Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993spie.1764..142a&link_type=abstract
In: Ultraviolet technology IV; Proceedings of the Meeting, San Diego, CA, July 20, 21, 1992 (A93-34426 13-35), p. 142-150.
Astronomy and Astrophysics
Astronomy
Atmospheric Composition, Electron Emission, Electron Impact, Iue, Planetary Atmospheres, Ultraviolet Astronomy, Configuration Interaction, Ultraviolet Spectrometers, Upper Atmosphere
Scientific paper
In recognition of the need for accurate collision cross-sections suitable for modeling spectroscopic observations of the planetary systems and calibrate flight instruments, NASA-JPL has determined the laboratory emission cross-sections of H, H2, N2, SO2, etc. Resonance excitation, predissociation, and non-Franck-Condon band intensity systems are determined by configuration interaction and must be taken into account in analyses of spacecraft observations. Attention is given to the application of the cross-sectional data obtained to both electron energy loss codes and models of Voyager, IUE, Galileo, and HST observations of the solar system.
Ajello Joseph M.
James Geoffrey K.
Kanik Inanc
Shemansky Don E.
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