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2014.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2014.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2014.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2012.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2012.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2012.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2012.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2011.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2011.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2011.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2011.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2010.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2010.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2010.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2009.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2009.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2008.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2008.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2008.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2008.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2007.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2007.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2006.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2006.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2005.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2005.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2005.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2004.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2004.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2004.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2003.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2003.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2002.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2002.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2001.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2001.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 2000.
NASA Financial Budget Documents, Strategic Plans and Performance Reports for fiscal year 1999.
This Reel Includes the Following Sections TRT 50:10 Hurricane Overviews 1:02; Hurricane Arthur 15:07; Cyclone Pam 19:48; Typhoon Hagupit 21:27; Hurricane Bertha 22:03; Hurricanes Iselle and Julio 23:15; September 2014 Hurricane Alley 25:07; Satellite Beauty Passes 28:31; Hurricane Katrina 36:32; Global Portrait of Precipitation 42:00; Typhoon Halong 42:36; Typhoon Maysak 43:13; Superstorm Sandy 44:21; Hurricanes Fay and Gonzalo 45:29; RapidScat 46:12; CYGNSS 49:16 Super(s): NASA; Center Contact: Rob Gutro 301-286-4044; HQ Contact: Steve Cole 202-358-0918.
Eyes on the Solar System is a software package developed by NASA Jet Propulsion Laboratory and the California Institute of Technology using data provided by NASA's Navigation and Ancillary Information Facility (NAIR). Eyes on the Solar System is a 3-D environment full of real NASA mission data. Explore the cosmos from your computer. Hop on an asteroid. Fly with NASA's Voyager spacecraft. See the entire solar system moving in real time. It's up to you. You control space and time. Before choosing any of the modules below, this visualization tool requires a quick one-time download and install. Once downloaded, run the file to install. To download, see the attachment here.
The NASA Earth Exchange (NEX) Downscaled Climate Projections (NEX-DCP30) dataset is comprised of downscaled climate scenarios for the conterminous United States that are derived from the General Circulation Model (GCM) runs conducted under the Coupled Model Intercomparison Project Phase 5 (CMIP5) [Taylor et al. 2012] and across the four greenhouse gas emissions scenarios known as Representative Concentration Pathways (RCPs) [Meinshausen et al. 2011] developed for the Fifth Assessment Report of the Intergovernmental Panel on Climate Change (IPCC AR5). The dataset includes downscaled projections from 33 models, as well as ensemble statistics calculated for each RCP from all model runs available. The purpose of these datasets is to provide a set of high resolution, bias-corrected climate change projections that can be used to evaluate climate change impacts on processes that are sensitive to finer-scale climate gradients and the effects of local topography on climate conditions. Each of the climate projections includes monthly averaged maximum temperature, minimum temperature, and precipitation for the periods from 1950 through 2005 (Retrospective Run) and from 2006 to 2099 (Prospective Run).
The NASA Earth Exchange (NEX) Global Daily Downscaled Projections (NEX-GDDP) dataset is comprised of downscaled climate scenarios that are derived from the General Circulation Model (GCM) runs conducted under the Coupled Model Intercomparison Project Phase 5 (CMIP5) [Taylor et al. 2012] and across the two of the four greenhouse gas emissions scenarios known as Representative Concentration Pathways (RCPs) [Meinshausen et al. 2011] developed for the Fifth Assessment Report of the Intergovernmental Panel on Climate Change (IPCC AR5). The dataset is an ensemble of projections from 21 different models and two RCPs (RCP 4.5 and RCP 8.5), and provides daily estimates of maximum and minimum temperatures and precipitation using a daily Bias-Correction - Spatial Disaggregation (BCSD) method (Thrasher, et al., 2012). The data spans the entire globe with a 0.25 degree (~25-kilometer) spatial resolution for the periods from 1950 through 2005 (Historical) and from 2006 to 2100 (Climate Projections).
Global MODIS vegetation indices are designed to provide consistent spatial and temporal comparisons of vegetation conditions. Blue, red, and near-infrared reflectances, centered at 469-nanometers, 645-nanometers, and 858-nanometers, respectively, are used to determine the MODIS daily vegetation indices. The MODIS Normalized Difference Vegetation Index (NDVI) complements NOAA's Advanced Very High Resolution Radiometer (AVHRR) NDVI products and provides continuity for time series historical applications. MODIS also includes a new Enhanced Vegetation Index (EVI) that minimizes canopy background variations and maintains sensitivity over dense vegetation conditions. The EVI also uses the blue band to remove residual atmosphere contamination caused by smoke and sub-pixel thin cloud clouds. The MODIS NDVI and EVI products are computed from atmospherically corrected bi-directional surface reflectances that have been masked for water, clouds, heavy aerosols, and cloud shadows. Global MOD13Q1 data are provided every 16 days at 250-meter spatial resolution as a gridded level-3 product in the Sinusoidal projection. Lacking a 250m blue band, the EVI algorithm uses the 500m blue band to correct for residual atmospheric effects, with negligible spatial artifacts. Vegetation indices are used for global monitoring of vegetation conditions and are used in products displaying land cover and land cover changes. These data may be used as input for modeling global biogeochemical and hydrologic processes and global and regional climate. These data also may be used for characterizing land surface biophysical properties and processes, including primary production and land cover conversion.
In the past, the U.S. Geological Survey (USGS) and NASA collaborated on the creation of four global land data sets from Landsat images: one from the 1970s, and one each from circa 1990, 2000, and 2005. Each of these global data sets was created from the primary Landsat sensor in use at the time: the Multispectral Scanner (MSS) in the 1970s, the Thematic Mapper (TM) in 1990, Enhanced Thematic Mapper Plus (ETM+) in 2000, and a combination of TM and ETM+ in 2005.
ACCEPT consists of an overall software infrastructure framework and two main software components. The software infrastructure framework consists of code written to pre-process data, pass information between the two main software components, learn models that will be shared by nearly all of the elements in one of the two software components (which will require calling third party open source software modules), and select which element/method should be used in each one of the two main software components. The two main software components can use interchangeable software elements that enable the regression and detection functionality. Some software elements are distributed with the initial release, while others need to be called separately as independent third party elements that have been open sourced already.
BigView allows for interactive panning and zooming of images of arbitrary size on desktop PCs running linux. Additionally, it can work in a multi-screen environment where multiple PCs cooperate to view a single large image. Using this software, one can explore -- on relatively modest machines -- images such as the Mars Orbiter Camera mosaic [92160x33280 pixels].
Block GP is a Gaussian Process regression framework for multimodal data, that can be an order of magnitude more scalable than existing state-of-the-art nonlinear regression algorithms. The framework builds local Gaussian Processes on semantically meaningful partitions of the data and provides higher prediction accuracy than a single global model with very high confidence.
The CFD Utility Software Library consists of nearly 30 libraries of Fortran 90 and 77 subroutines and almost 100 applications built on those libraries. Many of the utilities apply to multiblock structured grids and flow solutions, but numerous other reusable modules in such categories as interpolation, optimization, quadrature, rapid searching, and character manipulation appear from several decades of software development in the Aerodynamics Division and Space Technology Division at NASA Ames Research Center.
CODE is a software framework for control and observation in distributed environments. The basic functionality of the framework allows a user to observe a distributed set of resources, services, and applications. A user can also use the framework to manage distributed resources, services, and applications.
The Crisis Mapping Toolkit (CMT) is a collection of tools for processing geospatial data (images, satellite data, etc.) into cartographic products that improve understanding of large-scale crises, such as natural disasters. The cartographic products produced by CMT include flood inundation maps, maps of damaged or destroyed structures, forest fire maps, population density estimates, etc. CMT is designed to rapidly process large-scale data using Google Earth Engine and other geospatial data systems.
The purpose of this Opensource forum is to promote the development of a JAVA based Application Programming Interface for the field of Mass Properties Engineering.
ECHO is a clearinghouse of Earth science Metadata under the EOS Program.
The Geometry Manipulation Protocol (GMP) is a library which serializes datatypes between XML and ANSI C data structures to support CFD applications. This library currently provides a description of geometric configurations, general moving-body scenarios (prescribed and/or 6-DOF), and control surface settings.
Growler is a C++-based distributed object and event architecture. It is written in C++, and supports serialization of C++ objects as part of its Remote Method Invocation, Event Channels, and in its Interface Definition Language. Its primary application has been in support of interactive, distributed visualization, computational steering, and concurrent visualization, but it is a general purpose system for distributed programming.
IND is applicable to most data sets consisting of independent instances, each described by a fixed length vector of attribute values. An attribute value may be a number, one of a set of attribute specific symbols, or omitted. One of the attributes is delegated the 'target' and IND grows trees to predict the target. Prediction can then be done on new data or the decision tree printed out for inspection.
The Execution Service allows users to submit, monitor, and cancel complex jobs. Each job consists of a set of tasks that perform actions such as executing applications and managing data. Each task is executed based on a starting condition that is an expression on the states of other tasks. This formulation allows tasks to be executed in parallel and also allows a user to specify tasks to execute when other tasks succeed, fail or are cancelled.
JavaGenes is a fairly general purpose evolutionary software system written in Java. It implements several versions of the genetic algorithm, simulated annealing, stochastic hill climbing and other search techniques. JavaGenes has been used to evolve molecules, atomic force field parameters, digital circuits, Earth Observing Satellite schedules, and antennas.
Libibvpp is a C++ wrapper around libibverbs, which is part of the OpenFabrics software suite (www.openfabrics.org).
Livingstone2 is a reusable artificial intelligence (AI) software system designed to assist spacecraft, life support systems, chemical plants or other complex systems in operating robustly with minimal human supervision, even in the face of hardware failures or unexpected events. Livingstone2 diagnoses the current state of the spacecraft or other system and recommends commands or repair actions that will allow the system to continue operations.
Mariana is an algorithm that efficiently optimizes the hyperparameters for Support Vector Machines for regression and classification.
The MST is a simulation framework, supporting the development of autonomy technology for planetary exploration vehicles. The MST provides a software test bed which includes simulated robotic platforms, sensors, and environments.
Mesh is a secure, lightweight grid middleware that is based on the addition of a single sign-on capability to the built-in public key authentication mechanism of SSH using system call interposition.
The Multiple Kernel Anomaly Detection (MKAD) algorithm is designed for anomaly detection over a set of files.
Multi-Fidelity Simulator, MFSim is a pluggable framework for creating an air traffic flow simulator at multiple levels of fidelity. The framework is designed to allow low-fidelity simulations of the entire US Airspace to be completed very quickly (on the order of seconds). The framework allows higher-fidelity plugins to be added to allow higher-fidelity simulations to occur in certain regions of the airspace concurrently with the low-fidelity simulation of the full airspace.
NodeMon is a resource utilization monitor tailored to the Altix architecture, but is applicable to any Linux system or cluster. It allows distributed resource monitoring via the Growler software infrastructure. It is modular, with existing modules for monitoring of cpu, memory, network, and numalink activity.
An optimal alarm system can robustly predict a level-crossing event that is specified over a fixed prediction horizon. The code contained in this packages provides the tools necessary to design an optimal alarm system for a simple stationary linear dynamic system driven by white Gaussian noise.
Pathdroid is a framework to analyze binary Android applications for program defects and malicious behaviors. Pathdroid is based on the Java Pathfinder (JPF) verification system (http://babelfish.arc.nasa.gov/trac/jpf), and thus provides model checking capabilities for applications that are distributed as standard Android .dex or .apk files.
Pour is a general-purpose information service framework designed to accommodate a wide variety of information types with support for high volume, low frequency periodic updates, user-specified updates, and automatic updates collected on-demand when needed. Information is stored exclusively in XML and retrieved using standard XPath queries over a single unified namespace independent of the information's source.
QuIP (QUick Image Processing) is an interpreter for image processing, graphics, psychophysical experimentation and general scientific computing.
The ROBUS-2 Protocol Processor (RPP) is a custom-designed hardware component implementing the functionality of the ROBUS-2 fault-tolerant communication system. The Reliable Optical Bus (ROBUS) is the core communication system of the Scalable Processor-Independent Design for Enhanced Reliability (SPIDER), a general-purpose fault-tolerant integrated modular architecture currently under development at NASA Langley Research Center. ROBUS is a time-division multiple access (TDMA) broadcast communication system with medium access control by means of time-indexed communication schedule. ROBUS-2 is a developmental version of the ROBUS providing guaranteed fault-tolerant services to the attached processing elements (PEs), in the presence of a bounded number of faults.
The sequenceMiner was developed to address the problem of detecting and describing anomalies in large sets of high-dimensional symbol sequences. sequenceMiner works by performing unsupervised clustering (grouping) of sequences using the normalized longest common subsequence (LCS) as a similarity measure, followed by a detailed analysis of outliers to detect anomalies. sequenceMiner utilizes a new hybrid algorithm for computing the LCS that has been shown to outperform existing algorithms by a factor of five. sequenceMiner also includes new algorithms for outlier analysis that provide comprehensible indicators as to why a particular sequence was deemed to be an outlier. This provides analysts with a coherent description of the anomalies identified in the sequence, and why they differ from more 'normal' sequences.
Shift is a lightweight framework for high performance local and remote file transfers that provides resiliency across a wide variety of failure scenarios through various techniques. These include end-to-end integrity via cryptographic hashes, throttling of transfers to prevent resource exhaustion, balancing transfers across resources based on load and availability, and parallelization of transfers across multiple source and destination hosts for increased redundancy and performance.
SLAB is a software-based, real-time virtual acoustic environment rendering system being developed as a tool for the study of spatial hearing. SLAB is designed to work in the personal computer environment to take advantage of the low-cost PC platform while providing a flexible, maintainable, and extensible architecture to enable the quick development of experiments. The software provides an API (Application Programming Interface) for specifying the acoustic scene as well as an extensible architecture for exploring multiple rendering strategies.
Surfer is an extensible framework designed to select and rank grid resources where a resource is defined to be anything that may need selecting such as compute resources, storage resources, data resources, etc.
Swim is a software information service for the grid built on top of Pour, which is an information service framework developed at NASA. Swim provides true software resource discovery integrated with the tools used by administrators to install software.
IKOS is a C++ library designed to facilitate the development of sound static analyzers based on Abstract Interpretation. Specialization of a static analyzer for an application or family of applications is critical for achieving both precision and scalability. Developing such an analyzer is arduous and requires significant expertise in Abstract Interpretation.
The X-Plane Communications Toolbox (XPC) is an open source research tool used to interact with the commercial flight simulator software X-Plane. XPC allows users to control aircraft and receive state information from aircraft simulated in X-Plane using functions written in C or MATLAB in real time over the network. This research tool has been used to visualize flight paths, test control algorithms, simulate an active airspace, or generate out-the-window visuals for in-house flight simulation software.
ROC (Receiver Operating Characteristic) curve Code Augmentation was written by Rodney Martin and John Stutz at NASA Ames Research Center and is a modification of ROC Curve code originally authored by G.C. Cawley that provides additional functionality. The inclusion of more detailed bookkeeping of new and existing internal data structures that provide more visibility into various performance measures is one of the new features.
Save is a framework for implementing highly available network-accessible services. Save consists of a command-line utility and a small set of extensions for the existing Mon monitoring utility. Mon is a flexible command scheduler that has the ability to take various actions (called 'alerts') depending on the exit conditions of the periodic commands (called 'monitors') it executes. Save provides a set of monitors and alerts that execute within the Mon scheduler.
Mutil provides mcp and msum, which are drop-in replacements for cp and md5sum that utilize multiple types of parallelism to achieve maximum copy and checksum performance on clustered file systems.
The purpose of this set of maps is to provide an up-to-date source showing the locations of Mercury surface feature names approved by the International Astronomical Union (IAU).
Magellan imagery of Venus approved by the International Astronomical Union (IAU).
This set of maps diplays altimetric radar images of Venus approved by the International Astronomical Union (IAU).
This set of maps diplays altimetric radar images of Venus approved by the International Astronomical Union (IAU).
This set of maps diplays altimetric radar images of Venus approved by the International Astronomical Union (IAU).
This set of maps diplays altimetric radar images of Venus approved by the International Astronomical Union (IAU).
This set of maps diplays altimetric radar images of Venus approved by the International Astronomical Union (IAU).
This set of maps diplays altimetric radar images of Venus approved by the International Astronomical Union (IAU).
This set of maps diplays altimetric radar images of Venus approved by the International Astronomical Union (IAU).
This set of maps diplays altimetric radar images of Venus approved by the International Astronomical Union (IAU).
The purpose of the lunar maps is to provide an up-to-date and comprehensive depiction on lunar nomenclature approved by the International Astronomical Union (IAU).
These lunar maps display the four different areas of the moon with color-coded topography in low and high resolution approved by the International Astronomical Union (IAU).
These lunar maps display the four different areas of the moon with color-coded topography in low and high resolution approved by the International Astronomical Union (IAU).
These lunar maps display the four different areas of the moon with color-coded topography in low and high resolution approved by the International Astronomical Union (IAU).
These lunar maps display the four different areas of the moon with color-coded topography in low and high resolution approved by the International Astronomical Union (IAU).
THEMIS imagery of Mars approved by the International Astronomical Union (IAU).
These maps display regional feature names and boundaries of regional features of Mars approved by the International Astronomical Union (IAU).
These images display the two moons of Mars: Deimos and Phobos - with HRSC images and shaded relief images with cylindrical and hemispherical views approved by the International Astronomical Union (IAU).
These images display the two moons of Mars: Deimos and Phobos - with HRSC images and shaded relief images with cylindrical and hemispherical views approved by the International Astronomical Union (IAU).
These images display asteriods documented and approved by the International Astronomical Union (IAU).
These images display asteriods documented and approved by the International Astronomical Union (IAU).
These images display asteriods documented and approved by the International Astronomical Union (IAU).
These images display asteriods documented and approved by the International Astronomical Union (IAU).
These images display asteriods documented and approved by the International Astronomical Union (IAU).
These images display asteriods documented and approved by the International Astronomical Union (IAU).
These images display asteriods documented and approved by the International Astronomical Union (IAU).
These images display asteriods documented and approved by the International Astronomical Union (IAU).
These images display asteriods documented and approved by the International Astronomical Union (IAU).
These images display asteriods documented and approved by the International Astronomical Union (IAU).
These images display asteriods documented and approved by the International Astronomical Union (IAU).
These images display several of Jupiter's moons approved by the International Astronomical Union (IAU).
These images display several of Jupiter's moons approved by the International Astronomical Union (IAU).
These images display several of Jupiter's moons approved by the International Astronomical Union (IAU).
These images display several of Jupiter's moons approved by the International Astronomical Union (IAU).
These images display several of Jupiter's moons approved by the International Astronomical Union (IAU).
These images display several of Jupiter's moons approved by the International Astronomical Union (IAU).
These images display several of Saturn's moons approved by the International Astronomical Union (IAU).
These images display several of Saturn's moons approved by the International Astronomical Union (IAU).
These images display several of Saturn's moons approved by the International Astronomical Union (IAU).
These images display several of Saturn's moons approved by the International Astronomical Union (IAU).
These images display several of Saturn's moons approved by the International Astronomical Union (IAU).
These images display several of Saturn's moons approved by the International Astronomical Union (IAU).
These images display several of Saturn's moons approved by the International Astronomical Union (IAU).
These images display several of Saturn's moons approved by the International Astronomical Union (IAU).
These images display several of Saturn's moons approved by the International Astronomical Union (IAU).
These images display several of Saturn's moons approved by the International Astronomical Union (IAU).
These images display several of Saturn's moons approved by the International Astronomical Union (IAU).
These images display several of Uranus's moons approved by the International Astronomical Union (IAU).
These images display several of Uranus's moons approved by the International Astronomical Union (IAU).
These images display several of Uranus's moons approved by the International Astronomical Union (IAU).
These images display several of Uranus's moons approved by the International Astronomical Union (IAU).
These images display several of Neptune's moons approved by the International Astronomical Union (IAU).
These images display several of Neptune's moons approved by the International Astronomical Union (IAU).
This interactive multimedia timeline traces the search for extrasolar planets, from ancient philosophical speculation to modern discoveries.
Use this search engine to generate custom tables of orbital and/or physical parameters for all asteroids and comets (or a specified sub-set) in our small-body database. If this is your first time here, you may find it helpful to read our tutorial. Otherwise, simply follow the steps in each section: 'Search Constraints', 'Output Fields', and finally 'Format Options'. If you want details for a single object, use the Small Body Browser instead.
The JPL Small-Body Database Browser provides data for all known asteroids and many comets. Newly discovered objects and their orbits are added on a daily basis. Discovery circumstances are updated on a roughly monthly interval. Physical parameters, other than magnitude parameters, are updated on a less frequent basis.
This list of potential mission targets should not be interpreted as a complete list of viable NEAs for an actual human exploration mission. As the NEA orbits are updated, the viable mission targets and their mission parameters will change. To select an actual target and mission scenario, additional constraints must be applied including astronaut health and safety considerations, human space flight architecture elements, their performances and readiness, the physical nature of the target NEA and mission schedule constraints.
Walking to Olympus:  An EVA Chronology chronicles the 154 EVAs conducted from March 1965 to April 1997. It is intended to make clear the crucial role played by EVA in the history of spaceflight, as well as to chronicle the large body of EVA lessons learned.
The Scientific Visualization Studio hosts a collection of media galleries on Earth, air, and space themes.
The Earth Observatory is part of the EOS Project Science Office located at NASA Goddard Space Flight Center.
The Earth Resources Observation and Science (EROS) Center manages this collection of Landsat 7 scenes created for aesthetic purposes rather than scientific interpretation.
The Earth Resources Observation and Science (EROS) Center manages this collection of forty-five new scenes developed for their aesthetic beauty, rather than for scientific value. The artists of this collection come from three sensors aboard satellites orbiting the Earth - Landsat 7, ASTER, and MODIS.
The Earth Resources Observation and Science (EROS) Center manages the Earth as Art Three exhibit, which provides fresh and inspiring glimpses of different parts of our planet's complex surface.
The Earth Resources Observation and Science (EROS) Center manages the this image of the week gallery.
The Earth Resources Observation and Science (EROS) Center manages the this gallery of images of the 50 U.S. states plus Puerto Rico as derived by Landsat data.
The Earth Resources Observation and Science (EROS) Center manages the this gallery of images of the 50 U.S. states as derived by Landsat data.
The Earth Resources Observation and Science (EROS) Center manages the this gallery of Landsat-derived images of one of the most remarkable and productive scientific explorations in American history. The Corps of Discovery expedition crossed the territory of the newly acquired but uncharted Louisiana Purchase.
NASA Policy Directive: NASA IT Policy on the management of NASA scientific and technical information.
NASA records management program requirements.
NASA spaceflight program and project management requirements.
A fully queryable REST API with JSON, XML, and CSV output as well as inline, runable examples using data from the transcriptional profiling and phenotypic characterization of the major human opportunistic fungal pathogen, Candida albicans, grown in spaceflight conditions.
A fully queryable REST API with JSON, XML, and CSV output as well as inline, runable examples. This is a monitor using data from Swift/BAT, MAXI and Fermi/GBM instruments.
The CO2 Virtual Data Environment is a comprehensive effort at bringing together the models, data, and tools necessary to perform research on atmospheric CO2.This site presents web-based discovery and access resources designed to streamline the process of accessing relevant global and regional carbon dioxide data sets. Furthermore, this site provides tools for conversion, manipulation, and transformation of the data to facilitate research.
A fully queryable REST API with JSON, XML, and CSV output as well as inline, runable examples using data from the transcriptional profiling and phenotypic characterization of the major human opportunistic fungal pathogen, Candida albicans, grown in spaceflight conditions.
A RESTful web service for querying data and metadata components from data sets, including instruments, observatories, and inventory.
Activities done by an astronaut or cosmonaut outside a spacecraft beyond the Earth's appreciable atmosphere.
API using chronological data summary of fireball and bolide events provided by U.S. Government sensors.
API using Global Imagery Browse Services (GIBS) designed to deliver global, full-resolution satellite imagery to users in a highly responsive manner, enabling interactive exploration of the Earth.
The Heliocentric Trajectories Web services allow a software developer to use portions of the HelioWeb software in their own application.
The Helioviewer Project maintains a set of Public APIs with the goal of improving access to solar and heliospheric datasets to scientists, educators, developers, and the general public.
The {MAAS} API is an open source REST API built to help make it easier and more efficient to build interactive applications that want to utilize the wealth of weather data being transmitted by the Curiosity Rover on Mars. Our API is built upon the REMS (Rover Environmental Monitoring Station) data provided by the Centro de Astrobiologia (CSIC-INTA).
MODAPS Web Services API for LANCE-MODIS. This Application Programming Interface (API) encompasses a library of functions that provides programmatic data access to MODIS near-real-time data products. These routines enable both SOAP and REST based web service calls against the LANCE-MODIS near-real-time data archives. These routines mirror existing LAADS Web services.
The MODIS Web service provides users with subsets of MODIS Land Products through standards based SOAP (Simple Object Access Protocol) Web service.
API using comprehensive data set from The Meteoritical Society that contains information on all of the known meteorite landings.
API of NASA facilities.
API of NASA held and pending patents.
World Wind is a collection of components that interactively display 3D geographic information within Java applications or applets.
This API uses data from heliocentric ecliptic orbital elements for 170 NECs (Near-Earth Comets) sorted by object number/name.
This dataset lists out all software in use by NASA.
This API uses data from the Planetary Data System (PDS).
PO.DAAC provides several ways to discover and access physical oceanography data, from the PO.DAAC Web Portal to FTP access to front-end user interfaces (see http://podaac.jpl.nasa.gov).  That same data can also be discovered and accessed through PO.DAAC Web Services, enabling efficient machine-to-machine communication and data transfers.
PO.DAAC provides several ways to discover and access physical oceanography data, from the PO.DAAC Web Portal to FTP access to front-end user interfaces (see http://podaac.jpl.nasa.gov).  That same data can also be discovered and accessed through PO.DAAC Web Services, enabling efficient machine-to-machine communication and data transfers. Extract service subsets a granule in PO.DAAC catalog and produces either netcdf3 or hdf4 files.
PO.DAAC provides several ways to discover and access physical oceanography data, from the PO.DAAC Web Portal to FTP access to front-end user interfaces (see http://podaac.jpl.nasa.gov).  That same data can also be discovered and accessed through PO.DAAC Web Services, enabling efficient machine-to-machine communication and data transfers. Granule metadata service Retrieves the metadata of a granule(s) in PO.DAAC's catalog.
PO.DAAC provides several ways to discover and access physical oceanography data, from the PO.DAAC Web Portal to FTP access to front-end user interfaces (see http://podaac.jpl.nasa.gov).  That same data can also be discovered and accessed through PO.DAAC Web Services, enabling efficient machine-to-machine communication and data transfers. The PODAAC Image service renders granules in the PO.DAAC's catalog to images such as jpeg and/or png.
PO.DAAC provides several ways to discover and access physical oceanography data, from the PO.DAAC Web Portal to FTP access to front-end user interfaces (see http://podaac.jpl.nasa.gov).  That same data can also be discovered and accessed through PO.DAAC Web Services, enabling efficient machine-to-machine communication and data transfers. Dataset Search service searches PO.DAAC's dataset catalog.
PO.DAAC provides several ways to discover and access physical oceanography data, from the PO.DAAC Web Portal to FTP access to front-end user interfaces (see http://podaac.jpl.nasa.gov).  That same data can also be discovered and accessed through PO.DAAC Web Services, enabling efficient machine-to-machine communication and data transfers. Dataset Search service searches PO.DAAC's dataset catalog.
PO.DAAC provides several ways to discover and access physical oceanography data, from the PO.DAAC Web Portal to FTP access to front-end user interfaces (see http://podaac.jpl.nasa.gov). That same data can also be discovered and accessed through PO.DAAC Web Services, enabling efficient machine-to-machine communication and data transfers.
We are developing a set of NASA Extensions to the Google Maps API—and soon to other frameworks such as OpenLayers as well—that will make these platforms more useful to NASA scientists and our colleagues elsewhere.
A fully queryable REST API with JSON, XML, and CSV output as well as inline, runable examples using data from the transcriptional profiling and phenotypic characterization of the major human opportunistic fungal pathogen, Candida albicans, grown in spaceflight conditions.
This API allows any Web application to offer an interactive 4D display of the trajectories of satellites known to SSC.
The Satellite Situation Center (SSC) web services allow a software developer to use portions of the SSC software in their own applications. SSC is a system to cast geocentric spacecraft location information into a framework of (empirical) geophysical regions and mappings of spacecraft locations along lines of the Earth’s magnetic field. This capability is one key to mission science planning (both single missions and coordinated observations of multiple spacecraft with ground-based investigations) and to subsequent multi-mission data analysis.
This API uses data that show discovery statistics for NEAs and comets discovered by NASA's WISE mission - now renamed to NEOWISE.
The OMB Office of the Chief Information Officer (OFCIO) has a long-standing practice of making information about Federal IT available to the public through various tools and reports to Congress. Consistent with this practice, OMB OFCIO will be making agency cost savings and avoidances data available to the public via http://www.whitehouse.gov/omb/e-gov. This dataset links to NASA's Realized Cost Savings and Avoidances data in JSON format.
This endpoint structures the APOD imagery and associated metadata so that it can be repurposed for other applications. In addition, if the concept_tags parameter is set to True, then keywords derived from the image explanation are returned. These keywords could be used as auto-generated hashtags for twitter or instagram feeds; but generally help with discoverability of relevant imagery.
The Early Detection Research Network (EDRN) runs a distributed service known as the EDRN Resource Network Exchange (ERNE). ERNE is a virtual specimen bank. It unifies participating sites specimen databases using both classic OODT and Agile OODT.
The API is powered by Google Earth Engine, and currently only supports pan-sharpened Landsat 8 imagery.
The NASA TechPort system provides a RESTful web services API to make technology project data available in a machine-readable format. This API can be used to export TechPort data into an XML format, which can then be further processed and analyzed.
NASA has released a series of space sounds via sound cloud. We have abstracted away some of the hassle in accessing these sounds, so that developers can play with the audio files.
NeoWs (Near Earth Object Web Service) is a RESTful web service for near earth Asteroid information. With NeoWs a user can: search for Asteroids based on their closest approach date to Earth, lookup a specific Asteroid with its NASA JPL small body id, as well as browse the overall data-set.
This API is designed to collect image data gathered by NASA's Curiosity, Opportunity, and Spirit rovers on Mars and make it more easily available to other developers, educators, and citizen scientists.
This table contains precise epoch 2000 coordinates and cross-identifications to sources in the 2MASS Point Source Catalog for nearly all stars in the Gliese, Gliese-Jahreiss, and Woolley catalogs of nearby stars. The only Gliese objects where the authors were not successful are two Gliese sources that are actually QSOs; two proposed companions to brighter stars, which they believe do not exist; four stars included in one of the catalogs but identified there as only optical companions; one probable plate flaw; and two stars that simply remain unrecovered. For the 4251 recovered stars, 2693 have coordinates based on Hipparcos positions, 1549 have coordinates based on 2MASS data, and 9 have positions from other astrometric sources. All positions have been calculated at epoch 2000 using proper motions from the literature.
SAOImage DS9 is an astronomical imaging and data visualization application. DS9 supports FITS images and binary tables, multiple frame buffers, region manipulation, and many scale algorithms and colormaps. It provides for easy communication with external analysis tasks and is highly configurable and extensible via XPA and SAMP.
The NASA website features a schedule for upcoming spacecraft launches, including ISS resupply missions.
The NASA LSP website features a history of past spacecraft launches, going back to the launch of the Deep Space 1 mission to present.
A list of launch vehicles launched for NASA missions in 2015.
A list of launch vehicles launched for NASA missions in 2014.
A list of launch vehicles launched for NASA missions in 2013.
A list of launch vehicles launched for NASA missions in 2012.
A list of launch vehicles launched for NASA missions in 2011.
A list of launch vehicles launched for NASA missions in 2010.
A list of launch vehicles launched for NASA missions in 2009.
A list of launch vehicles launched for NASA missions in 2008.
A list of launch vehicles launched for NASA missions in 2007.
A list of launch vehicles launched for NASA missions in 2006.
A list of launch vehicles launched for NASA missions in 2005.
A list of launch vehicles launched for NASA missions in 2004.
A list of launch vehicles launched for NASA missions in 2003.
A list of launch vehicles launched for NASA missions in 2002.
A list of launch vehicles launched for NASA missions in 2001.
A list of launch vehicles launched for NASA missions in 2000.
A list of launch vehicles launched for NASA missions in 1999.
We present a set of novel algorithms which we call sequenceMiner, that detect and characterize anomalies in large sets of high-dimensional symbol sequences that arise from recordings of switch sensors in the cockpits of commercial airliners. While the algorithms we present are general and domain-independent, we focus on a specific
problem that is critical to determining system-wide health
of a fleet of aircraft. The approach taken uses unsupervised clustering of sequences using the normalized length of he longest common subsequence (nLCS) as a similarity measure, followed by a detailed analysis of outliers to detect anomalies. In this method, an outlier sequence is defined as a sequence that is far away from a cluster. We present new algorithms for outlier analysis that provide comprehensible indicators as to why a particular sequence is deemed to be an outlier. The algorithm provides a coherent description to an analyst of the anomalies in the sequence when compared to more normal sequences.

The final section of the paper demonstrates the effectiveness of sequenceMiner for anomaly detection on a real set of discrete sequence data from a fleet of commercial airliners.


We show that sequenceMiner discovers actionable and
operationally significant safety events. We also compare
our innovations with standard HiddenMarkov Models, and
show that our methods are superior
Many existing complex space systems have a significant
amount of historical maintenance and problem data
bases that are stored in unstructured text forms. The problem that we address in this paper is the discovery of recurring anomalies and relationships between problem reports that may indicate larger systemic problems. We will illustrate our techniques on data from discrepancy reports regarding software anomalies in the Space Shuttle. These free text reports are written by a number of different people, thus the emphasis and wording vary considerably.

With Mehran Sahami from Stanford University, I'm putting together a  book on text mining called "Text Mining: Theory and Applications" to be published by Taylor and Francis.
Here are some results from the Spectra Decomposition Algorithm on infrared spectral images of Saturn's moon Enceladus.

 

Figure 1  is the spatial contribution of the 2nd component. Notice the hot spot in red around the bottom left hand side. The hot spot correspond to a higher contribution of this component located at the "tiger scratch" features on the moon.

 

Figure 2  is the spectral component, which exhibits a pattern that indicates absorption of light due to the presence of CO2.
Electrical power systems play a critical role in spacecraft and aircraft. This paper discusses our development of a diagnostic capability for an electrical power system testbed, ADAPT, using probabilistic techniques. In the context of ADAPT, we present two challenges, regarding modelling and real-time performance, often encountered in real-world diagnostic applications. To meet the modelling challenge, we discuss our novel high-level specification language which supports auto-generation of Bayesian networks. To meet the real-time challenge, we compile Bayesian networks into arithmetic circuits.  Arithmetic circuits typically have small footprints and are optimized for the real-time avionics systems found in spacecraft and aircraft. Using our approach, we present how Bayesian networks with over 400 nodes are auto-generated and then compiled into arithmetic circuits. Using real-world data from ADAPT as well as simulated data, we obtain average inference times smaller than one millisecond when computing diagnostic queries using arithmetic circuits that model our real-world electrical power system.

Reference:

 O. J. Mengshoel, A. Darwiche, K. Cascio, M. Chavira, S. Poll, and S. Uckun, “Diagnosing Faults in Electrical Power Systems of Spacecraft and Aircraft”, In Proc. of the Twentieth Innovative Applications of Artificial Intelligence, Conference (IAAI-08), Chicago, IL, 2008.

BibTex Reference:  

 @inproceedings{mengshoel08diagnosing,
  author    = {Mengshoel, O. J. and Darwiche, A. and Cascio, K. and Chavira, M. and Poll, S. and Uckun, S.},
  title     = {Diagnosing Faults in Electrical Power Systems of Spacecraft and Aircraft},
  booktitle     = {Proceedings of the Twentieth Innovative Applications of Artificial Intelligence
                      Conference (IAAI-08)},
  pages = {1699--1705},
  address = {Chicago, IL},
  year      = {2008}
}
One of NASA’s key mission requirements is robust state estimation.  Sensing, using a wide range of sensors and sensor fusion approaches, plays a central role in robust state estimation, and there is a need to diagnose sensor failure as well as component failure.   Sensor validation techniques address this problem: given a vector of sensor readings, decide whether sensors have failed, therefore producing bad data.  We take in this paper a probabilistic approach, using Bayesian networks, to diagnosis and sensor validation, and investigate several relevant but slightly different Bayesian network queries. We emphasize that on-board inference can be performed on a compiled model, giving fast and predictable execution times. Our results are illustrated using an electrical power system, and we show that a Bayesian network with over 400 nodes can be compiled into an arithmetic circuit that can correctly answer queries in less than 500 microseconds on average.

Reference:

O. J. Mengshoel, A. Darwiche, and S. Uckun, "Sensor Validation using Bayesian Networks." In Proc. of the 9th International Symposium on Artificial Intelligence, Robotics, and Automation in Space (iSAIRAS-08), Los Angeles, CA, 2008.

BibTex Reference:

@inproceedings{mengshoel08sensor,
  author    = {Mengshoel, O. J. and Darwiche, A. and Uckun, S.},
  title     = {Sensor Validation using {Bayesian} Networks},
  booktitle     = {Proceedings of the 9th International Symposium on Artificial Intelligence, Robotics, and Automation in Space (iSAIRAS-08)},
  year      = {2008}
}
Our primary goal is to automatically analyze textual reports from the Aviation Safety Reporting System (ASRS) database to detect/discover the anomaly categories reported by the pilots, and to assign each report to the appropriate category/categories. We have used two state-of-the-art models for text analysis: (i) mixture of von Mises Fisher (movMF) distributions, and (ii) latent Dirichlet allocation (LDA) on a subset of all ASRS reports. The models achieve a reasonably high performance in discovering anomaly categories and clustering reports. Each category is represented by the most representative words with the highest probability in this category. In addition, since the inference algorithm for LDA was somewhat slow, we have developed a new fast LDA algorithm which is 5-10 times more efficient than the original one, therefore more applicable for the practical use. Further, we have developed a simple visualization tool based on non-linear manifold embedding (ISOMAP) to generate a 2-d visual representation of each report based on its content/topics, which gives a direct view of the structure of the whole dataset as well as the outliers.
Distributed data mining from privacy-sensitive multi-party data is likely to play an important role in the next generation of integrated vehicle health monitoring systems. For example, consider an airline manufacturer [tex]$\mathcal{C}$[/tex] manufacturing an aircraft model [tex]$A$[/tex] and selling it to five different airline operating companies [tex]$\mathcal{V}_1 \dots \mathcal{V}_5$[/tex]. These aircrafts, during their operation, generate huge amount of data. Mining this data can reveal useful information regarding the health and operability of the aircraft which can be useful for disaster management and prediction of efficient operating regimes. Now if the manufacturer [tex]$\mathcal{C}$[/tex] wants to analyze the performance data collected from different aircrafts of model-type [tex]$A$[/tex] belonging to different airlines then central collection of data for subsequent analysis may not be an option. It should be noted that the result of this analysis may be statistically more significant if the data for aircraft model [tex]$A$[/tex] across all companies were available to [tex]$\mathcal{C}$[/tex]. The potential problems arising out of such a data mining scenario are:
It is becoming increasingly clear that the next generation of web search and advertising will rely on a deeper understanding of user intent and task modeling, and a correspondingly richer interpretation of content on the web. How we get there, in particular, how we understand web content in richer terms than bags of words and links, is a wide open and fascinating question. I will discuss some of the options here, and look closely at the role that information extraction can play.

**Speaker Bio**

Raghu Ramakrishnan is Chief Scientist for Audience and Cloud Computing at Yahoo!, and is a Research Fellow, heading the Community Systems area in Yahoo! Research. He was Professor of Computer Sciences at the University of Wisconsin-Madison, and was founder and CTO of QUIQ, a company that pioneered question-answering communities, powering Ask Jeeves' AnswerPoint as well as customer-support for companies such as Compaq. His research has influenced query optimization in commercial database systems, and the design of window functions in SQL:1999. His paper on the Birch clustering algorithm received the SIGMOD 10-Year Test-of-Time award, and he has written the widely-used text "Database Management Systems" (with Johannes Gehrke).

He is Chair of ACM SIGMOD, on the Board of Directors of ACM SIGKDD and the Board of Trustees of the VLDB Endowment, and has served as editor-in-chief of the Journal of Data Mining and Knowledge Discovery, associate editor of ACM Transactions on Database Systems, and the Database area editor of the Journal of Logic Programming. Ramakrishnan is a Fellow of the Association for Computing Machinery (ACM) and the Institute of Electrical and Electronics Engineers (IEEE), and has received several awards, including a Distinguished Alumnus Award from IIT Madras, a Packard Foundation Fellowship in Science and Engineering, an NSF Presidential Young Investigator Award, and an ACM SIGMOD Contributions Award.
The land remote sensing community has a long history of using supervised and unsupervised methods to help interpret and analyze remote sensing data sets. Until relatively recently, most remote sensing studies have used fairly conventional image processing and pattern recognition methodologies. In the past decade, NASA has launched a series of remote sensing missions known as the Earth Observing System (EOS). The data sets acquired by EOS instruments provide an extremely rich source of information related to the properties and dynamics of the Earth’s terrestrial ecosystems. However, these data are also characterized by large volumes and complex spectral, spatial and temporal attributes. Because of the volume and complexity of EOS data sets, efficient and effective analysis of them presents significant challenges that are difficult to address using conventional remote sensing approaches. In this paper we discuss results from applying a variety of different data mining approaches to global remote sensing data sets. Specifically, we describe three main problem domains and sets of analyses: (1) supervised classification of global land cover from using data from NASA’s Moderate Resolution Imaging Spectroradiometer; (2) the use of linear and non-linear cluster and dimensionality reduction methods to examine coupled climate-vegetation dynamics using a twenty year time series of data from the Advanced Very High Resolution Radiometer; and (3) the use of functional models, non-parametric clustering, and mixture models to help interpret and understand the feature space and class structure of high dimensional remote sensing data sets. The paper will not focus on specific details of algorithms. Instead we describe key results, successes, and lessons learned from ten years of research focusing on the use of data mining and machine learning methods for remote sensing and Earth science problems.
Follow the link below to see a current version of NASA's Integrated Vehicle Health Management Project Plan:

 

www.aeronautics.nasa.gov/nra_pdf/ivhm_tech_plan_c1.pdf
In clique tree clustering, inference consists of propagation in a clique tree compiled from a Bayesian network. In this paper, we develop an analytical approach to characterizing clique tree growth as a function of increasing Bayesian network connectedness, specifically: (i) the expected number of moral edges in their moral graphs or (ii) the ratio of the number of non-root nodes to the number of root nodes.  In experiments, we systematically increase the connectivity of bipartite Bayesian networks, and find that clique tree size growth is well-approximated by Gompertz growth curves.  This research improves the understanding of the scaling behavior of clique tree clustering, provides a foundation for benchmarking and developing improved BN inference algorithms, and presents an aid for analytical trade-off studies of tree clustering using growth curves.

**Reference:**

O. J. Mengshoel, "Macroscopic Models of Clique Tree Growth for Bayesian Networks."  In Proc. of the 22nd National Conference on Artificial Intelligence (AAAI-07). July 2007, Vancouver, Canada, pp. 1256-1262.

**BibTex Reference:**

@inproceedings{mengshoel07macroscopic,
    author = "Mengshoel, O. J.",
    title = "Macroscopic Models of Clique Tree Growth for {Bayesian} Networks",
        year = "2007",
  booktitle = {Proceedings of the Twenty-Second National Conference on Artificial Intelligence (AAAI-07)},
  pages = "1256-1262",
  address = "Vancouver, British Columbia"
}
In this work we are concerned with the conceptual design of large-scale diagnostic and health management systems that use Bayesian networks. While they are potentially powerful, improperly designed Bayesian networks can result in too high memory requirements or too long inference times, to they point where they may not be acceptable for real-time diagnosis and health management in resource-bounded systems such as NASA's aerospace vehicles. We investigate the clique tree clustering approach to Bayesian network inference, where increasing the size and connectivity of a Bayesian network typically also increases clique tree size. This paper combines techniques for analytically characterizing clique tree growth with bounds on clique tree size imposed by resource constraints, thereby aiding the design and optimization of large-scale Bayesian networks in resource-bounded systems. We provide both theoretical and experimental results, and illustrate our approach using a NASA case study.

**Reference:**

O. J. Mengshoel, “Designing Resource-Bounded Reasoners using Bayesian Networks: System Health Monitoring and Diagnosis”, In Proc. of the 18th International Workshop on Principles of Diagnosis (DX-07), Nashville, TN, May 2007.

**BibTex Reference:**

@inproceedings{mengshoel07designing,
    author = "Mengshoel, O. J.",
    title = "Designing Resource-Bounded Reasoners using {Bayesian} Networks: System Health Monitoring and Diagnosis",
    booktitle = {Proceedings of the 18th International Workshop on Principles of Diagnosis (DX-07)},
    year = {2007},
    pages     = {330--337},
    address = {Nashville, TN},
}
The Joint Army Navy NASA Air Force Modeling and Simulation Subcommittee's Integrated Health Management panel was started about 6 years ago to help foster communication and collaboration in health management related issues for liquid and solid rocket propulsion systems.  The panel is co-chaired by Mr. Scott Hyde (ATK) and Ashok N. Srivastava, Ph.D. (NASA).

In order to have a common langauge for health management, we need to have a common set of definitions.  We have attached a MS Excel spreadsheet that covers the many terms that are of interest to us in the field.

Please take a look at the definitions and provide comments and additional terms (with or without definitions) using the feedback box below.  We will compile all the definitions into a master list for submittal to the Modeling and Simulation Subcommittee.
Aviation safety systems have undergone dramatic changes over the past fifty years.  If you take a look at the early technology in this area, you'll see that there was a lot of work done in the area of so-called 'built-in-testing' (BIT) which essentially tests connectivity between different components.

 

Technology has moved forward very far since that time.  With the massive storage systems and advanced sensors and other communications systems, we are now able to capture and store vast quantities of health and control related data.  This data is usually stored off-line for future analysis.  In many cases, we also have an abundance of human-written text reports that relate to known safety issues.  A key problem is to 'look' across all these data sources in order to find precursors to safety events.  Although humans do look at many aspects of the data, it is difficult, if not impossible for them to integrate all the information available in a meaningful way. 

 


Other industries face this glut of data in their own way.  Businesses have invested heavily in business intelligence products based on data mining that are designed to convert data into actionable information to maximize their profits or other metrics.  The IVHM project is investing in data mining technologies to help sift through these massive data sets to uncover actionable information from a safety perspective.  I've attached a presentation that Irv Statler and I gave at NASA HQ on this subject during an Aeronautics Technical Seminar. A video of the talk is also included.  It's about 90 minutes long, so grab some popcorn.  :)
One of the key problems that arises in many areas is to estimate a potentially nonlinear function [tex] G(x, \theta)[/tex] given input and output samples [tex] ( X,y ) [/tex] so that [tex]y approx G(x, \theta)[/tex].


There are many approaches to addressing this regression problem. Neural networks, regression trees, and many other methods have been developed to estimate [tex]$G$[/tex] given the input output pair [tex] ( X,y ) [/tex].

One method that I have worked with is called Gaussian process regression. There many good texts and papers on the subject. For more technical information on the method and its applications see: http://www.gaussianprocess.org/

A key problem that arises in developing these models on very large data sets is that it ends up requiring an [tex]O(N^3)[/tex] computation where N is the number of data points and the training sample. Obviously this becomes very problematic when N is large.

I discussed this problem with Leslie Foster, a mathematics professor at San Jose State University.  He, along with some of his students, developed a method  to address this problem based on Cholesky decomposition and pivoting.   He also shows that this leads to a numerically stable result.  If ou're interested in some light reading, I’d suggest you take a look at his [recent paper](    ) (which was accepted in the Journal of Machine Learning Research) posted on dashlink. We've also posted code for you to try it out. Let us know how it goes.

If you are interested in applications of this method in the area of prognostics, check out our [new paper](/dashlink/resources/51/) on the subject which was published in IEEE Transactions on Systems, Man, and Cybernetics.
Presentation given by SRI NRA winners on Verification and Validation for Complex Systems.
ISWHM: Tools and Techniques for Software and System Health Management
Integrity Assurance methods for Integrated Vehicle Health Management
The lecture of the [Stanford-IVHM lecture series](https://dashlink.arc.nasa.gov/group/stanford-ivhm-lecture-series/)  will give an overview of the approaches in building diagnostic solutions for networks and complex systems. The conventional rule-based approach and the top-down analysis will be compared with other innovative solutions based on information modeling and codebook correlation. One specific solution pioneered by research done in Columbia University and later implemented by SMARTS/EMC  will be presented in more detail as an example of a consistent approach to diagnostics. 

 

Speaker:

Yuri Rabover, Ph.D. VMTurbo

Dr. Yuri Rabover, is a co-founder and Director of Product Strategy of VMTurbo, a startup in a stealth mode. Prior to VMTurbo Yuri spent 12 years working for SMARTS as director of engineering, product management and technology partnership. After EMC acquired SMARTS for $275M in 2005, Yuri was managing the Advanced Solution Group in the EMC Corporate CTO Office developing prototypes and proof of concepts of new innovative solutions. He is a seasoned technologist, strategist and researcher in the wide area of system, network and storage management with more than 20 years of industry and academia experience.
This presentation will review the use of knowledge management in the development and support of Condition Based Maintenance (CBM) systems for complex systems with particular emphasis on the experience of the development of the Fault Model for large commercial  aircraft.  The presentation is divided into four sections:

1.       Review of experience of building fault models and Central Maintenance Computer for large commercial aircraft.
2.       Review of the key functions and usage scenarios for a typical CBM Knowledge Management System
3.       Identification of criteria for evaluation of implementation alternatives

The presentation will conclude with a short discussion of future directions for CBM Knowledge Management Systems.

**Speaker: Tim Felke, Honeywell**

 

Tim Felke joined Honeywell in 1984 as a control systems analyst and was the manager for their Systems Analysis and Engineering Sciences department for several years. He was a principle author of the proposal for the Central Maintenance Computer for the Boeing 777 and then was a leader in its development. Since then he has been an Engineering Fellow for the diagnostic and knowledge management functions of the Aircraft Diagnostic and Maintenance Systems group. In this work he has published several papers and is the principle inventor or significant contributor on nearly a dozen patents. He holds a BS in Electrical Engineering from Arizona State University.
This presentation will review the use of knowledge management in the development and support of Condition Based Maintenance (CBM) systems for complex systems with particular emphasis on the experience of the development of the Fault Model for large commercial  aircraft.  The presentation is divided into four sections:

1.       Review of experience of building fault models and Central Maintenance Computer for large commercial aircraft.
2.       Review of the key functions and usage scenarios for a typical CBM Knowledge Management System
3.       Identification of criteria for evaluation of implementation alternatives

The presentation will conclude with a short discussion of future directions for CBM Knowledge Management Systems.

**Speaker: Tim Felke, Honeywell**

 

Tim Felke joined Honeywell in 1984 as a control systems analyst and was the manager for their Systems Analysis and Engineering Sciences department for several years. He was a principle author of the proposal for the Central Maintenance Computer for the Boeing 777 and then was a leader in its development. Since then he has been an Engineering Fellow for the diagnostic and knowledge management functions of the Aircraft Diagnostic and Maintenance Systems group. In this work he has published several papers and is the principle inventor or significant contributor on nearly a dozen patents. He holds a BS in Electrical Engineering from Arizona State University.
Abstract

The semiconductor industry is constantly searching for new ways to increase the rate of both process development and yield learning.  As more data is being collected and stored throughout the chip manufacturing process, it has become increasingly more difficult to analyze yield signals using traditional statistical methods.  Most of the serious yield issues manifest themselves as non-random electrical failure maps. Our semi-supervised fault
detection framework has elements of Spatial Signature Analysis (SSA) to capture yield signals for very large datasets without losing the critical details typically involved with summarization techniques.  It includes signature detection, de-noising, clustering, and purification that allow one to create a true spatial response metric of the yield issue. Once this has been accomplished, one can load process data to join with the spatial
response and invoke customized rule induction algorithms that generate a set of hypotheses - likely process causes for a specific spatial target response.  The framework has been successfully used at Intel and represents an example of the growing influence of modern statistical learning in the semiconductor industry.

 

**Speaker:**

**Dr. Eugene Tuv, Intel**

Dr. Eugene Tuv is a Senior Staff Research Scientist in the Logic Technology Department at Intel. His research interests include supervised and unsupervised non-parametric machine learning with massive heterogeneous data. Prior to Intel he worked as a research scientist in the Institute of Nuclear Research, Ukrainian Academy of Science. He holds postgraduate degrees in Mathematics and Applied Statistics.
**Abstract**

In modern fighter aircraft with statically unstable airframe designs, the flight control system is considered flight critical, i.e. the aircraft will encounter a catastrophic event if the system fails. Consequently, the system design has to meet high levels of reliability and failure immunity. In this presentation, an overview will be provided on the basic concepts employed in flight critical system design for fault tolerance. Different methods of redundancy implementation, failure management, and health management will be discussed. Basic concepts in fault diagnostics will also be discussed, along with some new concepts for implementation of prognostics in reducing levels of physical system redundancy.

 
**Bio** 

David S. Bodden is Lockheed Martin Senior Fellow. He recieved BS in Aerospace Engineering from Texas A&M University in 1976 and MS in Engineering Science and Mechanics from Virginia Tech in 1984. Mr. Bodden’s technical career has encompassed a broad scope of technology areas. He has worked in structural dynamics, advanced design, conceptual design, flight control systems, and prognostics. His management experience includes six years as Chief of the Control Law design and Analysis Group followed by seven years as the Senior Manager of Flight Control Systems. Mr. Bodden was selected as a Technical Fellow in Flight Controls at LM Aeronautics in 2002 and as a Senior Fellow in 2007. Mr. Bodden has authored numerous papers and technical proposals, and managed numerous technology development programs. He served on the AIAA Guidance, Navigation, and Control Technical Committee, he has served as the Chairman of the Lockheed Martin Corporate Task Force on Guidance and Control, he initiated and served as Chairman of the Lockheed Martin GNC Technology Focus Group, is former Chairman of the SAE Aerospace Control and Guidance Systems Committee, and he currently serves as Chairman of the Texas A&M Aerospace Advisory Board.
Reliable systems health management is an important research area of NASA. A health management system that can accurately and quickly diagnose faults in various on-board systems of a vehicle will play a key role in the success of current and future NASA missions. We introduce in this paper the ProDiagnose algorithm, a diagnostic algorithm that uses a probabilistic approach, accomplished with Bayesian Network models compiled to Arithmetic Circuits, to diagnose these systems. We describe the ProDiagnose algorithm, how it works, and the probabilistic models involved. We show by experimentation on two Electrical Power Systems based on the ADAPT testbed, used in the Diagnostic Challenge Competition (DX-09), that ProDiagnose can produce results with over 96% accuracy and < 1 second mean diagnostic time.

**Reference:**

B. W. Ricks, and O. J. Mengshoel. "The Diagnostic Challenge Competition: Probabilistic Techniques for Fault Diagnosis in Electrical Power Systems." Proc. of the 20th International workshop on Principles of Diagnosis (DX-09) Stockholm, Sweden, 2009

**BibTex Reference:**

@inproceedings{ricks09diagnostic,
  author    = {Ricks, B. W. and Mengshoel, O. J.},
  title     = {The Diagnostic Challenge Competition: Probabilistic Techniques for Fault Diagnosis in Electrical Power Systems},
  booktitle     = {Proc. of the 20th International Workshop on Principles of Diagnosis (DX-09)},
  address = {Stockholm, Sweden},
  year      = {2009}
}
We present in this article a case study of the probabilistic
approach to model-based diagnosis. Here, the diagnosed
system is a real-world electrical power system, namely the
Advanced Diagnostic and Prognostic Testbed (ADAPT) located
at the NASA Ames Research Center. Our probabilistic approach
is formally well-founded, and based on Bayesian networks and
arithmetic circuits. We pay special attention to meeting two of the
main challenges  model development and real-time reasoning
 often associated with real-world application of model-based
diagnosis technologies. To address the challenge of model development,
we develop a systematic approach to representing electrical
power systems as Bayesian networks, supported by an easy-touse
specication language. To address the real-time reasoning
challenge, we compile Bayesian networks into arithmetic circuits.
Arithmetic circuit evaluation supports real-time diagnosis by
being predictable and fast. In experiments with the ADAPT
Bayesian network, which contains 503 discrete nodes and 579
edges and produces accurate results, the time taken to compute
the most probable explanation using arithmetic circuits has a
mean of 0.2625 milliseconds and a standard deviation of 0.2028
milliseconds. In comparative experiments, we found that while
the variable elimination and join tree propagation algorithms
also perform very well in the ADAPT setting, arithmetic circuit
evaluation was an order of magnitude or more faster.

**Reference:**

O. J. Mengshoel, M. Chavira, K. Cascio, S. Poll, A. Darwiche,
and S. Uckun. "Probabilistic Model-Based Diagnosis: An Electrical
Power System Case Study”. Accepted to IEEE Transactions on
Systems, Man, and Cybernetics, Part A, 2009.
This is the first version of the performance evaluation tool. Evaluation is based on point estimates of the RUL predictions.

a more detailed documentation will be available with the tool soon.

in the meantime, please download the attached files/folder in the same root folder to run a demo. To evaluate your own results create results & application data files in .mat format and save in the results folder. please make sure you name your files as xxx_results.mat for results and yyy_appData.mat for application data.
In performance maintenance in large, complex systems, sensor information from sub-components tends to be readily available, and can be used to make predictions about the system's health and diagnose possible anomalies. 

 However, existing methods can only use predictions of individual component anomalies to guess at systemic problems, not accurately estimate the magnitude of the problem, nor prescribe good solutions. 

 Since physical complex systems usually have well-defined semantics of operation, we here propose using anomaly detection  techniques drawn from data mining in conjunction with an automated theorem prover working on a domain-specific knowledge base to perform systemic anomalydetection on complex systems.

 For clarity of presentation, the remaining content of this submission is presented compactly in Fig 1.
Anomaly detection has recently become an important problem in many industrial and financial applications. In several instances, the data to be analyzed for possible anomalies is located at multiple sites and cannot be merged due to practical constraints such as bandwidth limitations and proprietary concerns. At the same time, the size of data sets affects prediction quality in almost all data mining applications. In such circumstances, distributed data mining algorithms may be used to extract information from multiple data sites in order to make better predictions. In the absence of theoretical guarantees, however, the degree to which data decentralization affects the performance of these algorithms is not known, which reduces the data providing participants' incentive to cooperate.This creates a metaphorical 'prisoners' dilemma' in the context of data mining.

 

In this work, we propose a novel general framework for distributed anomaly detection with theoretical performance guarantees. Our algorithmic approach combines existing anomaly detection procedures with a novel method for computing global statistics using local sufficient statistics. We show that the performance of such a distributed approach is indistinguishable from that of a centralized instantiation of the same anomaly detection algorithm, a condition that we call zero information loss. We further report experimental results on synthetic as well as real-world data to demonstrate the viability of our approach.

 The remaining content of this presentation is presented in Fig. 1.
The automated, real-time classification of variable
and transient events in terms of their astrophysical
nature is quickly becoming a necessity for the new synoptic sky surveys.

This generally has to be done using sparse
and heterogeneous measurements for
individual events, both from the survey
pipelines and existing archives.
The data we used in our tests are both from
archival observations, as well as from our
own follow-up of recent transients from
the PQ and CRTS surveys.

 

See file for more information.
AISRP Presentations from CIDU/AISRP 2009.
CIDU Presentations
Health management systems that more accurately and quickly diagnose faults that may occur in different technical systems on-board a vehicle will play a key role in the success of future NASA missions. We discuss in this paper the diagnosis of abrupt continuous (or parametric) faults within the context of probabilistic graphical models, more specifically Bayesian networks that are compiled to arithmetic circuits. This paper extends our previous research, within the same probabilistic setting, on diagnosis of abrupt discrete faults. Our approach and diagnostic algorithm ProDiagnose are domain-independent; however we use an electrical power system testbed called ADAPT as a case study. In one set of ADAPT experiments, performed as part of the 2009 Diagnostic Challenge, our system turned out to have the best performance among all competitors. In a second set of experiments, we show how we have recently further significantly improved the performance of the probabilistic model of ADAPT. While these experiments are obtained for an electrical power system testbed, we believe they can easily be transitioned to real-world systems, thus promising to increase the success of future NASA missions.

**Reference:**

B. W. Ricks and O. J. Mengshoel, "Methods for Probabilistic Fault Diagnosis: An Electrical Power System Case Study."  In Proc. of the First Annual Conference of the Prognostics and Health Management Society (PHM-09), San Diego, CA, September 27 – October 1, 2009.

**BibTex Reference:**

@inproceedings{ricks09methods,
  author    = {Ricks, B. W. and Mengshoel, O. J.},
  title     = {Methods for Probabilistic Fault Diagnosis: An Electrical Power System Case Study},
  booktitle = {Proc. of the Annual Conference of the Prognostics and Health Management Society (PHM-09)},
  address   = {San Diego, CA},  month     = sep,
  year      = {2009}
}
IVHM Presentations
Posters form 2009 Aviation Safety Technical Conference
Paper on this topic has been submitted to KDD 2010.
CIDU 2010 LaTeX and Microsoft Word templates.
Aviation Safety Information Analysis and Sharing (ASIAS) Symposiusm Presentations: July 27-28, 2009
This is a collection of different presentations that cover a range of topics within ISHM for Launch Vehicles
CIDU 2010 Student Travel Award Application Form
Modern aircraft are producing data at an unprecedented rate with hundreds of parameters being recorded on a second by second basis. The data can be used for studying the condition of the hardware systems of the aircraft and also for studying the complex interactions between the pilot and the aircraft. NASA is developing novel data mining algorithms to detect precursors to aviation safety incidents from these data sources. This talk will cover the theoretical aspects of the algorithms and practical aspects of implementing these techniques to study one of the most complex dynamical systems in the world: the national airspace.
Detailed schedule for CIDU 2010.
Spectral Decomposition Algorithm (SDA) is an unsupervised feature extraction technique similar to PCA that was developed to better distinguish spectral features in the space shuttle main engine's optical plume. See paper below:

 

Code is not open sourced and therefore it is not available. See paper for sample pseudo code.
Detecting and describing anomalies in large repositories of discrete symbol sequences.

 

**sequenceMiner has been open-sourced! Download the  file below to try it out.**

 

sequenceMiner was developed to address the problem of detecting and describing anomalies in large sets of high-dimensional symbol sequences. sequenceMiner works by performing unsupervised clustering (grouping) of sequences using the normalized longest common subsequence (LCS) as a similarity measure, followed by a detailed analysis of outliers to detect anomalies. sequenceMiner utilizes a new hybrid algorithm for computing the LCS that has been shown to outperform existing algorithms by a factor of five.

sequenceMiner also includes new algorithms for outlier analysis that provide comprehensible indicators as to why a particular sequence was deemed to be an outlier. This provides analysts with a coherent description of the anomalies identified in the sequence, and why they differ from more “normal” sequences.

 

sequenceMiner was developed with funding from the NASA Aviation Safety Program.  In the commercial aviation domain, sequenceMiner can be used to discover atypical behavior in airline performance data that may have possible operational significance for safety analysts.  But because the sequenceMiner approach is general and not restricted in any way to a domain, and these algorithms can be applied in other fields where anomaly detection and event mining would be useful.
Overview:  

ReADS can analyze text reports, such as aviation reports and problem or maintenance records.  ReADS uses text clustering algorithms to group loosely related reports and documents, this reduces human error and fatigue.  Plus, ReADS identifies interconnected reports; automating the discovery of possible recurring anomalies.  ReADS provides a visualization of the clusters and recurring anomalies. ReADS has been integrated into a secure web-based search tool to allow uses to perform their own text mining.

 

Recurring Anomaly Identification

ReADS identifies reports which mention other reports as a recurring anomaly using regular expressions to search documents and identify references of other reports by name. ReADS also detects recurring anomalies by determining the similarity between documents using a cosine distance similarity measure.  Then according to the similarity measure, ReADS will run a hierarchical clustering algorithm to detect the recurring anomalies.  The hierarchical tree is partitioned into clusters by setting a threshold. A low threshold implies that the reports must be very similar to be sorted into the same cluster.

 

Here's more [info](http://ti.arc.nasa.gov/projects/pria/).

 

The figure below is a screenshot of the clustering results.
The Mariana source code has been open sourced.  Download the tar file Mariana.tgz below.  I would love feedback.

 

Mariana is an auto-classifier algorithm that efficiently optimizes hyperparameters for Support Vector Machines.

Mariana is an algorithm that efficiently optimizes the hyperparameters for Support Vector Machines for regression and classification.  It currently uses Simulated Annealing for optimization but can be extended to use a variety of stochastic optimization techniques including, Markov Chain Monte Carlo, Sequential Monte Carlo, and Genetic Algorithms. Mariana can be applied to the text portion of reports, determining the likely categories that each report falls into, and calculating a confidence for each classification. Mariana¹s innovation is it automates the search for the optimum hyperparameters.  It does so by randomly selecting a set of hyperparameters.  Next it builds a model from the training data and tests the model's performance using the validation set.  That performance is compared to previous performances, and if the current set of hyperparameters are better than the previous one, then it records the hyperparameters.  This process is repeated until there are no noticeable improvements in performance or at a predefined stopping point.
We present a method of generating Mercer Kernels
from an ensemble of probabilistic mixture models,
where each mixture model is generated from a Bayesian
mixture density estimate. We show how to convert the
ensemble estimates into a Mercer Kernel, describe the
properties of this new kernel function, and give examples
of the performance of this kernel on unsupervised
clustering of synthetic data and also in the domain of
unsupervised multispectral image understanding.
IMS: Inductive Monitoring System 

The Inductive Monitoring System (IMS) is a tool that uses a data mining technique called clustering to extract models of normal system operation from archived data. IMS works with vectors of data values. IMS analyzes data collected during periods of normal system operation to build a system model. It characterizes how the parameters relate to one another during normal operation by finding areas in the vector space where nominal data tends to fall. These areas are called nominal operating regions and correspond to clusters of similar points found by the IMS clustering algorithm. These nominal operating regions are stored in a knowledge base that IMS uses for real-time telemetry monitoring or archived data analysis.  

During the monitoring operation, IMS reads real-time or archived data values, formats them into the predefined vector structure, and searches the knowledge base of nominal operating regions to see how well the new data fits the nominal system characterization. For each input vector, IMS returns the distance that vector falls from the nearest nominal operating region. Data that matches the normal training data well will have a deviation distance of zero. If one or more of the data parameters is slightly outside of expected values, a small non-zero result is returned. As incoming data deviates further from the normal system data, indicating a possible malfunction, IMS will return a higher deviation value to alert users of the anomaly. IMS also calculates the contribution of each individual parameter to the overall deviation, which can help isolate the cause of the anomaly.
Orca is a data-driven, unsupervised anomaly detection algorithm that uses a distance-based approach. It uses a novel pruning rule that allows it to run in nearly linear time. Orca was co-developed by Stephen Bay of ISLE and Mark Schwabacher of NASA ARC. More information about Orca, including downloadable software, can be found here:

[http://stephenbay.net/orca/](http://stephenbay.net/orca/)

A conference paper about Orca can be found here:

[https://dashlink.arc.nasa.gov/paper/mining-distance-based-outliers-in-near-linear-time/](https://dashlink.arc.nasa.gov/paper/mining-distance-based-outliers-in-near-linear-time/)
HyDE is a model-based diagnosis engine for stochastic hybrid systems. HyDE uses transitional and behavioral models of the system to diagnose the occurrence of unobserved events (a subset of which could be faults). More details can be found on the HyDE webpage [http://ti.arc.nasa.gov/project/hyde-diagnostics/](http://ti.arc.nasa.gov/project/hyde-diagnostics/)
The code in the stableGP package implements Gaussian process calculations using efficient and numerically stable algorithms. Description of the algorithms is in the paper "Stable and Efficient Gaussian Process Calculations" by L. Foster, A. Waagen, N. Aijaz, M. Hurley, A. Luis, J. Rinsky, C. Satyavolu, M. Way, P. Gazis, and A. Srivastava accepted in the Journal of Machine Learning Research, February, 2009.

The easiest way to get started using the code is to download and unzip the zip file, start Matlab (7.0 or higher), move to the appropriate folder and type either "demo_bootstrap" or "demo_history" to run one of the demonstration files.

Code in the zip file is based on the code used in the text Gaussian Processes or Machine Learning by Rasmussen and Williams (www.gaussianprocess.org/gpml/).  So that the demonstrations are self contained and do not require that the user download additional code the zip file contains a few functions that are copied directly from Rasmussen and Williams' code.
In this research, we propose a variant of the classical Matching Pursuit Decomposition (MPD) algorithm with significantly improved scalability and computational performance. MPD is a powerful iterative algorithm that decomposes a signal into linear combinations of its dictionary elements or “atoms”. A best fit atom from an arbitrarily defined dictionary is determined through cross-correlation. The selected atom is subtracted from the signal and this procedure is repeated on the residual in the subsequent iterations until a stopping criteria is met.

A sufficiently large dictionary is required for an accurate reconstruction; this in return increases the computational burden of the algorithm, thus limiting its applicability and level of adoption. Our main contribution lies in improving the computational efficiency of the algorithm to allow faster decomposition while maintaining a similar level of accuracy. The Correlation Thresholding and Multiple Atom Extractions techniques were proposed to decrease the computational burden of the algorithm. Correlation thresholds prune insignificant atoms from the dictionary. The ability to extract multiple atoms within a single iteration enhanced the effectiveness and efficiency of each iteration. The proposed algorithm, entitled MPD++, was demonstrated using real world data set.
Matrikon OPC server

 

Recurrent NARX NNs

 

LWPR
Blind source separation in Simulink using STFT and inverse STFT
(Signal processing blockset).
power cepstrum of sound, speech and vibrations using log of power spectrum estimation (periodogram)
One-class nu-Support Vector machine (SVMs) learning technique maps the 
input data into a much higher dimensional space and then uses a small 
portion of the training data (support vectors) to parametrize the 
decision surface that can linearly separate nu fraction of training 
points (labeled as anomalies) from the rest. The exact solution of 
standard one-class nu SVMs assigns (at least) nu fraction of training 
points as support vectors. However some of these support vectors may be 
unnecessary or redundant. Hence the computational issue turns alarming 
especially when SVMs based novelty detectors with nonlinear kernels are 
trained on data sets of huge size. The proposed nu-Anomica algorithm can 
solve this problem. The idea is to train the machine such that it can 
provide a close approximation to the exact decision plane using far less 
number of training points and without loosing much of the generalization 
performance of the classical approach. The developed procedure closely 
preserves the accuracy of standard One-class nu-SVMs while reducing both 
training time and test time by several factors.
This dataset contains the records of all the flights in the Northern California TRACON. The data was provided by the aircraft noise abatement office [(http://www.flyquietsfo.com/)](http://www.flyquietsfo.com/) of San Francisco International Airport.
The data cover Jan-Mar 2006. It is organized by day and flight. Each record contains some information about the flight and a sequence of 3D position and estimated speed.


This data contains thousands of trajectories that can be used for trajectory clustering. The data is used by the Aircraft Noise Abatement Office
to analyze the trajectories of aircraft flying in and out SFO. The objective is to minimize the noise pollution due to aircraft in the San Francisco Bay Area

The files have the extension "lt6" and are organized as follow, one file per day.

line number & explaination

<pre>1 TRACK OPNUM (TRACK header word and operation number)
2 eventid (Corralation number)
3 trackstart date (in time since 1900, A8 version four year digit)
4 trackstart time HH:MM:SS


5 trackend time HH:MM:SS
6 airportid
7 ACID (FLIGHTNUM/TAILNUMBER)
8 owner name
9 aircrafttype
10 aircraft category
11 beacon
12 adflag
13 waypoint
14 other_port (dest/origin)
15 runwayname


16 min alt
17 max alt
18 min range
19 max range
20 Count of trackpoints (to follow)
21 x,y,z,v,t (all points is meters relative to MRP, velocity and time from start of track)</pre>
Preliminary data from thermal overstress accelerated aging using the aging and characterization system. The data set contains aging data from 6 devices, one device aged with DC gate bias and the rest aged with a squared signal gate bias. Several variables are recorded and in some cases, high-speed measurements of gate voltage, collector-emitter voltage and collector current are available. The data set is provided by the Prognostics CoE at NASA Ames.
**Subject Area:**

Astronomical data

 

**Description:**

The Sloan Digital Sky Survey (SDSS) is a multi-organization effort to gather deep, multi-color images covering more than a quarter of the sky and create 3-dimensional maps of celestial objects. The data is released annually to the general public as data releases (DR)'s.

 

The SDSS used a dedicated 2.5-meter telescope at Apache Point Observatory, New Mexico, equipped with two powerful special-purpose instruments. The 120-megapixel camera imaged 1.5 square degrees of sky at a time, about eight times the area of the full moon. A pair of spectrographs fed by optical fibers measured spectra of (and hence distances to) more than 600 galaxies and quasars in a single observation. A custom-designed set of software pipelines kept pace with the enormous data flow from the telescope.

 

The data set and more info can be found at http://cas.sdss.org/astrodr6/en/.
Synthetic data used to demonstrate the effectiveness of the MKAD algorithm with respect to detecting anomalies in both the continuous numerical data and binary discrete data.
The world-wide aviation system is one of the most complex dynamical systems ever developed and is generating data at an extremely rapid rate. Most modern commercial aircraft record several hundred flight parameters including information from the guidance, navigation, and control systems, the avionics and propulsion systems, and the pilot inputs into the aircraft. These parameters may be continuous measurements or binary or categorical measurements recorded in one second intervals for the duration of the flight. Currently, most approaches to aviation safety are reactive, meaning that they are designed to react to an aviation safety incident or accident. In this paper, we discuss a novel approach based on the theory of multiple kernel learning to detect potential safety anomalies in very large data bases of discrete and continuous data from world-wide operations of commercial fleets. We pose a general anomaly detection problem which includes both discrete and continuous data streams, where we assume that the discrete streams have a causal influence on the continuous streams. We also assume that atypical sequences of events in the discrete streams can lead to off-nominal system performance. We discuss the application domain, novel algorithms, and also discuss results on real-world data sets. Our algorithm uncovers operationally significant events in high dimensional data streams in the
aviation industry which are not detectable using state of the art methods.
**Subject Area:**
    Text Mining

**Description:**
    This is the dataset used for the SIAM 2007 Text Mining competition. This competition focused on developing text mining algorithms for document classification. The documents in question were aviation safety reports that documented one or more problems that occurred during certain flights. The goal was to label the documents with respect to the types of problems that were described. This is a subset of the Aviation Safety Reporting System (ASRS) dataset, which is publicly available.

**How Data Was Acquired:**
    The data for this competition came from human generated reports on incidents that occurred during a flight.

**Sample Rates, Parameter Description, and Format:**
    There is one document per incident. The datasets are in raw text format. All documents for each set will be contained in a single file. Each row in this file corresponds to a single document. The first characters on each line of the file are the document number and a tilde separats the document number from the text itself.

**Anomalies/Faults:**
    This is a document category classification problem.
**PHM08 Challenge Dataset is now publicly available at the NASA Prognostics Respository + [Download](http://ti.arc.nasa.gov/tech/dash/pcoe/prognostic-data-repository/)** An online evaluation utility is also provided to let users evaluate their results and get feedback on test dataset.

Run-to-failure data: Engine degradation simulation was carried out using C-MAPSS tool. Four different sets were simulated under different combinations of operational conditions and fault modes. Several sensor channels were recorded to characterize fault evolution.
The data set was provided by the Prognostics CoE at NASA Ames. The set is in text format and has been zipped including a readme file. Please cite: "A. Saxena and K. Goebel (2008). "Turbofan Engine Degradation Simulation Data Set", [NASA Ames Prognostics Data Repository](http://ti.arc.nasa.gov/project/prognostic-data-repository), NASA Ames, Moffett Field, CA."
How Data Was Acquired: The data presented is from a physical simulator that simulated engine disks.
Sample Rates and Parameter Description: All parameters are sampled once per revolution measuring 32 blade to edge clearances on each revolution. Data is recorded for approximately 3 minutes for each run. The parameters are the revolution measurement, the clock time, the measured RPM, the maximum, average, and minimum gap across all gap sensors, and the measured gap for blade 0 to blade 31.
Anomalies/Faults: Faults include medium and large cracks on the disk.
This data set is a simulated data set based on the flight simulator "FLTz" used by the Intelligent Flight Control (IFC) group at NASA ARC. Flights were preprogrammed to fly through randomly generated circular flight paths starting from San Francisco International Airport (SFO) and ending at approximately the same location. No known anomalous flights were simulated.
We discuss a statistical framework that underlies envelope detection schemes as well as dynamical models based on Hidden Markov Models (HMM) that can encompass both discrete and continuous sensor measurements for use in Integrated System Health Management (ISHM) applications. The HMM allows for the rapid assimilation, analysis, and discovery of system anomalies.  We motivate our work with a discussion of an aviation problem where the identification of anomalous sequences is essential for safety reasons. The data in this application are discrete and continuous sensor measurements and can be dealt with seamlessly using the methods described here to discover anomalous flights. We specifically treat the problem of discovering anomalous features in the time series that may be hidden from the sensor suite and compare those methods to standard
envelope detection methods on test data designed to accentuate the differences between the two methods. Identification
of these hidden anomalies is crucial to building stable, reusable, and cost-efficient systems. We also discuss a data mining framework for the analysis and discovery of anomalies in high-dimensional time series of sensor measurements that would be found in an ISHM system. We conclude with recommendations that describe the tradeoffs in building an integrated scalable platform for robust anomaly detection in ISHM applications.
We present a set of novel algorithms which we call sequenceMiner that detect and characterize anomalies in large sets of high-dimensional symbol sequences that arise from recordings of switch sensors in the cockpits of commercial airliners. While the algorithms we present are general and domain-independent, we focus on a specific problem that is critical to determining the system-wide health of a fleet of aircraft. The approach taken uses
unsupervised clustering of sequences using the normalized length of the longest common subsequence (nLCS) as a similarity measure, followed by detailed outlier analysis to detect anomalies. In this method, an outlier sequence is defined as a sequence that is far away from the cluster centre. We present new algorithms for outlier analysis that provide comprehensible indicators as to why a particular sequence is deemed to be an outlier. The algorithms provide a coherent description to an analyst of the anomalies in the sequence when compared to more normal sequences. In the final section of the paper we demonstrate the effectiveness of sequenceMiner for anomaly detection on a real set of discrete sequence data from a fleet of commercial airliners. We show that sequenceMiner discovers actionable and operationally significant safety events. We also compare our innovations with standard HiddenMarkov Models, and show that our methods are superior.
This paper describes the application of known and novel prognostic algorithms on systems that can be described by low dimensional, potentially nonlinear dynamics. The methods rely on estimating the conditional probability distribution of the output of the system at a future time given knowledge of the current state of the system. We show how to estimate these conditional probabilities using a variety of techniques, including bagged neural networks and kernel methods such as Gaussian Process Regression (GPR). The results are compared with standard method such as the nearest neighbor algorithm. We demonstrate the algorithms on a real-world data set and a simulated data set. The real-world data set consists of the intensity of an NH3 laser. The laser data set has been shown by other authors to exhibit low-dimensional chaos with sudden drops in intensity. The simulated data set is generated from the Lorenz attractor and has known statistical characteristics. On these data sets, we show the evolution of the estimated conditional probability distribution, the way it can act as a prognostic signal, and its use as an early warning system. We also review a novel approach to perform Gaussian Process Regression with large numbers of data points.
The analysis of spectral signals for features that represent physical phenomenon is ubiquitous in the science and engineering communities. There are two main approaches that can be taken to extract relevant features from these high-dimensional data streams. The first set of approaches relies on extracting features using a physics-based paradigm where the underlying physical mechanism that generates the spectra is used to infer the most important features in the data stream. We focus on a complementary methodology that uses a data-driven technique that is informed by the underlying physics but also has the
ability to adapt to unmodeled system attributes and dynamics. We discuss the following four algorithms: Spectral Decomposition Algorithm (SDA), Non-Negative Matrix Factorization (NMF), Independent Component Analysis (ICA) and Principal Components Analysis (PCA) and compare their performance on a spectral emulator which we use to generate artificial data with known statistical properties. This spectral emulator mimics the real-world phenomena arising from the plume of the space shuttle main engine and can be used to validate the results that arise from various spectral decomposition algorithms and is very useful for situations where real-world systems have very low probabilities of fault or failure. Our results indicate that methods like SDA and NMF provide a straightforward way of incorporating prior physical knowledge while NMF with a tuning mechanism can give superior performance on some tests. We demonstrate these
algorithms to detect potential system-health issues on data from a spectral emulator with tunable health parameters.
This paper provides a review of three different advanced machine learning algorithms for anomaly detection in continuous data streams from a ground-test firing of a subscale Solid Rocket Motor (SRM). This study compares Orca, one-class support vector machines, and the Inductive Monitoring System (IMS) for anomaly detection on the data streams. We measure the performance of the algorithm with respect to the detection horizon for situations where fault information is available. These algorithms have been also studied by the present authors (and other co-authors) as applied to liquid propulsion systems. The trade space will be explored between these algorithms for both types of propulsion systems.
Several different unsupervised anomaly detection algorithms have been applied to Space Shuttle Main Engine (SSME) data to serve the purpose of developing a comprehensive suite of Integrated Systems Health Management (ISHM) tools. As the theoretical bases for these methods vary considerably, it is reasonable to conjecture that the resulting anomalies detected by them may differ quite significantly as well. As such, it would be useful to apply a common metric with which to compare the results. However, for such a quantitative analysis to be statistically significant, a sufficient number of examples of both nominally categorized and anomalous data must be available. Due to the lack of sufficient examples of anomalous data, use of any statistics that rely upon a statistically significant sample of anomalous data is infeasible. Therefore, the main focus of this paper will be to compare actual examples of anomalies detected by the algorithms via the sensors in which they appear, as well the times at which they appear. We find that there is enough overlap in detection of the anomalies among all of the different algorithms tested in order for them to corroborate the severity of these anomalies. In certain cases, the severity of these anomalies is supported by their categorization as failures by experts, with realistic physical explanations. For those anomalies that can not be corroborated by at least one other method, this overlap says less about the severity of the anomaly, and more about their technical nuances, which will also be discussed.
The use of Gaussian processes can be an effective approach to prediction in a supervised learning environment. For large data sets, the standard Gaussian process approach requires solving very large systems of linear equations and approximations are required for the calculations to be practical. We will focus on the subset of regressors approximation technique. We will demonstrate that there can be numerical instabilities in a well known implementation of the technique. We discuss alternate implementations that have better numerical stability properties and can lead to better predictions. Our results will be illustrated by looking at an application involving prediction of galaxy redshift  from broadband spectrum data.
This paper presents a new methodology for automatic knowledge driven data mining based on the theory of Mercer Kernels, which are highly nonlinear symmetric positive definite mappings from the original image space to a very high, possibly infinite dimensional feature space. We describe a new method called Mixture Density Mercer Kernels (MDMK) to learn kernel function directly from data, rather than using pre-defined kernels. These data adaptive kernels can encode prior knowledge in the kernel using a Bayesian formulation, thus allowing for physical information to be encoded in the model. Specifically, we demonstrate the use of the algorithm in situations with extremely small samples of data. We compare the results with existing algorithms on data from the Sloan Digital Sky Survey (SDSS) and demonstrate the method’s superior performance against standard methods. The results show that the Mixture Density Mercer Kernel described here outperforms tree-based classification in distinguishing high-redshift galaxies from low redshift galaxies by approximately 16% on test data, bagged trees by approximately 7%, and bagged trees built on a much larger sample of data by approximately 2%. The code for these experiments has been generated with the AutoBayes tool, which automatically generates efficient and documented C/C++ code from abstract statistical model specifications. The core of the system is a schema library which contains templates for learning and knowledge discovery algorithms like different versions of EM, or numeric optimization methods like conjugate gradient methods. The template instantiation is supported by symbolic algebraic computations, which allows AutoBayes to find closed form solutions and, where possible, to integrate them into the code.
In previous papers, we introduced the idea of a Virtual Sensor,  which is a mathematical model trained to learn the potentially  nonlinear relationships between spectra for a given image scene for the purpose of predicting values of a subset of those spectra when only partial measurements have been taken. Such models can be created for a variety of disciplines including the Earth and Space Sciences as well as engineering domains. These nonlinear relationships are induced by the physical characteristics of the  image scene. In building a Virtual Sensor a key question that arises is that of characterizing the stability of the model as the underlying scene changes. For example, the spectral relationships could change for a given physical location, due to seasonal weather conditions. This paper, based on a talk given at the American Geophysical Union (2005), discusses the stability of predictions through time and also demonstrates the use of a Virtual Sensor in making multi-resolution predictions. In this scenario, a model is trained to learn the nonlinear relationships between spectra at a low resolution in order to predict the spectra at a high resolution.
This paper presents a method of generating Mercer Kernels from an ensemble of probabilistic mixture models, where each mixture model is generated from a Bayesian mixture density estimate. We show how to convert the ensemble estimates into a Mercer Kernel, describe the properties of this new kernel function, and give examples of the performance of this kernel on unsupervised clustering of synthetic data and also in the domain of unsupervised multispectral image understanding.
The detection of clouds within a satellite image is essential for retrieving surface geophysical parameters from optical and thermal imagery. Even a small percentage of cloud cover within a radiometer pixel can adversely affect the determination of surface variables such as albedo and temperature. Thus, onboard processing of satellite data requires reliable automated cloud detection algorithms that are applicable to a wide range of surface types. Unfortunately cloud-detection, particularly over snow- and ice-covered surfaces, is a problem that plagues the field of remote sensing because of the lack of spectral contrast.
This paper discusses preliminary results based on kernel methods for unsupervised discovery of snow, ice, clouds, and other geophysical processes based on data from the MODIS instrument and discusses implementation in computationally constrained environments such as those found on satellites.
This paper describes the results of a significant research and development effort conducted at NASA Ames Research Center to develop new text mining algorithms to discover anomalies in free-text reports regarding system health and safety of two aerospace systems. We discuss two problems of significant import in the aviation industry. The first problem is that of automatic anomaly discovery concerning an aerospace system through the analysis of tens of thousands of free-text problem reports that are written about the system. The second problem that we address is that of automatic discovery of recurring anomalies, i.e., anomalies that may be described in different ways by different authors, at varying times and under varying conditions, but that are truly about the same part of the system. The intent of recurring anomaly identification is to determine project or system weakness or high-risk issues. The discovery of recurring anomalies is a key goal in building safe, reliable, and cost-effective aerospace systems.
The Optical Plume Anomaly Detection (OPAD) system is under development to predict engine anomalies and engine parameters of the Space Shuttle's Main Engine (SSME). The anomaly detection is based on abnormal metal concentrations in the optical spectrum of the rocket plume. Such abnormalities could be indicative of engine corrosion or other malfunctions. Here, we focus on the second task of the OPAD system, namely the prediction of engine parameters such as rated power level (RPL) and mixture ratio (MR). Because of the high dimensionality of the spectrum, we developed a linear algorithm to resolve the optical spectrum of the exhaust plume into a number of separate components, each with a different physical interpretation. These components are used to predict the metal concentrations and engine parameters for online support of ground-level testing of the SSME. Currently, these
predictions are labor intensive and cannot be done online. We predict RPL using neural networks and give preliminary results.
Damage characterization through wave propagation and scattering is of considerable interest to many non-destructive evaluation techniques. For fiber-reinforced composites, complex waves can be generated during the tests due to the non-homogeneous and anisotropic nature of the material when compared to isotropic materials. Additional complexities are introduced due to the presence of the damage and thus results in difficulty to characterize these defects. The inability to detect damage in composite structures limits their use in practice. A major task of structural health monitoring is to identify and characterize the existing defects or defect evolution through the interactions between structural features and multidisciplinary physical phenomena. In a wave-based approach to addressing this problem, the presence of damage is characterized by the changes in the signature of the resultant wave that propagates through the structure. In order to measure and characterize the wave propagation, we use the response of the surface-mounted piezoelectric transducers as input to an advanced machine-learning based classifier known as a support vector machine.
NASA has some of the largest and most complex data sources in the world, with data sources ranging from the earth sciences, space sciences, and massive distributed engineering data sets from commercial aircraft and spacecraft. This talk will discuss some of the issues and algorithms developed to analyze and discover patterns in these data sets. We will also provide an overview of a large research program in Integrated Vehicle Health Management. The goal of this program is to develop advanced technologies to automatically detect, diagnose, predict, and mitigate adverse events during the flight of an aircraft. A case study will be presented on a recent data mining analysis performed to support the Flight Readiness Review of the Space Shuttle Mission STS-119.
Expanding upon the work of Way & Srivastava (2006) we demonstrate how the use of training sets of comparable size continue to make Gaussian Process Regression a competitive approach to that of Neural Networks and other least squares fitting methods. This is possible via new large size matrix inversion techniques developed for Gaussian Processes that do not require that the kernel matrix be sparse. This development, combined with a neural-network kernel function appears to give superior results for this problem. Our best t results for the Sloan Digital Sky Survey Main Galaxy Sample using u,g,r,i,z gives an rms error of 0.0201 while our results for the same in the Luminous Red Galaxy Sample yield 0.0220.
In this paper we propose ν-Anomica, a novel anomaly detection technique that can be trained on huge data sets with much reduced running time compared to the benchmark one-class Support Vector Machines algorithm. In ν-Anomica, the idea is to train the machine such that it can provide a close approximation to the exact decision plane using fewer training points and without losing much of the generalization performance of the classical approach. We have tested the proposed algorithm on a
variety of continuous data sets under different conditions. We show that under all test conditions the developed procedure closely preserves the accuracy of standard oneclass Support Vector Machines while reducing both the training time and the test time by 5 − 20 times.
his paper describes a local and distributed expectation maximization algorithm for learning parameters of Gaussian mixture models (GMM) in large peer-to-peer (P2P) environments. The algorithm can be used for a variety of well-known data mining tasks in distributed environments such as clustering, anomaly detection, target tracking, and density estimation to name a few, necessary for many emerging P2P applications in bioinformatics, webmining and sensor networks. Centralizing all or some of the data to build global models is impractical in such P2P environments because of the large number of data sources, the asynchronous nature of the P2P networks, and dynamic nature of the data/network. The proposed algorithm takes a two-step approach. In the monitoring phase, the algorithm checks if the model ‘quality’ is acceptable by using an efficient local algorithm. This is then used as a feedback loop to sample data from the network and rebuild the GMM when it is outdated. We present thorough experimental results to verify our theoretical claims.
This paper is about applying recurrent least squares support vector machines (LS-SVM) on three ESTSP08 competition datasets. Least squares

support vector machines are used as nonlinear models in order to avoid local

minima problems. Then prediction task is re-formulated as function approximation

task. Recurrent LS-SVM uses nonlinear autoregressive exogenous (NARX) model

to build nonlinear regressor, by estimating in each iteration the next output value,

given the past output and input measurements.
Title: Unsupervised Anomaly Detection for Liquid-Fueled Rocket Propulsion Health Monitoring.

Abstract: This article describes the results of applying four unsupervised anomaly detection algorithms to data from two rocket propulsion testbeds. The first testbed uses historical data from the Space Shuttle Main Engine. The second testbed uses data from an experimental rocket engine test stand located at NASA Stennis Space Center. The article describes nine anomalies detected by the four algorithms. The four algorithms use four different definitions of anomalousness. Orca uses a nearest-neighbor approach, defining a point to be an anomaly if its nearest neighbors in the data space are far away from it. The Inductive Monitoring System clusters the training data, and then uses the distance to the nearest cluster as its measure of anomalousness. GritBot learns rules from the training data, and then classifies points as anomalous if they violate these rules. One-class support vector machines map the data into a high-dimensional space in which most of the normal points are on one side of a hyperplane, and then classify points on the other side of the hyperplane as anomalous. Because of these different definitions of anomalousness, different algorithms detect different anomalies. We therefore conclude that it is useful to use multiple algorithms.
In a large network of computers, wireless sensors, or mobile devices, each of the components (hence, peers) has some data about the global status of the system. Many of the functions of the system, such as routing decisions, search strategies, data cleansing, and the assignment of mutual trust, depend on the global status. Therefore, it is essential that the system be able to detect, and react to, changes in its global status. Computing global predicates in such systems is usually very costly. Mainly because of their scale, and in some cases (e.g., sensor networks) also because of the high cost of communication. The cost further increases when the data changes rapidly (due to state changes, node failure, etc.) and computation has to follow these changes. In this paper we describe a two step approach for dealing with these costs. First, we describe a highly efficient local algorithm which detect when the L2 norm of the average data surpasses a threshold. Then, we use this algorithm as a feedback loop for the monitoring of complex predicates on the data – such as the data’s k-means clustering. The efficiency of the L2 algorithm guarantees that so long as the clustering results represent the data (i.e., the data is stationary) few resources are required. When the data undergoes an epoch change – a change in the underlying distribution – and the model no longer represents it, the feedback loop indicates this and the model is rebuilt. Furthermore, the existence of a feedback loop allows using approximate and “best-effort ” methods for constructing the model; if an ill-fit model is built the feedback loop would indicate so, and the model would be rebuilt.
In this paper we present a framework for forming interests-based Peer-to-Peer communities using client-side web browsing history. At the heart of this framework is the use of an order statistics-based approach to build communities with hierarchical structure. We have also carefully considered privacy concerns of the peers and adopted cryptographic protocols to measure similarity between them without disclosing their personal profiles. We evaluated our framework on a distributed data mining platform we have developed. The experimental results show that our framework could effectively build interests-based communities.
Peer-to-peer (P2P) networks are gaining popularity in many applications such as file sharing, e-commerce, and social networking, many of which deal with rich, distributed data sources that can benefit from data mining. P2P networks are, in fact,well-suited to distributed data mining (DDM), which deals with the problem of data analysis in environments with distributed data,computing nodes,and users. This article offers an overview of DDM applications and algorithms for P2P environments,focusing particularly on local algorithms that perform data analysis by using computing primitives with limited communication overhead. The authors describe both exact and approximate local P2P data mining algorithms that work in a decentralized and communication-efficient manner.
Peer-to-Peer (P2P) networks are gaining increasing popularity in many distributed applications such as file-sharing, network storage, web caching, sear- ching and indexing of relevant documents and P2P network-threat analysis. Many of these applications require scalable analysis of data over a P2P network. This paper starts by offering a brief overview of distributed data mining applications and algorithms for P2P environments. Next it discusses some of the privacy concerns with P2P data mining and points out the problems of existing privacy-preserving multi-party data mining techniques. It further points out that most of the nice assumptions of these existing privacy preserving techniques fall apart in real-life applications of privacy-preserving distributed data mining (PPDM). The paper offers a more realistic formulation of the PPDM problem as a multi-party game and points out some recent results.
This paper offers a local distributed algorithm for multivariate regression in large peer-to-peer environments. The algorithm is designed for distributed inferencing, data compaction, data modeling and classification tasks in many emerging peer-to-peer applications for bioinformatics, astronomy, social networking, sensor networks and web mining. Computing a global regression model from data available at the different peer-nodes using a traditional centralized algorithm for regression can be very costly and impractical because of the large number of data sources, the asynchronous nature of the peer-to-peer networks, and dynamic nature of the data/network. This paper proposes a two-step approach to deal with this problem. First, it offers an efficient local distributed algorithm that monitors the “quality ” of the current regression model. If the model is outdated, it uses this algorithm as a feedback mechanism for rebuilding the model. The local nature of the monitoring algorithm guarantees low monitoring cost. Experimental results presented in this paper strongly support the theoretical claims.
Inner product computation is an important primitive used in many techniques for feature dependency detection, distance computation, clustering and correlation computation among others. Recently, peer-to-peer networks are getting increasing attention in various applications involving distributed file sharing, sensor networks, and mobile ad hoc networks. Efficient identification of top few inner product entries from the entire inner product matrix of features in a distributed peer-to-peer network is a challenging problem since centralizing the data from all the nodes in a synchronous, communication efficient manner may not be an option. This paper deals with the problem of identifying significant inner products among features in a peer-to-peer environment where different nodes observe a different set of data. It uses an ordinal framework to develop probabilistic algorithms to find top-LaTeX elements in the inner product matrix. These l  inner product entries are important in making crucial decisions about dependency or relatedness between feature pairs, important for a number of data mining applications. In this paper we present experimental results demonstrating accurate and scalable performance of this algorithm for large peer-to-peer networks and also describe a real-world application for this algorithm.
This paper offers a scalable and robust distributed algorithm for decision-tree induction in large peer-to-peer (P2P) environments. Computing a decision tree in such large distributed systems using standard centralized algorithms can be very communication-expensive and impractical because of the synchronization requirements. The problem becomes even more challenging in the distributed stream monitoring scenario where the decision tree needs to be updated in response to changes in the data distribution. This paper presents an alternate solution that works in a completely asynchronous manner in distributed environments and offers low communication overhead, a necessity for scalability. It also seamlessly handles changes in data and peer failures. The paper presents extensive experimental results to corroborate the theoretical claims.
This paper offers a local distributed algorithm for multivariate regression in large peer-to-peer environments. The algorithm can be used for distributed inferencing, data compaction, data modeling and classification tasks in many emerging peer-to-peer applications for bioinformatics, astronomy, social networking, sensor networks and web mining. Computing a global regression model from data available at the different peer-nodes using a traditional centralized algorithm for regression can be very costly and impractical because of the large number of data sources, the asynchronous nature of the peer-to-peer networks, and dynamic nature of the data/network. This paper proposes a two-step approach to deal with this problem. First, it offers an efficient local distributed algorithm that monitors the quality  of the current regression model. If the model is outdated, it uses this algorithm as a feedback mechanism for rebuilding the model. The local nature of the monitoring algorithm guarantees low monitoring cost. Experimental results presented in this paper strongly support the theoretical claims.
In a large network of computers or wireless sensors, each of the components (henceforth, peers) has some data about the global state of the system. Much of the system's functionality such as message routing, information retrieval and load sharing relies on modeling the global state. We refer to the outcome of the function (e.g., the load experienced by each peer) as the emph{model} of the system. Since the state of the system is constantly changing, it is necessary to keep the models up-to-date. Computing global data mining models e.g. decision trees, k-means clustering in large distributed systems may be very costly due to the scale of the system and due to communication cost, which may be high. The cost further increases in a dynamic scenario when the data changes rapidly. In this paper we describe a two step approach for dealing with these costs. First, we describe a highly efficient emph{local} algorithm which can be used to monitor a wide class of data mining models. Then, we use this algorithm as a feedback loop for the monitoring of complex functions of the data such as its k-means clustering. The theoretical claims are corroborated with a thorough experimental analysis.
This paper considers the problem of change detection using local
distributed eigen monitoring algorithms for next generation
of astronomy petascale data pipelines such as the Large Synoptic
Survey Telescopes (LSST). This telescope will take repeat images
of the night sky every 20 seconds, thereby generating 30 terabytes of calibrated imagery every night that will need to be coanalyzed with other astronomical data stored at different locations around the world. Change point detection and event classification in such data sets may provide useful insights to unique astronomical phenomenon displaying astrophysically significant variations: quasars, supernovae, variable stars, and potentially hazardous asteroids. However, performing such data mining tasks is a challenging problem for such high-throughput distributed data streams. In this paper we propose a highly scalable and distributed asynchronous algorithm for monitoring the principal components (PC) of such dynamic data streams. We demonstrate the algorithm on a large set of distributed astronomical data to accomplish well-known astronomy tasks such as measuring variations in the fundamental plane of
galaxy parameters. The proposed algorithm is provably correct (i.e. converges to the correct PCs without centralizing any data) and can seamlessly handle changes to the data or the network. Real experiments performed on Sloan Digital Sky Survey (SDSS) catalogue data show the effectiveness of the algorithm.
This paper proposes a scalable, local privacy-preserving algorithm for distributed peer-to-peer (P2P) data aggregation useful for many advanced data mining/analysis tasks such as average/sum computation, decision tree induction, feature selection, and more. Unlike most multi-party privacy-preserving data mining algorithms, this approach works in an asynchronous manner through local interactions and therefore, is highly scalable. It particularly deals with the distributed computation of the sum of a set of numbers stored at different peers in a P2P network in the context of a P2P web mining application. The proposed optimization-based privacy-preserving technique for computing the sum allows different peers to specify different privacy requirements without having to adhere to a global set of parameters for the chosen privacy model. Since distributed sum computation is a frequently used primitive, the proposed approach is likely to have significant impact on many data mining tasks such as multi-party privacypreserving clustering, frequent itemset mining, and statistical aggregate computation.
The world-wide aviation system is one of the most complex dynamical systems ever developed and is generating data at an extremely rapid rate. Most modern commercial aircraft record several hundred flight parameters including information from the guidance, navigation, and control systems, the
avionics and propulsion systems, and the pilot inputs into the aircraft. These parameters may be continuous measurements or binary or categorical measurements recorded in one second intervals for the duration of the flight. Currently, most approaches to aviation safety are reactive, meaning
that they are designed to react to an aviation safety incident or accident. Here, we discuss a novel approach based on the theory of multiple kernel learning to detect potential safety anomalies in very large data bases of discrete and continuous data from world-wide operations of commercial fleets. We pose a general anomaly detection problem which includes both discrete and continuous data streams,
where we assume that the discrete streams have a causal influence on the continuous streams. We also assume that atypical sequence of events in the discrete streams can lead to off-nominal system performance. We discuss the application domain, novel algorithms, and also briefly discuss results on
synthetic and real-world data sets. Our algorithm uncovers operationally significant events in high dimensional data streams in the aviation industry which are not detectable using state of the art methods.
Air transportation, one of the most important modes of transportation, is also one of the safest. Nevertheless, the public demands that safety levels continuously improve and that the absolute number of aviation accidents continue to decline, even as air-traffic levels increase.  On February 12, 1997, after the tragedy of TWA 800, President William J. Clinton declared,
“We will achieve a national goal of reducing the fatal aircraft accident rate by 80% within 10 years.”
 
In response to this presidential declaration, the administrator of NASA announced that NASA would undertake a new program in aviation safety in support of this objective. NASA quickly formed the Aviation Safety Investment Strategy Team (ASIST) in collaboration with the Federal Aviation Administration (FAA) and the National Transportation Safety Board (NTSB), which organized a series of five workshops to examine the options and recommend an approach for NASA to develop the enabling technologies that address the president's goal. The exceptional and dedicated participation from all sectors of the aviation industry in the development of NASA’s strategy was remarkable.
This report describes a cooperative experiment conducted by ONERA and NASA, with the support of Airbus S.A.S. and easyJet Airline Company, Ltd. The study evaluated the benefits of two distinctly different methodologies for analyzing the same set of digital flight-recorded data. The experiment analyzed a set of easyJet commercial-flight data with both typical Flight Operational Quality Assur-ance (FOQA) software of an airline (in this case, AirFASE, developed by Airbus and Teledyne) and The Morning Report of Atypical Flights (developed by NASA). The study demonstrated the feasibility and potential value of using The Morning Report tool in conjunction with the FOQA airline tool and also showed the complementarities of the results produced by the two approaches.
This is a report on a continuing study of automated analyses of experiential textual reports to gain insight into the causal factors of human errors in aviation operations. The intent of this research is to
better understand the quantitative and qualitative attributes of an aviation incident, and to identify the respective contributions of their interaction to incident occurrence.
A proactive approach to identifying and alleviating life-threatening conditions in the aviation system entails a well-defined process of identifying threats, evaluating causes, assessing risks, and implementing appropriate solutions. This process is not a trivial undertaking. It requires continuous monitoring of system performance in a non-punitive culture; learning from normal operational experience; comparing actual performance to expected performance; identifying the precursor events and conditions that foreshadow most accidents; designing appropriate interventions to minimize the risk of their occurrence; and having a system in place to monitor the efficacy of the interventions.
Full title: Mining Distance-Based Outliers in Near Linear Time with Randomization and a Simple Pruning Rule

Abstract: Defining outliers by their distance to neighboring examples is a popular approach to finding unusual examples in a data set. Recently, much work has been conducted with the goal of finding fast algorithms for this task. We show that a simple nested loop algorithm that in the worst case is quadratic can give near linear time performance when the data is in random order and a simple pruning rule is used. We test our algorithm on real high-dimensional data sets with millions of examples and show that the near linear scaling holds over several orders of magnitude. Our average case analysis suggests that much of the efficiency is because the time to process non-outliers, which are the majority of examples, does not depend on the size of the data set.
Universal log-periodic correction to renormalization group scaling for rupture stress prediction from acoustic emissions.
Various instruments are used to create images of the Earth and other objects in the universe in a diverse set of wavelength bands with the aim of understanding natural phenomena. Sometimes these instruments are built in a phased approach, with additional measurement capabilities added in later phases. In other cases, technology may mature to the point that the instrument offers new measurement capabilities that were not planned in the original design of the instrument. In still other cases, high resolution spectral measurements may be too costly to perform on a large sample and therefore lower resolution spectral instruments are used to take the majority of measurements. Many applied science questions that are relevant to the earth science remote sensing community require analysis of enormous amounts of data that were generated by instruments with disparate measurement capabilities. This paper addresses this problem using Virtual Sensors: a method that uses modelstrained on spectrally rich (high spectral resolution) data to "fill in" unmeasured spectral channels in spectrally poor (low spectral resolution) data. The models we use in this paper are Multi-Layer Perceptrons (MLPs), Support Vector Machines (SVMs) with Radial Basis Function (RBF) kernels and SVMs with Mixture Density Mercer Kernels (MDMK). We demonstrate this method by using models trained on the high spectral resolution Terra MODIS instrument to estimate what the equivalent of the MODIS 1.6 micron channel would be for the NOAA AVHRR/2 instrument. The scientific motivation for the simulation of the 1.6 micron channel is to improve the ability of the AVHRR/2 sensor to detect clouds over snow and ice.
The automation of pre-launch diagnostics for launch vehicles offers three potential benefits: improving safety, reducing cost, and reducing launch delays. The Ares I-X Ground Diagnostic Prototype demonstrated anomaly detection, fault detection, fault isolation, and diagnostics for the Ares I-X first-stage Thrust Vector Control and for the associated ground hydraulics while the vehicle was in the Vehicle Assembly Building at Kennedy Space Center (KSC) and while it was on the launch pad. The prototype combines three existing tools. The first tool, TEAMS (Testability Engineering and Maintenance System), is a model-based tool from Qualtech Systems Inc. for fault isolation and diagnostics. The second tool, SHINE (Spacecraft Health Inference Engine), is a rule-based expert system that was developed at the NASA Jet Propulsion Laboratory. We developed SHINE rules for fault detection and mode identification, and used the outputs of SHINE as inputs to TEAMS. The third tool, IMS (Inductive Monitoring System), is an anomaly detection tool that was developed at NASA Ames Research Center. The three tools were integrated and deployed to KSC, where they were interfaced with live data. This paper describes how the prototype performed during the period before the launch, including accuracy and computer resource usage. The paper concludes with some of the lessons that we learned from the experience of developing and deploying the prototype.
Prior to the launch of STS-119 NASA had completed a study of an issue in the flow control valve (FCV) in the Main Propulsion System of the Space Shuttle using an adaptive learning method known as Virtual Sensors.  Virtual Sensors are a class of algorithms that estimate the value of a time series given other potentially nonlinearly correlated sensor readings.  In the case presented here, the Virtual Sensors algorithm is based on an ensemble learning approach and takes sensor readings and control signals as input to estimate the pressure in a subsystem of the Main Propulsion System.  Our results indicate that this method can detect faults in the FCV at the time when they occur.  We use the standard deviation of the predictions of the ensemble as a measure of uncertainty in the estimate.  This uncertainty estimate was crucial to understanding the nature and magnitude of transient characteristics during startup of the engine.   This paper overviews the Virtual Sensors algorithm and discusses results on a comprehensive set of Shuttle missions and also discusses the architecture necessary for deploying such algorithms in a real-time, closed-loop system or a human-in-the-loop monitoring system. These results were presented at a Flight Readiness Review of the Space Shuttle in early 2009.
We present a novel and general methodology for modeling time-varying vector autoregressive processes which are widely used in many areas such as modeling of chemical processes, mobile communication channels and biomedical signals. In the literature, most work utilize multivariate Gaussian models for the mentioned applications, mainly due to the lack of efficient analytical tools for modeling with non-Gaussian distributions. In this paper, we propose a particle filtering approach which can model non-Gaussian autoregressive processes having cross-correlations among them. Moreover, time-varying parameters of the process can be modeled as the most general case by using this sequential Bayesian estimation method. Simulation results justify the performance of the proposed technique, which potentially can model also Gaussian processes as a sub-case.
In this work, we present a novel method for modeling time-varying  autoregressive impulsive signals driven by symmetric alpha stable distributions. The proposed method can be interpreted as a two-stage Gibbs sampler composed of a particle filter, which is capable of estimating the unknown time-varying autoregressive coefficients, and a hybrid Monte Carlo method for estimating the unknown but constant  distribution parameters of a symmetric alpha stable process. This method is an alternative to a recently published technique in which both the autoregressive coefficients and the distribution parameters are estimated jointly within a single sequential Monte Carlo framework—the single particle filter technique. The proposed method achieves lower error variances in estimating the distribution parameters compared with the single sequential Monte Carlo technique, and thus, successfully models symmetric impulsive signals.
In the literature, impulsive signals are mostly modeled by symmetric alpha-stable processes. To represent their temporal dependencies, usually autoregressive models with time-invariant coefficients are utilized. We propose a general sequential Bayesian modeling methodology where both unknown autoregressive coefficients and distribution parameters can be estimated successfully, even when they are time-varying. In contrast to most work in the literature on signal processing with alpha-stable distributions, our work is general and models also skewed alpha-stable processes. Successful performance of our method is demonstrated by computer simulations. We support our empirical results by providing posterior Cramer–Rao lower bounds. The proposed method is also tested on a practical application where seismic data events are modeled.
Understanding the origins of life has been one of the greatest dreams throughout history. It is now known that star-forming regions contain complex organic molecules, known as Polycyclic Aromatic Hydrocarbons (PAHs), each of which has particular infrared spectral characteristics. By understanding which PAH species are found in specific star-forming regions, we can better understand the biochemistry that takes place in interstellar clouds. Identifying and classifying PAHs is not an easy task: we can only observe a single superposition of PAH spectra at any given astrophysical site, with the PAH species perhaps numbering in the hundreds or even thousands. This is a challenging source separation problem since we have only one observation composed of numerous mixed sources. However, it is made easier with the help of a library of hundreds of PAH spectra. In order to separate PAH molecules from their mixture, we need to identify the specific species and their unique concentrations that would provide the given mixture. We develop a Bayesian approach for this problem where sources are separated from their mixture by Metropolis Hastings algorithm. Separated PAH concentrations are provided with their error bars, illustrating the uncertainties involved in the estimation process. The approach is demonstrated on synthetic spectral mixtures using spectral resolutions from the Infrared Space Observatory (ISO). Performance of the method is tested for different noise levels.
Information-theoretic quantities, such as entropy, are used to quantify the amount of information a given variable provides.  Entropies can be used together to compute the mutual information, which quantifies the amount of information two variables share.  However, accurately estimating these quantities from data is extremely challenging. We have developed a set of computational techniques that allow one to accurately compute marginal and joint entropies.  These algorithms are probabilistic in nature and thus provide information on the uncertainty in our estimates, which enable us to establish statistical significance of our findings. We demonstrate these methods by identifying relations between cloud data from the International Satellite Cloud Climatology Project (ISCCP) and data from other sources, such as equatorial pacific sea surface temperatures (SST).
In the last decade alpha-stable distributions have become a
standard model for impulsive data. Especially the linear
symmetric alpha-stable processes have found applications in
various fields. When the process parameters are time-
invariant, various techniques are available for estimation.
However, time-invariance is an important restriction given
that in many communications applications channels are
time-varying. For such processes, we propose a relatively
new technique, based on particle filters which obtained great
success in tracking applications involving non-Gaussian
signals and nonlinear systems. Since particle filtering is a
sequential method, it enables us to track the time-varying
autoregression coefficients of the alpha-stable processes.
The method is tested both for abruptly and slowly changing
autoregressive parameters of signals, where the driving
noises are symmetric-alpha-stable processes and is observed
to perform very well. Moreover, the method can easily be
extended to skewed alpha-stable distributions.
In this paper, we propose a novel approach to reduce the noise in Synthetic Aperture Radar (SAR) images using particle filters. Interpretation of SAR images is a difficult problem, since they are contaminated with a multiplicative noise, which is known as the “Speckle Noise”. In literature, the general approach  for removing
the speckle is to use the local statistics, which are computed in a square window. Here, we propose to use particle filters, which is a sequential Bayesian technique. The proposed method also uses the local statistics to denoise the images. Since this is a Bayesian
approach, the computed statistics of the window can be exploited as a priori information. Moreover, particle filters are sequential methods, which are more appropriate to handle the heterogeneous structure of the image. Computer simulations show that the proposed method provides better edge-preserving results with
satisfactory speckle removal, when compared to the results obtained by Gamma Maximum a posteriori (MAP) filter.
In adaptive signal processing, joint process estimation plays
an important role in various estimation problems. It is well
known that a joint process estimator consists of two struc-
tures, namely the orthogonalizer and the regression filter. In
literature, orthogonalization step is performed either by or-
thogonal transformations or by linear predictors. While the
orthogonal transformations do not preserve entropy; the
predictors, such as the lattice, do preserve it. However, the
steady-state performance of such linear predictors is not as
good as those of the orthogonal transformations. Lattice
filters do not perform perfect orthogonalization when they
operate as gradient-based adaptive predictors. In this work,
adaptive escalator predictor is proposed to be used as the
orthogonalizer of the joint process estimator. The proposed
method preserves the entropy and achieves perfect orthogo-
nalization at all times. Moreover it has good steady-state
performance compared to those structures utilizing gradient
adaptive lattice filters.
In this work, we propose a novel approach to perform Dependent Component Analysis (DCA). DCA can be thought as the separation of latent, dependent sources from their observed mixtures which is a more realistic model than Independent Component Analysis (ICA) where the sources are assumed to be independent. In general, the sources can be spatio-temporally dependent and the mixing system may be non-stationary. Here, we propose a DCA algorithm, that combines concepts of particle filters and Markov Chain Monte Carlo (MCMC) methods in order to separate non-stationary mixtures of spatially dependent Gaussian sources.
In this paper we develop a local distributed privacy preserving algorithm for feature selection in a large peer-to-peer environment. Feature selection is often used in machine learning for data compaction and efficient learning by eliminating the curse of dimensionality. There exist many solutions for feature selection when the data is located at a central location. However, it becomes extremely challenging to perform the same when the data is distributed across a large number of peers or machines. Centralizing the entire dataset or portions of it can be very costly and impractical because of the large number of data sources, the asynchronous nature of the peer-to-peer networks,
dynamic nature of the data/network and privacy concerns. The solution proposed in this paper allows us to perform feature selection in an asynchronous fashion with a low communication overhead where each peer can specify its own privacy constraints. The algorithm works based on local interactions among participating nodes. We present results on real-world datasets in order to performance of the proposed algorithm.
not available
Abstract and Agenda book for CIDU 2010.
CLAIRE MONTELEONI*, GAVIN SCHMIDT**, AND SHAILESH SAROHA***

Climate models are complex mathematical models designed by meteorologists, geophysicists,
and climate scientists to simulate and predict climate. Given temperature predictions
from the top 20 climate models worldwide, and over 100 years of historical temperature data, we
track the changing sequence of which model currently predicts best. We use an algorithm due to
Monteleoni and Jaakkola that models the sequence of observations using a hierarchical learner,
based on a set of generalized Hidden Markov Models (HMM), where the identity of the current
best climate model is the hidden variable. The transition probabilities between climate models
are learned online, simultaneous to tracking the temperature predictions. On historical data, our
online learning algorithm’s average prediction loss nearly matches that of the best performing
climate model in hindsight. Moreover its performance surpasses that of the average model prediction,
which was the current state-of-the-art in climate science, the median prediction, and least
squares linear regression. We also experimented on climate model predictions through the year
2098. Simulating labels with the predictions of any one climate model, we found significantly improved
performance using our online learning algorithm with respect to the other climate models,
and techniques.
COMPLEX NETWORKS IN CLIMATE SCIENCE:
PROGRESS, OPPORTUNITIES AND CHALLENGES
KARSTEN STEINHAEUSER, NITESH V. CHAWLA, AND AUROOP R. GANGULY

Abstract. Networks have been used to describe and model a wide range of complex systems,
both natural as well as man-made. One particularly interesting application in the earth sciences
is the use of complex networks to represent and study the global climate system. In this paper,
we motivate this general approach, explain the basic methodology, report on the state of the art
(including our contributions), and outline open questions and opportunities for future research.
SPATIALLY ADAPTIVE SEMI-SUPERVISED LEARNING WITH GAUSSIAN
PROCESSES FOR HYPERSPECTRAL DATA ANALYSIS
GOO JUN * AND JOYDEEP GHOSH*


Abstract. A semi-supervised learning algorithm for the classification of hyperspectral data,
Gaussian process expectation maximization (GP-EM), is proposed. Model parameters for each
land cover class is first estimated by a supervised algorithm using Gaussian process regressions
to find spatially adaptive parameters, and the estimated parameters are then used to initialize a
spatially adaptive mixture-of-Gaussians model. The mixture model is updated by expectationmaximization
iterations using the unlabeled data, and the spatially adaptive parameters for unlabeled
instances are obtained by Gaussian process regressions with soft assignments. Two sets
of hyperspectral data taken from the Botswana area by the NASA EO-1 satellite are used for experiments.
Empirical evaluations show that the proposed framework performs significantly better
than baseline algorithms that do not use spatial information, and the results are also better than
any previously reported results by other algorithms on the same data.
IMPROVING CAUSE DETECTION SYSTEMS WITH ACTIVE LEARNING
ISAAC PERSING AND VINCENT NG

Abstract. Active learning has been successfully applied to many natural language processing
tasks for obtaining annotated data in a cost-effective manner. We propose several extensions to an
active learner that adopts the margin-based uncertainty sampling framework. Experimental results
on a cause detection problem involving the classification of aviation safety reports demonstrate
the effectiveness of our extensions.
Classification of Mars Terrain Using Multiple Data Sources

Alan Kraut1, David Wettergreen1

ABSTRACT. Images of Mars are being collected faster than they can be analyzed by planetary
scientists. Automatic analysis of images would enable more rapid and more consistent image
interpretation and could draft geologic maps where none yet exist. In this work we develop a
method for incorporating images from multiple instruments to classify Martian terrain into
multiple types. Each image is segmented into contiguous groups of similar pixels, called
superpixels, with an associated vector of discriminative features. We have developed and
tested several classification algorithms to associate a best class to each superpixel. These
classifiers are trained using three different manual classifications with between 2 and 6 classes.
Automatic classification accuracies of 50 to 80% are achieved in leave-one-out cross-validation
across 20 scenes using a multi-class boosting classifier.
SCALABLE TIME SERIES CHANGE DETECTION FOR BIOMASS
MONITORING USING GAUSSIAN PROCESS

VARUN CHANDOLA* AND RANGA RAJU VATSAVAI*

Abstract. Biomass monitoring, specifically, detecting changes in the biomass or vegetation of
a geographical region, is vital for studying the carbon cycle of the system and has significant
implications in the context of understanding climate change and its impacts. Recently, several time
series change detection methods have been proposed to identify land cover changes in temporal
profiles (time series) of vegetation collected using remote sensing instruments. In this paper, we
adapt Gaussian process regression to detect changes in such time series in an online fashion. While
Gaussian process (GP) has been widely used as a kernel based learning method for regression and
classification, their applicability to massive spatio-temporal data sets, such as remote sensing data,
has been limited owing to the high computational costs involved. In our previous work we proposed
an efficient Toeplitz matrix based solution for scalable GP parameter estimation. In this paper we
apply these solutions to a GP based change detection algorithm. The proposed change detection
algorithm requires a memory footprint which is linear in the length of the input time series and
runs in time which is quadratic to the length of the input time series. Experimental results show
that both serial and parallel implementations of our proposed method achieve significant speedups
over the serial implementation. Finally, we demonstrate the effectiveness of the proposed change
detection method in identifying changes in Normalized Difference Vegetation Index (NDVI) data.
ANALYZING AVIATION SAFETY REPORTS: FROM TOPIC MODELING TO
SCALABLE MULTI-LABEL CLASSIFICATION

AMRUDIN AGOVIC*, HANHUAI SHAN*, AND ARINDAM BANERJEE*

Abstract. The Aviation Safety Reporting System (ASRS) is used to collect voluntarily submitted
aviation safety reports from pilots, controllers and others. As such it is particularly useful
in researching aviation safety deficiencies. In this paper we address two challenges related to the
analysis of ASRS data: (1) the unsupervised extraction of meaningful and interpretable topics
from ASRS reports and (2) multi-label classification of ASRS data based on a set of predefined
categories. For topic modeling we investigate the practical usefulness of Latent Dirichlet Allocation
(LDA) when it comes to modeling ASRS reports in terms of interpretable topics. We also
utilize LDA to generate a more compact representation of ASRS reports to be used in multi-label
classification. For multi-label classification we propose a novel and highly scalable multi-label classification
algorithm based on multi-variate regression. Empirical results indicate that our approach
is superior to several baseline and state-of-the-art approaches.
OPTIMAL PARTITIONS OF DATA IN HIGHER DIMENSIONS

BRADLEY W. JACKSON*, JEFFREY D. SCARGLE**, AND CHRIS CUSANZA, DAVID BARNES, DENNIS
KANYGIN, RUSSELL SARMIENTO, SOWMYA SUBRAMANIAM, TZU-WANG CHUANG***

Abstract. Consider piece-wise constant approximations to a function of several parameters, and
the problem of finding the best such approximation from measurements at a set of points in the
parameter space. We find good approximate solutions to this problem in two steps: (1) partition
the parameter space into cells, one for each of the N data points, and (2) collect these cells into
blocks, such that within each block the function is constant to within measurement uncertainty.
We describe a branch-and-bound algorithm for finding the optimal partition into connected blocks,
as well as an O(N2) dynamic programming algorithm that finds the exact global optimum over this
exponentially large search space, in a data space of any dimension. This second solution relaxes
the connectivity constraint, and requires additivity and convexity conditions on the block fitness
function, but in practice none of these items cause problems. From the wide variety of intelligent
data understanding applications (including cluster analysis, classification, and anomaly detection)
we demonstrate two: partitioning of the State of California (2D) and the Universe (3D).
DISTRIBUTED ANOMALY DETECTION USING SATELLITE DATA FROM
MULTIPLE MODALITIES

KANISHKA BHADURI*, KAMALIKA DAS**, AND PETR VOTAVA***

Abstract. There has been a tremendous increase in the volume of Earth Science data over the
last decade from modern satellites, in-situ sensors and different climate models. All these datasets
need to be co-analyzed for finding interesting patterns or for searching for extremes or outliers.
Information extraction from such rich data sources using advanced data mining methodologies is
a challenging task not only due to the massive volume of data, but also because these datasets
ate physically stored at different geographical locations. Moving these petabytes of data over the
network to a single location may waste a lot of bandwidth, and can take days to finish. To solve this
problem, in this paper, we present a novel algorithm which can identify outliers in the global data
without moving all the data to one location. The algorithm is highly accurate (close to 99%) and
requires centralizing less than 5% of the entire dataset. We demonstrate the performance of the
algorithm using data obtained from the NASA MODerate-resolution Imaging Spectroradiometer
(MODIS) satellite images.
LUNAR TERRAIN AND ALBEDO RECONSTRUCTION FROM APOLLO
IMAGERY

ARA V NEFIAN*, TAEMIN KIM**, MICHAEL BROXTON**, AND ZACH MORATTO**

Abstract. Generating accurate three dimensional planetary models and albedo maps is becoming
increasingly more important as NASA plans more robotics missions to the Moon in the coming
years. This paper describes a novel approach for separation of topography and albedo maps
from orbital Lunar images. Our method uses an optimal Bayesian correlator to refine the stereo
disparity map and generate a set of accurate digital elevation models (DEM). The albedo maps
are obtained using a multi-image formation model that relies on the derived DEMs and the Lunar-
Lambert reflectance model. The method is demonstrated on a set of high resolution scanned
images from the Apollo era missions.
DATA MINING THE GALAXY ZOO MERGERS

STEVEN BAEHR*, ARUN VEDACHALAM*, KIRK BORNE*, AND DANIEL SPONSELLER*

Abstract. Collisions between pairs of galaxies usually end in the coalescence (merger) of the two
galaxies. Collisions and mergers are rare phenomena, yet they may signal the ultimate fate of
most galaxies, including our own Milky Way. With the onset of massive collection of astronomical
data, a computerized and automated method will be necessary for identifying those colliding
galaxies worthy of more detailed study. This project researches methods to accomplish that goal.
Astronomical data from the Sloan Digital Sky Survey (SDSS) and human-provided classifications
on merger status from the Galaxy Zoo project are combined and processed with machine learning
algorithms. The goal is to determine indicators of merger status based solely on discovering those
automated pipeline-generated attributes in the astronomical database that correlate most strongly
with the patterns identified through visual inspection by the Galaxy Zoo volunteers. In the end,
we aim to provide a new and improved automated procedure for classification of collisions and
mergers in future petascale astronomical sky surveys. Both information gain analysis (via the
C4.5 decision tree algorithm) and cluster analysis (via the Davies-Bouldin Index) are explored as
techniques for finding the strongest correlations between human-identified patterns and existing
database attributes. Galaxy attributes measured in the SDSS green waveband images are found to
represent the most influential of the attributes for correct classification of collisions and mergers.
Only a nominal information gain is noted in this research, however, there is a clear indication of
which attributes contribute so that a direction for further study is apparent.
KEYWORD SEARCH IN TEXT CUBE: FINDING TOP-K RELEVANT CELLS

BOLIN DING*, YINTAO YU*, BO ZHAO*, CINDY XIDE LIN*, JIAWEI HAN*, AND CHENGXIANG ZHAI*

Abstract. We study the problem of keyword search in a data cube with text-rich dimension(s)
(so-called text cube). The text cube is built on a multidimensional text database, where each row
is associated with some text data (e.g., a document) and other structural dimensions (attributes).
A cell in the text cube aggregates a set of documents with matching attribute values in a subset
of dimensions. A cell document is the concatenation of all documents in a cell. Given a keyword
query, our goal is to find the top-k most relevant cells (ranked according to the relevance scores of
cell documents w.r.t. the given query) in the text cube.
We define a keyword-based query language and apply IR-style relevance model for scoring and
ranking cell documents in the text cube. We propose two efficient approaches to find the top-k
answers. The proposed approaches support a general class of IR-style relevance scoring formulas
that satisfy certain basic and common properties. One of them uses more time for pre-processing
and less time for answering online queries; and the other one is more efficient in pre-processing and
consumes more time for online queries. Experimental studies on the ASRS dataset are conducted
to verify the efficiency and effectiveness of the proposed approaches.
PROBABILITY CALIBRATION BY THE MINIMUM AND MAXIMUM PROBABILITY
SCORES IN ONE-CLASS BAYES LEARNING FOR ANOMALY DETECTION

GUICHONG LI, NATHALIE JAPKOWICZ, IAN HOFFMAN, R. KURT UNGAR

ABSTRACT. One-class Bayes learning such as one-class Naïve Bayes and one-class Bayesian
Network employs Bayes learning to build a classifier on the positive class only for discriminating
the positive class and the negative class. It has been applied to anomaly detection for identifying
abnormal behaviors that deviate from normal behaviors. Because one-class Bayes classifiers can
produce probability score, which can be used for defining anomaly score for anomaly detection,
they are preferable in many practical applications as compared with other one-class learning
techniques. However, previously proposed one-class Bayes classifiers might suffer from poor
probability estimation when the negative training examples are unavailable. In this paper, we
propose a new method to improve the probability estimation. The improved one-class Bayes
classifiers can exhibits high performance as compared with previously proposed one-class Bayes
classifiers according to our empirical results.
A COMPARATIVE STUDY OF ALGORITHMS FOR LAND COVER CHANGE

SHYAM BORIAH*, VARUN MITHAL*, ASHISH GARG*, VIPIN KUMAR*, MICHAEL STEINBACH*,
CHRIS POTTER**, AND STEVE KLOOSTER***

Abstract. Ecosystem-related observations from remote sensors on satellites offer huge potential
for understanding the location and extent of global land cover change. This paper presents a
comparative study of three time series based algorithms for detecting changes in land cover. The
techniques are evaluated quantitatively using forest fire ground truth from the state of California
for 2000–2009. On relatively high quality data sets, all three schemes perform reasonably well,
but their ability to handle noise and natural variability in the vegetation data differs dramatically.
In particular, one of the algorithms significantly outperforms the other two since it accounts for
variability in the time series.
USAGE OF DISSIMILARITY MEASURES AND MULTIDIMENSIONAL SCALING FOR LARGE SCALE SOLAR DATA ANALYSIS

Juan M Banda, Rafal Anrgyk

ABSTRACT: This work describes the application of several dissimilarity measures combined with multidimensional scaling for large scale solar data analysis.  Using the first solar domain-specific benchmark data set that contains multiple types of phenomena, we investigated combination of different image parameters with different dissimilarity measure sin order to determine which combination will allow us to differentiate our solar data within each class and versus the rest of the classes. In this work we also address the issue of reducing dimensionality by applying multidimensional scaling to our dissimilarity matrices produced by the previously mentioned combination.  By applying multidimensional scaling we can investigate how many resulting components are needed in order to maintain a good representation of our data (in an artificial dimensional space) and how many can be discarded in order to economize our storage costs.  We present a comparative analysis between different classifiers in order to determine the amount of dimensionality reduction that can be achieved with said combination of image parameters, similarity measure and multidimensional scaling.
A KNOWLEDGE DISCOVERY STRATEGY FOR RELATING SEA SURFACE
TEMPERATURES TO FREQUENCIES OF TROPICAL STORMS AND
GENERATING PREDICTIONS OF HURRICANES UNDER 21ST-CENTURY
GLOBAL WARMING SCENARIOS

CAITLIN RACE*, MICHAEL STEINBACH*, AUROOP GANGULY**, FRED SEMAZZI***,
AND VIPIN KUMAR*

Abstract. The connections among greenhouse-gas emissions scenarios, global warming, and frequencies
of hurricanes or tropical cyclones are among the least understood in climate science
but among the most fiercely debated in the context of adaptation decisions or mitigation policies.
Here we show that a knowledge discovery strategy, which leverages observations and climate
model simulations, offers the promise of developing credible projections of tropical cyclones based
on sea surface temperatures (SST) in a warming environment. While this study motivates the
development of new methodologies in statistics and data mining, the ability to solve challenging
climate science problems with innovative combinations of traditional and state-of-the-art methods
is demonstrated. Here we develop new insights, albeit in a proof-of-concept sense, on the relationship
between sea surface temperatures and hurricane frequencies, and generate the most likely
projections with uncertainty bounds for storm counts in the 21st-century warming environment
based in turn on the Intergovernmental Panel on Climate Change Special Report on Emissions
Scenarios. Our preliminary insights point to the benefits that can be achieved for climate science
and impacts analysis, as well as adaptation and mitigation policies, by a solution strategy that
remains tailored to the climate domain and complements physics-based climate model simulations
with a combination of existing and new computational and data science approaches.
UNDERSTANDING SEVERE WEATHER PROCESSES THROUGH
SPATIOTEMPORAL RELATIONAL RANDOM FORESTS

AMY MCGOVERN, TIMOTHY SUPINIE, DAVID JOHN GAGNE II, NATHANIEL TROUTMAN,
MATTHEW COLLIER, RODGER A. BROWN, JEFFREY BASARA, AND JOHN K. WILLIAMS

Abstract. Major severe weather events can cause a significant loss of life and property. We
seek to revolutionize our understanding of and ability to predict such events through the mining
of severe weather data. Because weather is inherently a spatiotemporal phenomenon, mining
such data requires a model capable of representing and reasoning about complex spatiotemporal
dynamics, including temporally and spatially varying attributes and relationships. We introduce
an augmented version of the Spatiotemporal Relational Random Forest, which is a Random Forest
that learns with spatiotemporally varying relational data. Our algorithm maintains the strength
and performance of Random Forests but extends their applicability, including the estimation of
variable importance, to complex spatiotemporal relational domains. We apply the augmented
Spatiotemporal Relational Random Forest to three severe weather data sets. These are: predicting
atmospheric turbulence across the continental United States, examining the formation of tornadoes
near strong frontal boundaries, and understanding the translation of drought across the southern
plains of the United States. The results on such a wide variety of real-world domains demonstrate
the extensive applicability of the Spatiotemporal Relational Random Forest. Our long-term goal
is to significantly improve the ability to predict and warn about severe weather events.
ADAPTIVE MODEL REFINEMENT
FOR THE IONOSPHERE AND THERMOSPHERE

ANTHONY M. D’AMATO∗, AARON J. RIDLEY∗∗, AND DENNIS S. BERNSTEIN∗∗∗

Abstract. Mathematical models of physical phenomena are of critical importance in
virtually all applications of science and technology. This paper addresses the problem of
how to use data to improve the fidelity of a given model. We approach this problem using
retrospective cost optimization, a novel technique that uses data to recursively update an
unknown subsystem interconnected to a known system. Applications of this research are
relevant to a wide range of applications that depend on large-scale models based on firstprinciples
physics, such as the Global Ionosphere-Thermosphere Model (GITM). Using
GITM as the truth model, we demonstrate that measurements can be used to identify
unknown physics. Specifically, we estimate static thermal conductivity parameters, and
we identify a dynamic cooling process.
PADMINI: A PEER-TO-PEER DISTRIBUTED ASTRONOMY DATA MINING
SYSTEM AND A CASE STUDY

TUSHAR MAHULE*, KIRK BORNE**, SANDIPAN DEY*, SUGANDHA ARORA*,
AND HILLOL KARGUPTA***

Abstract. Peer-to-Peer (P2P) networks are appealing for astronomy data mining from virtual
observatories because of the large volume of the data, compute-intensive tasks, potentially large
number of users, and distributed nature of the data analysis process. This paper offers a brief
overview of PADMINI—a Peer-to-Peer Astronomy Data MINIng system. It also presents a case
study on PADMINI for distributed outlier detection using astronomy data. PADMINI is a webbased
system powered by Google Sky and distributed data mining algorithms that run on a
collection of computing nodes. This paper offers a case study of the PADMINI evaluating the
architecture and the performance of the overall system. Detailed experimental results are presented
in order to document the utility and scalability of the system.
MULTI-TEMPORAL REMOTE SENSING IMAGE CLASSIFICATION - A
MULTI-VIEW APPROACH

VARUN CHANDOLA* AND RANGA RAJU VATSAVAI*

Abstract. Multispectral remote sensing images have been widely used for automated land use
and land cover classification tasks. Often thematic classification is done using single date image,
however in many instances a single date image is not informative enough to distinguish between
different land cover types. In this paper we show how one can use multiple images, collected at
different times of year (for example, during crop growing season), to learn a better classifier. We
propose two approaches, an ensemble of classifiers approach and a co-training based approach, and
show how both of these methods outperform a straightforward stacked vector approach often used
in multi-temporal image classification. Additionally, the co-training based method addresses the
challenge of limited labeled training data in supervised classification, as this classification scheme
utilizes a large number of unlabeled samples (which comes for free) in conjunction with a small
set of labeled training data.
MULTI-LABEL ASRS DATASET CLASSIFICATION USING SEMI-SUPERVISED
SUBSPACE CLUSTERING

MOHAMMAD SALIM AHMED, LATIFUR KHAN, NIKUNJ OZA, AND MANDAVA RAJESWARI

Abstract. There has been a lot of research targeting text classification. Many of them focus
on a particular characteristic of text data - multi-labelity. This arises due to the fact that a
document may be associated with multiple classes at the same time. The consequence of such a
characteristic is the low performance of traditional binary or multi-class classification techniques on
multi-label text data. In this paper, we propose a text classification technique that considers this
characteristic and provides very good performance. Our multi-label text classification approach
is an extension of our previously formulated [3] multi-class text classification approach called
SISC (Semi-supervised Impurity based Subspace Clustering). We call this new classification model
as SISC-ML(SISC Multi-Label). Empirical evaluation on real world multi-label NASA ASRS
(Aviation Safety Reporting System) data set reveals that our approach outperforms state-of-theart
text classification as well as subspace clustering algorithms.
not available
Link to Sharepoint website containing a repository of more detailed internal information for authorized users
Sample data, including nominal and faulty scenarios, for Diagnostic Problems I and II of the Second International Diagnostic Competition. Three file formats are provided, tab-delimited .txt files, Matlab .mat files, and tab-delimited .scn files. The scenario (.scn) files are read by the DXC framework. See the Second International Diagnostic Competition project page for more information.
Competition data, including nominal and faulty scenarios, for Diagnostic Problems I and II of the Second International Diagnostic Competition. Three file formats are provided, tab-delimited .txt files, Matlab .mat files, and tab-delimited .scn files. The scenario (.scn) files are read by the DXC framework. See the DXC'10 Industrial Track Sample Data resource page for additional documentation, including system catalogs and schematics.
The DXC Framework is a collection of programs and APIs for running and evaluating diagnostic algorithms (DAs) under identical experimental conditions. It is complementary to system XML catalogs and data sets. 

The Oracle is new to DXC'10 and provides a querying capability to the DAs to determine the correct actions for given faults. Because the oracle uses proprietary NASA software, it is provided only in binary form. Thus the framework is available as a windows binary installer, linux source files + binary oracle, or windows source files +
binary oracle. Please see the included READMEs and example DAs for more information.
Results for the DXC'10 Industrial Track.
A framework to compare and evaluate diagnosis algorithms (DAs) has been created jointly by NASA Ames Research Center, Palo Alto Research Center, and Delft University of Technology. In this paper, we present the second implementation of this framework in a competition called DXC’10. The overall goal of this competition is to evaluate the performance of different diagnostic methods.  In order to accurately mimic diagnostic technology use in a real-world context, we have defined diagnostic problems driven by use cases representing different roles of diagnosis results. In the end, the competition pitted seven DAs competing in two diagnostic problems. The paper presents the systems used in DXC’10, a description of faults and data sets used for each diagnostic problem, a listing of participating DAs, the performance metrics and results computed from running the DAs with the framework, and an analysis of the results.
Slides presented at DXC'10 session of 21st International Workshop on Principles of Diagnosis
FLTz flight simulator RecorderRun9 data are analyzed in order 
to compute systems health score using Granger causal connectovity 
analysis. First G-causality is computed, and then causal density (cd) is 
computed in interval [0,1].  Numerical value of causal density for this data file is 0.4711, which corresponds to systems health score.
Multivariate Time-Series (MTS) are ubiquitous, and are generated in areas as disparate as sensor recordings in aerospace systems, music and video streams, medical monitoring, and financial systems. Domain experts are often interested in searching for interesting multivariate patterns from these MTS databases which can contain up to several gigabytes of data. Surprisingly, research on MTS search is very limited. Most existing work only supports queries with the same length of data, or queries on a fixed set of variables. In this paper, we propose an efficient and flexible subsequence search framework for massive MTS databases, that, for the first time, enables querying on any subset of variables with arbitrary time delays between them. We propose two provably correct algorithms to solve this problem — (1) an R-tree Based Search (RBS) which uses Minimum Bounding Rectangles (MBR) to organize the subsequences, and (2) a List Based Search (LBS) algorithm which uses sorted lists for indexing. We demonstrate the performance of these algorithms using two large MTS databases from the aviation domain, each containing several millions of observations. Both these tests show that our algorithms have very high prune rates (>95%) thus needing actual disk access for only less than 5% of the observations. To the best of our knowledge, this is the first flexible MTS search algorithm capable of subsequence search on any subset of variables. Moreover, MTS subsequence search has never been attempted on datasets of the size we have used in this paper.
This paper describes a local and distributed expectation maximization algorithm for learning parameters of Gaussian mixture models (GMM) in large peer-to-peer (P2P)
environments. The algorithm can be used for a variety of well-known data mining tasks in distributed environments such as clustering, anomaly detection, target tracking, and
density estimation to name a few, necessary for many emerging P2P applications in bioinformatics, webmining and sensor networks. Centralizing all or some of the data to build global models is impractical in such P2P environments because of the large number of data sources, the asynchronous nature of the P2P networks, and dynamic nature of the data/network. The proposed algorithm takes a two-step approach. In the
monitoring phase, the algorithm checks if the model ‘quality’ is acceptable by using an efficient local algorithm. This is then
used as a feedback loop to sample data from the network and rebuild the GMM when it is outdated. We present thorough experimental results to verify our theoretical claims.
In this paper we propose ν-Anomica, a novel
anomaly detection technique that can be trained on huge data sets with much reduced running time compared to the benchmark one-class Support Vector Machines algorithm.
In ν-Anomica, the idea is to train the machine such that it can provide a close approximation to the exact decision
plane using fewer training points and without losing much of the generalization performance of the classical approach. We have tested the proposed algorithm on a variety of continuous data sets under different conditions. We show that under all test conditions the developed
procedure closely preserves the accuracy of standard oneclass Support Vector Machines while reducing both the training time and the test time by 5 − 20 times.
Consider a scenario in which the data owner has some private/sensitive data and wants a data miner to access it for studying important patterns without revealing the sensitive information. Privacy preserving data mining aims to solve this problem by randomly transforming the data prior to its release to data miners. Previous work only considered the case of linear data perturbations — additive, multiplicative or a combination of both for studying the usefulness of the perturbed output. In
this paper, we discuss nonlinear data distortion using potentially nonlinear random data transformation and show how it can be
useful for privacy preserving anomaly detection from sensitive datasets. We develop bounds on the expected accuracy of the
nonlinear distortion and also quantify privacy by using standard definitions. The highlight of this approach is to allow a user
to control the amount of privacy by varying the degree of nonlinearity. We show how our general transformation can be used for anomaly detection in practice for two specific problem instances: a linear model and a popular nonlinear model using the sigmoid function. We also analyze the proposed nonlinear transformation in full generality and then show that for specific
cases it is distance preserving. A main contribution of this paper is the discussion between the invertibility of a transformation
and privacy preservation and the application of these techniques to outlier detection. Experiments conducted on real-life datasets
demonstrate the effectiveness of the approach.
There has been a tremendous increase in the volume of Earth Science data over the last decade from modern satellites, in-situ sensors and different climate models. All these datasets need to be co-analyzed for finding interesting patterns or for searching for extremes or outliers. Information extraction from such rich data sources using advanced data mining methodologies is
a challenging task not only due to the massive volume of data, but also because these datasets are physically stored at different geographical locations. Moving these petabytes of data over the network to a single location may waste a lot of bandwidth, and can take days to finish. To solve this
problem, in this paper, we present a novel algorithm which can identify outliers in the global data without moving all the data to one location. The algorithm is highly accurate (close to 99%) and requires centralizing less than 5% of the entire dataset. We demonstrate the performance of the
algorithm using data obtained from the NASA MODerate-resolution Imaging Spectroradiometer
(MODIS) satellite images.
This paper proposes a scalable, local privacy preserving algorithm for distributed Peer-to-Peer (P2P) data aggregation useful for many advanced data mining/analysis tasks such as average/sum computation, decision tree induction, feature selection, and more.
Unlike most multi-party privacy-preserving data mining algorithms, this approach works in an asynchronous manner through local interactions and it is highly scalable. It particularly deals with the distributed computation of the sum of a set of numbers stored at different peers in a P2P network in the context of a P2P web mining application. The proposed optimization based privacy-preserving technique for computing the sum allows different peers to specify different privacy requirements without having to adhere to a global set of parameters for the chosen privacy model. Since distributed sum computation is a frequently used primitive,
the proposed approach is likely to have significant impact on many data mining tasks such as multi-party privacy-preserving clustering, frequent itemset mining, and statistical aggregate computation.
Sample data, including nominal and faulty scenarios, for Tier 1 and Tier 2 of the First International Diagnostic Competition. Three file formats are provided, tab-delimited .txt files, Matlab .mat files, and tab-delimited .scn files. The scenario (.scn) files are read by the DXC framework. See the Support/Documentation section below and the First International Diagnostic Competition project page for more information.
Competition data, including nominal and faulty scenarios, for Industrial Track Tier 1 and Tier 2 of the First International Diagnostic Competition. Three file formats are provided, tab-delimited .txt files, Matlab .mat files, and tab-delimited .scn files. The scenario (.scn) files are read by the DXC framework. See the DXC'09 Industrial Track Sample Data resource page for additional documentation, including system catalogs and schematics.

Note that a "rematch" took place after the competition at the DX-09 Workshop. The rematch data consisted of the data for the original competition plus new data sets taken specifically for the rematch.
Sample data for the DXC'09 Synthetic Track.
Synthetic Track Competition Data
Results for DXC'09
Diagnostic inference involves the detection of anomalous system behavior and the identification of its cause, possibly down to a failed unit or to a parameter of a failed unit. Traditional approaches to solving this problem include expert/rule-based, model-based, and data-driven methods. Each approach (and various techniques within each approach) use different representations of the knowledge required to perform the diagnosis. The sensor data is expected to be combined with these internal representations to produce the diagnosis result. In spite of the availability of various diagnosis technologies, there have been only minimal efforts to develop a standardized software framework to run, evaluate, and compare different diagnosis technologies on the same system. This paper presents a framework that defines a standardized representation of the system knowledge, the sensor data, and the form of the diagnosis results – and provides a run-time architecture that can execute diagnosis algorithms, send sensor data to the algorithms at appropriate time steps from a variety of sources (including the actual physical system), and collect resulting diagnoses. We also define a set of metrics that can be used to evaluate and compare the performance of the algorithms, and provide software to calculate the metrics.
A framework to compare and evaluate diagnosis algorithms (DAs) has been created jointly by NASA Ames Research Center and PARC. In this paper, we present the first concrete implementation of this framework as a competition called DXC’09. The goal of this competition was to evaluate and compare DAs in a common platform and to determine a winner based on diagnosis results. 12 DAs (model-based and otherwise) competed in this first year of the competition in 3 tracks that included industrial and synthetic systems. Specifically, the participants provided algorithms that communicated with the run-time architecture to receive scenario data and return diagnostic results. These algorithms were run on extended scenario data sets (different from sample set) to compute a set of pre-defined metrics. A ranking scheme based on weighted metrics was used to declare winners. This paper presents the systems used in DXC’09, description of faults and data sets, a listing of participating DAs, the metrics and results computed from running the DAs, and a superficial analysis of the results.
A variety of rule-based, model-based and datadriven
techniques have been proposed for detection
and isolation of faults in physical systems.
However, there have been few efforts to comparatively
analyze the performance of these approaches
on the same system under identical conditions.
One reason for this was the lack of a standard
framework to perform this comparison. In this paper
we introduce a framework, called DXF, that
provides a common language to represent the system
description, sensor data and the fault diagnosis
results; a run-time architecture to execute
the diagnosis algorithms under identical conditions
and collect the diagnosis results; and an evaluation
component that can compute performance
metrics from the diagnosis results to compare the
algorithms. We have used DXF to perform an empirical
evaluation of 13 diagnostic algorithms on a
hardware testbed (ADAPT) at NASA Ames Research
Center and on a set of synthetic circuits
typically used as benchmarks in the model-based
diagnosis community. Based on these empirical
data we analyze the performance of each algorithm
and suggest directions for future development.
Slides presented at DXC'09 session of 20th International Workshop on Principles of Diagnosis
The finite element model being used by the AePW is based on the model provided at 
[**HIRENASD website**](https://heinrich.lufmech.rwth-aachen.de/index.php?lang=en&pg=home)

The NASTRAN FEM's using HEXA solid elements and identified as "structured"(str) is the one that will be used.  Another exists which uses TETRA elements and is labeled "unstructured"(unstr).  The original FEM's as provided on the website had different coordinate systems and are in different units. 
<LI> str = mm 
<LI> unstructured = meters

The coordinate systems for each of the FEM are different also.  To facilitate use both FEM's were modified so that the x direction is in the flow direction, y - is out the wing and z is goes from lower surface to upper surface of the wing and the models are in meters. 

Mode shapes and frequencies were calculated with both FEM's and a frequency comparison is provided.  The only model NASA has used is the "str" model.   

Comparisons of the FEM as provided from HIRENASD website with as modified are <a href="https://c3.ndc.nasa.gov/dashlink/static/media/dataset/HIRENASD_coordinate_system_2.pdf">provided</a>

<TABLE>
<TR><TD>
<img src="https://c3.ndc.nasa.gov/dashlink/static/media/other/CoordinateSystem_StructuredFEM.jpg">
</TD></TR>
<TR><TD>
<img src="https://c3.ndc.nasa.gov/dashlink/static/media/other/CoordinateSystem_UnstructuredFEM.jpg">
</TD></TR></TABLE>
not available
Prognostic performance evaluation has gained significant attention in the past few years.*Currently, prognostics concepts lack standard definitions and suffer from ambiguous and inconsistent interpretations. This lack of standards is in part due to the varied end- user requirements for different applications, time scales, available information, domain dynamics, etc. to name a few. The research community has used a variety of metrics largely based on convenience and their respective requirements. Very little attention has been focused on establishing a standardized approach to compare different efforts. This paper presents several new evaluation metrics tailored for prognostics that were recently introduced and were shown to effectively evaluate various algorithms as compared to other conventional metrics. Specifically, this paper presents a detailed discussion on how these metrics should be interpreted and used. These metrics have the capability of incorporating probabilistic uncertainty estimates from prognostic algorithms. In addition to quantitative assessment they also offer a comprehensive visual perspective that can be used in designing the prognostic system. Several methods are suggested to customize these metrics for different applications. Guidelines are provided to help choose one method over another based on distribution characteristics. Various issues faced by prognostics and its performance evaluation are discussed followed by a formal notational framework to help standardize subsequent developments.
The problem of monitoring a multivariate linear regression model is relevant in studying the evolving relationship between a set of input variables (features) and one or more dependent target variables. This problem becomes challenging for large scale data in a distributed computing environment when only a subset of instances is available at individual nodes and the local data changes frequently. Data centralization and periodic model recomputation can add high overhead to tasks like anomaly detection in such dynamic settings. Therefore, the goal is to develop techniques for monitoring and updating the model over the union of all nodes' data in a communication-efficient fashion. Correctness guarantees on such techniques are also often highly desirable, especially in safety-critical application scenarios. In this paper we develop <i>DReMo</i> --- a distributed algorithm  with very low resource overhead, for monitoring the quality of a regression model in terms of its coefficient of determination (<i>R2</i> statistic). When the nodes collectively determine that <i>R2</i> has dropped below a fixed threshold, the linear regression model is recomputed via a network-wide convergecast and the updated model is broadcast back to all nodes. We show empirically, using both synthetic and real data, that our proposed method is highly communication-efficient and scalable, and also provide theoretical guarantees on correctness.
Regression problems on massive data sets are ubiquitous in many application domains including the Internet, earth and space sciences, and finances. In many cases, regression algorithms such as linear regression or neural networks attempt to fit the target variable as a function of the input variables without regard to the underlying joint distribution of the variables. As a result, these global models are not sensitive to variations in the local structure of the input space. Several algorithms, including the mixture of experts model, classification and regression trees (CART), and others have been developed, motivated by the fact that a variability in the local distribution of inputs may be reflective of a significant change in the target variable. While these methods can handle the non-stationarity in the relationships to varying degrees, they are often not scalable and, therefore, not used in large scale data mining applications. In this paper we develop Block-GP, a Gaussian Process regression framework for multimodal data, that can be an order of magnitude more scalable than existing state-of-the-art nonlinear regression algorithms. The framework builds local Gaussian Processes on semantically meaningful partitions of the data and provides higher prediction accuracy than a single global model with very high confidence. The method relies on approximating the covariance matrix of the entire input space by smaller covariance matrices that can be modeled independently, and can therefore be parallelized for faster execution. Theoretical analysis and empirical studies on various synthetic and real data sets show high accuracy and scalability of Block-GP compared to existing nonlinear regression techniques.
Computational Unsteady Aerodynamics computer codes are being increasingly used. In order to
validate their results they must be tested against valid experimental data. The present report aims at
collecting reliable experimental data on unsteady aerodynamics and presenting them in a form
which permits use for verification of codes. For ease of handling, the data are also presented in
machine readable form (CD-ROM). Data on increasingly complex generic forms were selected and
the following categories are covered: flutter, buffet, stability and control, dynamic stall, cavity
flows, store separation. Computational solutions are included in order to permit evaluation of codes
and analysis of solutions which differ from experimental data.
<b>Benchmark Supercritical Wing</b> was also tested on the OTT with oscillations in Pitch.  Only one row of pressure transducers were acquired during these tests.  The time histories for this test (548) are available

The Physical Properties of the BSCW (Benchmark Supercritical Wing are provided in <a href="https://c3.ndc.nasa.gov/dashlink/static/media/other/NASA_TM4457_BSCW.pdf">
NASA TM 4457</a> published 1993.  Note the previous file that was loaded to this website did not have the tables.

Some results for the test are provided in <a href="https://c3.ndc.nasa.gov/dashlink/static/media/other/AIAA_2002-0171_OTT.pdf">AIAA 2002-0171</a> and <a href="https://c3.ndc.nasa.gov/dashlink/static/media/other/AIAA-JA_Vol40_no1_Piatak_OTT.pdf">JOURNAL OF AIRCRAFT article</a>
<b>Rectangular Supercritical Wing (Ricketts)</b> - design and measured locations are provided in an Excel file <a href="https://c3.ndc.nasa.gov/dashlink/static/media/dataset/RSW_airfoil_coordinates_ricketts.xls">RSW_airfoil_coordinates_ricketts.xls</a> .  One sheet is with Non dimensional coordinates (RSW-nd) to be able to compare with other supercritical airfoils.  The other sheet (RectSupercriticalWing) has the data which should be used to generate the grids.

<b>Benchmark Supercritical Wing</b> are available in PDF file of tables. The data was OCR'd.   Matlab code was written to read data line by line to be able to extract the data.  The "*" flag associated with points that have deviation greater the specified value were replaced with blank space.  Bad lines were omitted - lines that have non-numerical digits.  


Comparison of Rectangular Supercritical Wing (Ricketts), Benchmark Supercritical Wing, MBB_A3

<img src="https://c3.ndc.nasa.gov/dashlink/static/media/dataset/SCWairfoils.png">

2D Airfoil tested at DLR - comparison of theoretical and actual.
<img src="
https://c3.ndc.nasa.gov/dashlink/static/media/dataset/mbb_a3.png" height=200>
not available
not available
not available
not available
not available
not available
not available
not available
With the forecast increase in air traffic demand over the next decades, it is imperative to develop tools to provide traffic flow managers with the information required to support decision making. In particular, decision-support tools for traffic flow management should aid in limiting controller workload and complexity, while supporting increases in air traffic throughput. While many decision-support tools exist for short-term traffic planning, few have addressed the strategic needs for medium- and long-term planning for time horizons greater than 30 minutes. This paper seeks to address this gap through the introduction of 3D aircraft proximity maps that evaluate the future probability of presence of at least one or two aircraft at any given point of the airspace. Three types of proximity maps are presented: presence maps that indicate the local density of traffic; conflict maps that determine locations and probabilities of potential conflicts; and outliers maps that evaluate the probability of conflict due to aircraft not belonging to dominant traffic patterns. These maps provide traffic flow managers with information relating to the complexity and difficulty of managing an airspace. The intended purpose of the maps is to anticipate how aircraft flows will interact, and how outliers impact the dominant traffic flow for a given time period. This formulation is able to predict which "critical" regions may be subject to conflicts between aircraft, thereby requiring careful monitoring. These probabilities are computed using a generative aircraft flow model. Time-varying flow characteristics, such as geometrical configuration, speed, and probability density function of aircraft spatial distribution within the flow, are determined from archived Enhanced Traffic Management System data, using a tailored clustering algorithm. Aircraft not belonging to flows are identified as outliers.
This paper discusses the effect of sequential conflict resolution maneuvers of an infinite aircraft flow through a finite control volume. Aircraft flow models are utilized to simulate traffic flows and determine stability. Pseudo-random flow geometry is considered to determine airspace stability in a more random airspace, where aircraft flows are spread over a given positive width. The use of this aircraft flow model generates a more realistic flow geometry. A set of upper bounds on the maximal aircraft deviation during conflict resolution is derived. Also with this flow geometry it is proven that these bounds are not symmetric, unlike the symmetric bounds derived in previous papers for simpler flow configurations. Stability is preserved under sequential conflict resolution algorithms for all flow geometries discussed in this paper.
This paper takes an empirical approach
to identify operational factors at busy airports that
may predate go-around maneuvers. Using four years
of data from San Francisco International Airport, we
begin our investigation with a statistical approach
to investigate which features of airborne, ground
operations (e.g., number of inbound aircraft, number
of aircraft taxiing from gate, etc.) or weather are
most likely to fluctuate, relative to nominal operations,
in the minutes immediately preceding a missed
approach. We analyze these findings both in terms
of their implication on current airport operations
and discuss how the antecedent factors may affect
NextGen. Finally, as a means to assist air traffic controllers,
we draw upon techniques from the machine
learning community to develop a preliminary alert
system for go-around prediction.
This paper presents a framework aimed at monitoring
the behavior of aircraft in a given airspace. Trajectories
that constitute typical operations are determined and learned
using data driven methods. Standard procedures are used by air
traffic controllers (ATC) to guide aircraft, ensure the safety of the
airspace, and to maximize the runway occupancy. Even though
standard procedures are used by ATC, the control of the aircraft
remains with the pilots, leading to a large variability in the flight
patterns observed. Two methods to identify typical operations
and their variability from recorded radar tracks are presented.
This knowledge base is then used to monitor the conformance
of current operations against operations previously identified as
typical. A tool called AirTrajectoryMiner is presented, aiming at
monitoring the instantaneous health of the airspace, in real time.
The airspace is “healthy” when all aircraft are flying according
to the typical operations. A measure of complexity is introduced,
measuring the conformance of current flight to typical flight
patterns. When an aircraft does not conform, the complexity
increases as more attention from ATC is required to ensure a
safe separation between aircraft.
A method to quantify the probabilistic controller taskload inherent to maintaining aircraft adherence to 4-D trajectories within flow corridors is presented. An Ornstein-
Uhlenbeck model of the aircraft motion and a Poisson model of the flow scheduling are introduced along with reasonable numerical values of the model parameters. Analytic expressions are derived for the taskload probability density functions for basic functional elements of the flow structure. Monte Carlo simulations are performed for these basic functional elements and the controller taskload probabilities are exhibited.
Model-based diagnosis typically uses
analytical redundancy to compare predictions from a model against observations from the system being diagnosed. However this approach does not work very well when it is not feasible to create analytic relations describing all the observed data, e.g., for vibration data which is usually sampled at very high rates and requires very detailed finite element models to describe its behavior. In such cases, features (in time and frequency domains) that contain diagnostic information are extracted from the data. Since this is a computationally intensive process, it is not efficient to extract all the features all the time. In this paper we present an approach that combines the analytic model-based and feature-driven diagnosis approaches. The analytic approach is used to reduce the set of possible faults and then features are chosen to best distinguish among the remaining faults. We describe an implementation of this approach on the Flyable Electro-mechanical Actuator (FLEA) test bed.
With the advent of the next generation of aerospace systems equipped with fly-by-wire controls, electro- mechanical actuators (EMA) are quickly becoming components critical to safety of aerospace vehicles. Being relatively new to the field, however, EMA lack the knowledge base compared to what is accumulated for the more traditional actuator types, especially when it comes to fault detection and prognosis. Scarcity of health monitoring data from fielded systems and prohibitive costs of carrying out real flight tests create the need to build high-fidelity system models and design affordable yet realistic experimental setups. The objective of this work is to build an EMA test stand that, unlike current laboratory stands typically weighing in excess of one metric ton, is portable enough to be easily placed aboard a wide variety of aircraft. This stand, named the FLEA (for Flyable Electro- mechanical Actuator test stand), allows testing EMA fault detection and prognosis technologies in flight environment, thus substantially increasing their technology readiness level – all without the expense of dedicated flights, as the stand is designed to function as a non-intrusive secondary payload. No aircraft modifications are required and data can be collected during any available flight opportunity: pilot currency flights, ferry flights, or flights dedicated to other experiments. The stand is currently equipped with a prototype version of NASA Ames developed prognostic health management system with models aimed at detecting and tracking several fault types. At this point the team has completed test flights of the stand on US Air Force C-17 aircraft and US Army UH-60 helicopters and more experiments, both laboratory and airborne, are planned for the coming months.
This is the code for fast discriminative latent Dirichlet allocation, which is an algorithm for topic modeling and text classification. The related paper is at http://www-users.cs.umn.edu/~shan/icdm09_dm.pdf
Response to the FAA request for comments on zero accidents. The responses propose estimating the age-specific field reliability of all aircraft service parts, not just safety-or-fracture- critical parts tracked by hours and cycles. Proposal includes an example. The proposal is still valid.
NASA researchers recently demonstrated
successful real-time fault detection and isolation of a virtual reusable launch vehicle main propulsion system. Using a detailed simulation of a vehicle propulsion system to produce synthesized sensor readings, the NASA team demonstrated that advanced diagnostic algorithms, running on flight-like computers, can, in real time, successfully diagnose the presence and cause of faults.
This demonstration was conducted as part of the NASA Propulsion IVHM Technology Experiment, or PITEX.
not available
Data collected on a UH-60 helicopter on nominal (Y) and jam-injected (X) actuators.
Dataset collected in laboratory conditions on actuators with a jammed ballscrew return channel and actuators with a failed motor.
This is the publically accessible website for AePW

What will be posted here:

## Outline:

<ol>
<LI>Rectangular Supercritical Wing</LI>
<LI>Benchmark Supercritical Wing</LI>
<LI>HIRENASD</LI>
</ol>
    A.  Grids  
    A.  Grids  
    A.  Grids
    B.  Finite Element Models or grids and modal deflections

<a href="
https://c3.ndc.nasa.gov/dashlink/projects/39/"> Organizing Committee</a>
not available
Table explaining the naming convention and parameters of FLEA experiments performed in the laboratory.
The Multiple Kernel Anomaly Detection (MKAD) algorithm is designed for anomaly detection over a set of files. It combines multiple kernels into a single optimization function using the One Class Support Vector Machine (OCSVM) framework. Any kernel function can be combined in the algorithm as long as it meets the Mercer conditions, however for the purposes of this code the data preformatting and kernel type is specific to the Flight Operations Quality Assurance (FOQA) data and has been integrated into the coding steps.  For this domain, discrete binary switch sequences are used in the discrete kernel, and discretized continuous parameter features are used to form the continuous kernel. The OCSVM uses a training set of nominal examples (in this case flights) and evaluates test examples for anomaly detection to determine whether they are anomalous or not. After completing this analysis the algorithm reports the anomalous examples and determines whether there is a contribution from either or both continuous and discrete elements.
This is a resource where HTML files will be stored for the website
This contains the list of all important figures and concepts my research work is based on.
IGES files
Grids
Validation Data
not available
Grid resource link goes here

[**IGES file**](https://c3.ndc.nasa.gov/dashlink/static/media/dataset/hirenasd_AePW_DLR.igs.gz)

[**Finite element model**](https://c3.ndc.nasa.gov/dashlink/resources/274/)


[**Beam model**](https://c3.ndc.nasa.gov/dashlink/resources/401/)

[**Modes and Frequencies at a reduced set of nodes**](https://c3.nasa.gov/dashlink/resources/400/)

Experimental data link goes here
not available
This will contain publications used by the AePW
Nominal, ballscrew jam fault, and spall fault scenarios (diagnostic and prognostic)
Ballscrew jam fault datasets (diagnostic and prognostic)
not available
Images for the website main pages and all configurations.
The upload and access points for the other images are:
<center><h1><font color="#DF01A5><a href="https://c3.nasa.gov/dashlink/resources/836/" > Website Template </a> </font></h1> </center>

<center><h1><font color="#DF01A5><a href="https://c3.nasa.gov/dashlink/resources/837/" > 
RSW images </a> </font></h1> </center>

<center><h1><font color="#DF01A5><a href="https://c3.nasa.gov/dashlink/resources/838/" > BSCW Images </a> </font></h1> </center>

<center><h1><font color="#DF01A5><a href="https://c3.nasa.gov/dashlink/resources/839/" > HIRENASD Images </a> </font></h1> </center>
Documentation of tests conducted at NASA TDT of Rectangular Supercritical wing test in the 1980's and documented in RTO Report 26.  More results are also published in other references.  Time history data for this test (TDT Test number 353) is not available.
not available
not available
Under files is the link to the RTI wiki. 

Research Test and Integration (RTI) focuses on the development of long term plans for test and integration opportunities for research products from the SSAT, VSST, and AEST projects. RTI planning is primarily focused on AvSafe projects, however collaboration also includes other NASA programs, other government agencies, as well as industry and academic partners. This Wiki is intended to document the Research Test and Integration Plan (RTIP). The purpose of RTIP is to keep track of significant AvSafe research activities and maintain a database of testing facilities and assets available to enable and enhance the AvSafe research milestones. In addition RTIP will facilitate the development of collaborative research testing plans. This research collaboration will enable pooling research and test activities where possible. This pooling of research and test activities has the possibility of creating benefits that include: 

1. increasing the Technology Readiness Level for test activities with little or no additional cost to perform the tests, 
2. improving the quality of research activities by increasing the quantity of data sets available to researchers through the acquisition of test data via ride-along test activities which add little or no additional cost, and 
3. increasing the overall knowledge base by improving communication among principal investigators and research partners while reducing the duplication of work.
A primary goal to design smart homes is to provide automatic assistance for the residents to make them able to live independently at home.  Activity recognition is done to achieve the mentioned goal and then to provide assistance, we would need three sort of information. First, we would need to know the goal of the resident, then the pattern that the resident should obey to achieve its goal and third sort of needed information is the deviations from the previously known patterns.  In the presented paper, spatiotemporal aspects of daily activities are surveyed to mine the patterns of activities realized by the smart homes residents.  Necessary data to model the spatiotemporal aspects of daily activities is provided by embedded sensors in the smart home. We believe that to accomplish daily activities, specific objects are applied and by analyzing the movement of objects and resident(s), we would obtain valuable information to model the daily activities of the Smart Home’s residents.
In this paper, we develop a distributed algorithm for monitoring the principal components (PCs) for next generation
of astronomy petascale data pipelines such as the Large Synoptic Survey Telescopes (LSST). This telescope will take repeated
images of the night sky every 20 s, thereby generating 30 terabytes of calibrated imagery every night that will need to be
co-analyzed with other astronomical data stored at different locations around the world. Event detection, classification, and
isolation in such data sets may provide useful insights to unique astronomical phenomenon displaying astrophysically significant
variations: quasars, supernovae, variable stars, and potentially hazardous asteroids. However, performing such data mining tasks
is a challenging problem for such high-throughput distributed data streams. In this paper, we propose a highly scalable and
distributed asynchronous algorithm for monitoring the PCs of such dynamic data streams and discuss a prototype web-based
system PADMINI (Peer-to-Peer Astronomy Data Mining) which implements this algorithm for use by the astronomers. We
demonstrate the algorithm on a large set of distributed astronomical data to accomplish well-known astronomy tasks such as
measuring variations in the fundamental plane of galaxy parameters. The proposed algorithm is provably correct (i.e., converges
to the correct PCs without centralizing any data) and can seamlessly handle changes to the data or the network. Real experiments
performed on Sloan Digital Sky Survey (SDSS) catalogue data show the effectiveness of the algorithm.
There has been a tremendous increase in the volume of sensor data collected over the last decade
for different monitoring tasks. For example, petabytes of earth science data are collected from modern
satellites, in-situ sensors and different climate models. Similarly, huge amount of flight operational data
is downloaded for different commercial airlines. These different types of datasets need to be analyzed
for finding outliers. Information extraction from such rich data sources using advanced data mining
methodologies is a challenging task not only due to the massive volume of data, but also because these
datasets are physically stored at different geographical locations with only a subset of features available
at any location. Moving these petabytes of data to a single location may waste a lot of bandwidth.
To solve this problem, in this paper, we present a novel algorithm which can identify outliers in the
entire data without moving all the data to a single location. The method we propose only centralizes
a very small sample from the different data subsets at different locations. We analytically prove and
experimentally verify that the algorithm offers high accuracy compared to complete centralization with
only a fraction of the communication cost. We show that our algorithm is highly relevant to both earth
sciences and aeronautics by describing applications in these domains. The performance of the algorithm
is demonstrated on two large publicly available datasets: (1) the NASA MODIS satellite images and (2) a
simulated aviation dataset generated by the ‘Commercial Modular Aero-Propulsion System Simulation’ (CMAPSS).
Coarse grid for node-based unstructured methods using mixed-elements based on the grid guidelines.
Medium grid for node-based unstructured methods using mixed-elements based on the grid guidelines.
This is the fully tetra coarse mesh for the RSW based on gridding guidelines.
This is the fully tetra medium mesh for the RSW based on gridding guidelines.
This dataset is the fully tetrahdral fine mesh for the RSW configuration.
This is the RSW Mixed Element Unstructured Fine Grid Set.
not available
Unstructured HIRENASD mesh:
- medium size (16 million nodes, 39 million elements)
- for node centered solvers
- 31.05.2011
- caution: dimensions in mm
blockstructured hexahedral grid, 6.7 mio elements, 24 degree minimum grid angle, CGNS format version 2.4, double precision

Binary, Plot3D file

Please contact Thorsten Hansen for information about these files/grids.
Unstructured HIRENASD mesh:
- coarse size (5.7 million nodes, 14.4 million elements)
- for node centered solvers
- 01.06.2011
- caution: dimensions in mm
Over the last several years researchers at NASA Glenn and Ames Research Centers have developed a real-time fault detection and isolation system for propulsion subsystems of future space vehicles. The Propulsion IVHM Technology Experiment (PITEX), as it is called follows the model-based diagnostic methodology and employs Livingstone, developed at NASA Ames, as its reasoning engine. The system has been tested on flight-like hardware through a series of nominal and fault scenarios. These scenarios have been developed using a highly detailed simulation of the X-34 flight demonstrator main propulsion system and include realistic failures involving valves, regulators, microswitches, and sensors. This paper focuses on one of the recent research and development
efforts under PITEX – to provide more complete transient region coverage. It describes the development of the transient monitors, the corresponding modeling methodology, and the interface software responsible for coordinating the flow of information between the quantitative monitors and the qualitative, discrete representation in Livingstone.
The Propulsion IVHM Technology Experiment (PITEX) has been an on-going research effort conducted over several
years. PITEX has developed and applied a model-based diagnostic system for the main propulsion system of the X-34
reusable launch vehicle, a space-launch technology demonstrator. The application was simulation-based using detailed models of the propulsion subsystem to generate nominal and failure scenarios during captive carry, which is the most safety-critical portion of the X-34 flight. Since no system-level testing of the X-34 Main Propulsion System (MPS) was performed, these simulated data were used to verify and validate the software system. Advanced diagnostic and signal processing algorithms were developed and tested in real-time on flight-like hardware. In an attempt to expose potential performance problems, these PITEX algorithms were subject to numerous real-world effects in the simulated data including noise, sensor resolution, command/valve talkback information, and nominal build variations. The current research has demonstrated the potential benefits of model-based diagnostics, defined the performance metrics required to evaluate the diagnostic system, and studied the impact of real-world challenges encountered when monitoring
propulsion subsystems.
Few human endeavors present as much of a planning and scheduling challenge as space flight, particularly manned space flight. Just on the operational side of it, efforts of thousands of people across hundreds of organizations need
to be coordinated. Numerous tasks of varying complexity and nature, from scientific to construction, need to be
accomplished within limited mission time frames. Resources need to be carefully managed and contingencies worked out, often on a very short notice. From the beginning of the NASA space program, planning has been done by large teams of domain experts working
months, sometimes years, to put together a single mission. This approach, while proven very reliable up to now, is becoming increasingly harder to sustain. Elevated levels of
NASA space activities, from deployment of the new Crew
Exploration Vehicle (CEV) and completion of the
International Space Station (ISS), to the planned lunar
missions and permanent lunar bases, will put an even
greater strain on this largely manual process. While several
attempts to automate it have been made in the past, none
have fully succeeded. In this paper we describe the current
NASA planning methods, outline their advantages and
disadvantages, discuss the planning challenges of upcoming
missions and propose a distributed planning/scheduling
framework (CMMD) aimed at unifying and optimizing the
planning effort. CMMD will not attempt to make the
process completely automated, but rather serve in a decision
support capacity for human managers and planners. It will
help manage information gathering, creation of partial and
consolidated schedules, inter-team negotiations,
contingencies investigation, and rapid re-planning when the
situation demands it. The first area of CMMD application
will be planning for Extravehicular Activities (EVA) and
associated logistics. Other potential applications, not only
in the space flight domain, and future research efforts will
be discussed as well.
execute plans and schedules that achieve stated goals while simultaneously minimizing the cost of logistics management and maximizing resource productivity. This goal is a challenge in space flight environments where just-in-time logistics management can’t be supported and large scale planning and scheduling requires collaborations and negotiations that aross many divisions and departments. Although there have been many systems proposed and/or developed that address one or more of these concerns, a key element missing in these systems is the
tight coupling that is necessary between maintenance, logistics, and operations. This close relationship is particularly important in space operations where changes to scheduled missions and/or the logistics chain can greatly impact overall operations. Based on previous work on combined maintenance and operations planning/scheduling for Marine
Aviation, we propose a software-based infrastructure that coordinates planning, scheduling, and execution across multiple departments and disciplines.
The Drilling Automation for Mars Environment (DAME) project, led by NASA Ames Research Center, is aimed at developing a lightweight, low-power drill prototype that can be mounted on a Mars lander and be capable of drilling down several meters below the Mars surface for conducting geology and astrobiology research. The DAME drill system incorporates a large degree of autonomy - from quick diagnosis of system state and fault conditions to making the appropriate recovery actions - while also striving to achieve as many of the operational objectives as possible. This paper outlines, on a general level, the overall DAME architecture, equipment, and autonomy package. The main focus, however, is on describing the model-based fault detection and diagnosis system, including the modeling approach, the fault modes handled, and the diagnostic algorithms. The results of the latest field tests, conducted in 2006 in Haughton Crater on Devon Island (a Mars analogue site in Canadian Arctic), are also discussed.
Expanded deployment of Electro-Mechanical Actuators (EMAs) in critical applications has created much interest in EMA Prognostic Health Management (PHM), a key enabling technology of Condition Based Maintenance (CBM). As such, Impact Technologies, LLC is collaborating with the NASA Ames Research Center to perform a number of research efforts in support of NASA’s Integrated Vehicle Health Management (IVHM) initiatives. These efforts have combined experimental test stand development, laboratory seeded fault testing, and physical model-based health monitoring in a comprehensive PHM
system development strategy. This paper discusses two closely related EMA research programs being conducted by
Impact and NASA Ames. The first of these efforts resulted in the creation of an electro-mechanical actuator test stand for the Prognostics Center of Excellence at the NASA Ames Research Center. The second effort is ongoing and is utilizing physics-based modeling techniques to develop an algorithm and software package toolset for PHM of aircraft EMA systems using a hybrid (virtual sensor) approach.