Vacuum ultraviolet backgrounds from space - ten years after

Details Vacuum ultraviolet backgrounds from space - ten years after Vacuum ultraviolet backgrounds from space - ten years after

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989stin...9012493h&link_type=abstract

Presented at the 33rd SPIE Symposium, San Diego, CA, 6-11 Aug. 1989

Computer Science

Auroras, Earth Atmosphere, Electron Density Profiles, Far Ultraviolet Radiation, Vacuum, Data Processing, Earth (Planet), Images, Observation, Position (Location), Remote Sensors, Sun

Scientific paper

The past ten years has seen progress in the understanding of the ultraviolet background of the earth's atmosphere. These airglow, auroral, and scattering emission sources set limits on the usefulness of UV for space observations. They also, however, enable several types of passive remote sensing; such as, electron density profiles, neutral density and composition, and auroral location and strength. The paper describes our measurements and data analysis in these areas. UV imaging of the aurora has been achieved by four experiments, and these are briefly reviewed. UV imaging has opened up a new way to study solar-terrestrial relationships.

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