Transmission of CO2 in the atmosphere of Venus for the spectral region near ten micrometers

Details Transmission of CO2 in the atmosphere of Venus for the spectral region near ten micrometers Transmission of CO2 in the atmosphere of Venus for the spectral region near ten micrometers

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icar...43..102y&link_type=abstract

Icarus, vol. 43, July 1980, p. 102-110.

Mathematics

Atmospheric Models, Carbon Dioxide, Gas Transport, Venus Atmosphere, Atmospheric Composition, Gas Pressure, High Temperature Gases, Spectral Bands, Temperature Effects, Vibrational Spectra, Venus, Atmosphere, Carbon Dioxide, Spectrum, Mathematical Models, Data, Comparisons, Optical Properties, Wavelengths, Temperatures, Intensity

Scientific paper

A total of 145 vibration-rotation bands are used to compute the transmission for a clear Venus atmosphere in the region near 10 microns. Synthetic spectra for each layer of a seven-layer model atmosphere show that the atmosphere is effectively black below 40 km above the surface. Comparison of calculated transmission with laboratory measurements shows good agreement up to 759 K.

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