Heat transfer by a meridional circulation cell and the static stability of the atmosphere on a slowly rotating planet

Details Heat transfer by a meridional circulation cell and the static stability of the atmosphere on a slowly rotating planet Heat transfer by a meridional circulation cell and the static stability of the atmosphere on a slowly rotating planet

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kosis..27..932z&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 27, Nov.-Dec. 1989, p. 932-942. In Russian.

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Atmospheric Circulation, Heat Transfer, Meridional Flow, Planetary Atmospheres, Planetary Rotation, Static Stability, Circulation Distribution, Parameterization, Temperature Distribution, Venus Atmosphere, Wind Velocity

Scientific paper

Equations are derived for determining the equator-pole temperature contrast and the static-stability parameter in a planetary atmosphere in which the main heat-transfer mechanism is ordered meridional circulation. The results obtained are used to estimate the atmosphere heat-adaptation periods, the wind-velocity scales, and other circulation characteristics on Venus.

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