The thermal balance of the atmosphere of Venus

Details The thermal balance of the atmosphere of Venus The thermal balance of the atmosphere of Venus

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ssrv...20..389t&link_type=abstract

Space Science Reviews, vol. 20, June 1977, p. 389-412.

Physics

1

Atmospheric Heat Budget, Atmospheric Temperature, Venus Atmosphere, Exosphere, Infrared Radiometers, Insolation, Pioneer Venus Spacecraft, Pioneer Venus 1 Spacecraft, Radiant Flux Density, Radiative Heat Transfer, Venus Clouds, Vertical Distribution, Wind Measurement

Scientific paper

Current knowledge of the temperature structure of the atmosphere of Venus is briefly summarized. The principal features to be explained are the high surface temperature, the small horizontal temperature contrasts near the cloud tops in the presence of strong apparent motions, and the low value of the exospheric temperature. In order to understand the role of radiative and dynamical processes in maintaining the thermal balance of the atmosphere, a great deal of additional data on the global temperature structure, solar and thermal radiation fields, structure and optical properties of the clouds, and circulation of the atmosphere are needed. The ability of the Pioneer Venus Orbiter and Multiprobe Missions to provide these data is indicated.

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