Transmission of CO2 in the atmosphere of Venus for the spectral region near 7 microns

Details Transmission of CO2 in the atmosphere of Venus for the spectral region near 7 microns Transmission of CO2 in the atmosphere of Venus for the spectral region near 7 microns

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982icar...51..606y&link_type=abstract

Icarus, vol. 51, Sept. 1982, p. 606-609.

Physics

Optics

4

Atmospheric Attenuation, Atmospheric Boundary Layer, Atmospheric Models, Carbon Dioxide, Infrared Absorption, Venus Atmosphere, Absorption Spectra, Atmospheric Optics, Atmospheric Radiation, Brightness Temperature, Electric Dipoles

Scientific paper

The transmission in the 7-micron 'window' of Venus was calculated for a 7-layer model atmosphere. The synthetic spectra show that radiation from the layer 20-30 km above the surface would reach the top of the atmosphere between 6.2 and 7.0 microns if there were no absorption besides the isotopic CO2 bands; for the 7.0- to 8.2-micron region, the radiating level would be located 40-50 km above the surface of Venus. The brightness temperature for the entire region is 430 K; for the above two regions it is 494 and 341 K, respectively.

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