The Venus nitric oxide night airglow - Model calculations based on the Venus Thermospheric General Circulation Model

Details The Venus nitric oxide night airglow - Model calculations based on the Venus Thermospheric General Circulation Model The Venus nitric oxide night airglow - Model calculations based on the Venus Thermospheric General Circulation Model

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....95.6271b&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 95, May 1, 1990, p. 6271-6284. Research supported by FNRS.

Physics

41

Atmospheric General Circulation Models, Nightglow, Nitric Oxide, Thermosphere, Ultraviolet Radiation, Venus Atmosphere, Pioneer Venus 1 Spacecraft, Solar Activity, Ultraviolet Spectrometers, Venus, Nitric Oxide, Airglow, Models, Calculations, Thermosphere, Circulation, Spacecraft Observations, Pvo Mission, Ouvs Instrument, Nightside, Brightness, Emissions, Nitrogen, Transport, Parameters, Density, Photochemistry, Diagrams, Chemistry, Eddy Diffusion, Solar Cycles

Scientific paper

The mechanism responsible for the Venus nitric oxide (0,1) delta band nightglow observed in the Pioneer Venus Orbiter UV spectrometer (OUVS) images was investigated using the Venus Thermospheric General Circulation Model (Dickinson et al., 1984), modified to include simple odd nitrogen chemistry. Results obtained for the solar maximum conditions indicate that the recently revised dark-disk average NO intensity at 198.0 nm, based on statistically averaged OUVS measurements, can be reproduced with minor modifications in chemical rate coefficients. The results imply a nightside hemispheric downward N flux of (2.5-3) x 10 to the 9th/sq cm sec, corresponding to the dayside net production of N atoms needed for transport.

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