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

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989spie.1157...93h&link_type=abstract

IN: Infrared technology XV; Proceedings of the Meeting, San Diego, CA, Aug. 7-9, 1989 (A90-44129 19-35). Bellingham, WA, Society

Physics

Background Radiation, Far Ultraviolet Radiation, Remote Sensing, Ultraviolet Detectors, Airglow, Auroras, Light Scattering

Scientific paper

The airglow, scattering, and auroral emission sources of the VUV background of the earth's atmosphere set limits on the usefulness of UV space observations, but facilitate such passive remote sensing types as electron density profiling and auroral location and strength determinations, which are presently discussed. UV auroral imaging has to date been conducted by four different experiments: (1) the VUV Backgrounds observations (flown on the S3-4 satellite in 1978); (2) the Horizon UV Program experiment (flown on STS-4 in 1982); the HILAT satellite's Atmospheric/Ionospheric Monitor (1986); and the Atmospheric/Ionospheric Remote Sensor (flown on the Polar BEAR satellite, 1988-1989).

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