Physics
Scientific paper
Jan 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..261c&link_type=abstract
(Middle and upper atmosphere results; Proceedings of the Topical Meeting of the Interdisciplinary Scientific Commission C /Meeti
Physics
Airglow, Dayglow, Extreme Ultraviolet Radiation, Oxygen Atoms, San Marco Satellites, Solar Spectra, Solar Flux, Solar Spectrometers, Solar Terrestrial Interactions, Space Plasmas, Upper Atmosphere
Scientific paper
The mechanisms governing the interactions between two of the fundamental components of the solar-terrestrial system - solar ionizing radiation and the earth's upper atmosphere - are investigated. The physical parameters of the EUV emissions resulting from these interactions are characterized so that EUV remote sensing can gainfully be employed as a quantitative diagnostic of the terrestrial atmosphere and plasma environment. This analysis uses the solar flux measurements of the Airglow and Solar Spectrometer Instrument (ASSI) on board the San Marco D/L satellite. Preliminary modeling results of the altitude and zenith angle distribution of these emissions are presented along with the data.
Chakrabarti Sangeeta
Cotton Daniel M.
Gladstone Randall G.
Kent Tobiska W.
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