Physics
Scientific paper
May 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agusmsa51a..11s&link_type=abstract
American Geophysical Union, Spring Meeting 2002, abstract #SA51A-11
Physics
7538 Solar Irradiance, 0310 Airglow And Aurora, 0355 Thermosphere: Composition And Chemistry, 0358 Thermosphere: Energy Deposition, 2423 Ionization Mechanisms
Scientific paper
The Solar EUV Experiment (SEE) on the Thermosphere-Ionosphere-Mesosphere Energetics and Dynamics (TIMED) spacecraft is performing the first comprehensive measurements of the extreme-ultraviolet and soft X-ray region of the solar spectrum since the end of the Atmosphere Explorer (AE) mission in 1981. Comparison of TIMED/SEE measurements to contemporaneous satellite observations and a calibration rocket shows that solar irradiance in the soft X-ray and hard EUV spectral ranges, from about 2 to 25 nm, is much more intense than the AE-era observations. Using these new results as inputs to thermosphere/ionosphere models causes revisions to predicted photoelectron fluxes, ionization rates, electron density, ion composition, odd-nitrogen composition, and airglow emission rates. We compare predictions to measurements for some of these, including ground based measurements of ionospheric parameters during the first phase of the TIMED mission and far-ultraviolet dayglow limb profiles measured by the GUVI instrument.
Bailey Scott M.
Christensen Andrew B.
Eparvier Francis G.
Gladstone Randall G.
Paxton Larry J.
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