Radiative transfer in the 2.86-4.16 micron transparence window in the Venus atmosphere

Details Radiative transfer in the 2.86-4.16 micron transparence window in the Venus atmosphere Radiative transfer in the 2.86-4.16 micron transparence window in the Venus atmosphere

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977kosis..15..747a&link_type=abstract

Kosmicheskie Issledovaniia, vol. 15, Sept.-Oct. 1977, p. 747-754. In Russian.

Physics

Atmospheric Windows, Infrared Spectra, Radiative Transfer, Venus Atmosphere, Absorptivity, Carbon Dioxide, Spectral Bands, Transparence, Vertical Distribution

Scientific paper

Thermal radiation fluxes were calculated for the 2.86-4.16 micron transparence window of the Venus atmosphere using new experimental data on the absorption coefficients of stimulated, weak IR and isotopic bands of CO2, which enter the window. It is found that consideration of absorption in these bands leads to a reduction of an order of magnitude in the effective flux.

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