Generation of the kinetic energy of atmospheric circulation on slowly rotating planets

Details Generation of the kinetic energy of atmospheric circulation on slowly rotating planets Generation of the kinetic energy of atmospheric circulation on slowly rotating planets

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976dossr.227.1315b&link_type=abstract

Akademiia Nauk SSSR, Doklady, vol. 227, Apr. 21, 1976, p. 1315-1318. In Russian.

Physics

2

Atmospheric Circulation, Kinetic Energy, Planetary Atmospheres, Atmospheric Models, Atmospheric Turbulence, Energy Dissipation, Planetary Rotation, Venus Atmosphere

Scientific paper

An expression is presented for the generation of kinetic energy of atmospheric circulation on a slowly rotating planet in the case when the Coriolis effect can be ignored, i.e., direction of the main flow and the pressure gradient coincide. Formulas are presented for energy generation efficiency and for turbulent energy dissipation. A numerical circulation model of the Venus atmosphere is examined.

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