Computer Science
Scientific paper
May 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..103....1p&link_type=abstract
Icarus (ISSN 0019-1035), vol. 103, no. 1, p. 1-42.
Computer Science
136
Infrared Spectroscopy, Near Infrared Radiation, Night Sky, Spectroscopic Analysis, Venus Atmosphere, Airglow, Emission Spectra, Nightglow, Radiative Transfer, Spectral Bands, Venus, Nightside, Near-Infrared, Wavelength, Spectroscopy, Emissions, Simulation, Atmosphere, Scattering, Absorption, Gases, Depth, Clouds, Abundance, Optical Properties, Thickness, Spectra, Mixing, Gradient, Comparison, Theoretical Studies, Opacity, Procedure, Radiative Transfer, Parameters, Altitude, Pressure, Temperature, Intensity,
Scientific paper
The near-IR spectra of the Venus nightside emission are here simulated by means of a radiative transfer code that allows for emission, absorption, and scattering by atmospheric gases and particles. An effort is made to assess the adequacy of current gas data bases in simulating Venus' nightside near-IR spectra and, within these limitations, to derive information on gas abundances below the main clouds and these clouds' optical thickness. It is in this way established that the HITRAN data base for the permitted transitions of CO2 is completely inadequate for simulating the Venus nightside near-IR emissions.
Allen David A.
Bezard Bruno
Crisp Dave
Dalton James Bradley
de Bergh Catherine
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