Ultraviolet night airglow of Venus

Details Ultraviolet night airglow of Venus Ultraviolet night airglow of Venus

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979sci...205...59s&link_type=abstract

Science, vol. 205, July 6, 1979, p. 59-62.

Computer Science

19

Airglow, Nitric Oxide, Pioneer Venus Spacecraft, Ultraviolet Spectra, Venus Atmosphere, Abundance, Atmospheric Composition, Carbon Dioxide, Iue, Nitrogen Atoms, Oxygen Atoms, Radiative Recombination, Thermosphere, Circulation, Gamma Rays, Delta Rays, Dayside, Venus, Pioneer Venus, Ultraviolet, Airglow, Emissions, Oxygen, Nitrogen, Thermosphere, Nitric Oxides, Limbs, Brightness, Nightside

Scientific paper

The night airglow spectrum of Venus in the ultraviolet is dominated by the V-prime = 0 progressions of the gamma and delta bands of nitric oxide. The bands are produced by two-body radiative recombination of nitrogen and oxygen atoms. Since the source of these atoms is in the dayside thermosphere, the night airglow is a tracer of the day-to-night thermospheric circulation. The airglow is brightest at equatorial latitudes and at longitudes on the morning side of the antisolar meridian.

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