Radiative heat transfer in the atmosphere of Venus

Details Radiative heat transfer in the atmosphere of Venus Radiative heat transfer in the atmosphere of Venus

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980dossr.251r1345k&link_type=abstract

(Akademiia Nauk SSSR, Doklady, vol. 251, no. 6, 1980, p. 1345-1349.) Soviet Physics - Doklady, vol. 25, Apr. 1980, p. 221-223. T

Physics

Atmospheric Diffusion, Radiative Heat Transfer, Venus Atmosphere, Pioneer Venus Spacecraft, Temperature Profiles, Venera Satellites, Venus Clouds, Vertical Distribution

Scientific paper

Pioneer-Venus and Venera probe data are used to examine radiative heat transfer in the Venusian atmosphere. A vertical temperature profile in the approximations of radiative-adiabatic and radiative equilibria of the atmosphere is obtained, and a radiative flux profile is presented. Results show that the cloud/haze optical model of Kondrat'ev et al. (1980) is suitable for the interpretation of radiative heat fluxes in the 0-90 km height range.

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