The rotationally resolved 3400- to 3800-A terrestrial nightglow

Details The rotationally resolved 3400- to 3800-A terrestrial nightglow The rotationally resolved 3400- to 3800-A terrestrial nightglow

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jgr....88.4137s&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 88, May 1, 1983, p. 4137-4139.

Physics

16

Computerized Simulation, Emission Spectra, Nightglow, Oxygen Spectra, Terrestrial Radiation, Electron Transitions, Line Spectra, Molecular Relaxation, Molecular Rotation, Spectrum Analysis, Venus (Planet)

Scientific paper

Analysis and synthesis have been performed on portions of unpublished ground-based nightglow spectra taken at ≡0.5 Å resolution by A. L. Broadfoot in 1968. The bands of the three O2 systems radiating in the 3400- to 3800-Å region are rotationally resolved, and lines from three different c1Σu-→X3Σg- bands, the system that dominates the visible Venusian nightglow, are clearly identified.

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