Physics – Atmospheric and Oceanic Physics
Scientific paper
Sep 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977fizao..13r.204s&link_type=abstract
(Akademiia Nauk SSSR, Izvestiia, Fizika Atmosfery i Okeana, vol. 13, Feb. 1977, p. 204-207.) Academy of Sciences, USSR, Izvestiy
Physics
Atmospheric and Oceanic Physics
Atmospheric Circulation, Atmospheric Models, Convective Heat Transfer, Planetary Atmospheres, Troposphere, Venus Atmosphere, Algorithms, Kinetic Energy, Solar Radiation, Time Dependence, Vertical Air Currents, Vertical Distribution, Wind Velocity
Scientific paper
Burangulov et al. (1974) have shown that a numerical model based on primitive equations and heat transport equations reproduces such basic experimentally observed characteristics of the Venusian atmosphere as small temperature constrasts at the day and night sides of the planet, the vertical nonuniformity of potential temperature, and the increase in wind velocity in the upper layers of the troposphere. In the present paper, the model is improved by introducing a more detailed radiation scheme developed with allowance for new experimental and theoretical data and an improved convection scheme, and by extending the number of computational levels to twenty.
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