Numerical simulation of the general circulation of the Cytherean lower atmosphere

Details Numerical simulation of the general circulation of the Cytherean lower atmosphere Numerical simulation of the general circulation of the Cytherean lower atmosphere

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icar...26..178c&link_type=abstract

Icarus, vol. 26, Oct. 1975, p. 178-208.

Astronomy and Astrophysics

Astronomy

3

Atmospheric Circulation, Atmospheric Models, Lower Atmosphere, Turbulent Heat Transfer, Venus Atmosphere, Astronomical Models, Finite Difference Theory, Greenhouse Effect, Planetary Rotation, Solar Heating

Scientific paper

A finite difference model is used to study the three-dimensional circulation of the Venus atmosphere. The model takes into account the effect of slow planetary rotation, which leads into an uneven planetary distribution of solar energy absorption, the effects of atmospheric mechanical and thermal inertia, and the opacity of the atmosphere to long-wave radiation which results in turbulent vertical heat transfer. The greenhouse effect is discussed in detail.

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