Internally heated convection in the atmosphere of Venus and in the laboratory

Details Internally heated convection in the atmosphere of Venus and in the laboratory Internally heated convection in the atmosphere of Venus and in the laboratory

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.257..110t&link_type=abstract

Nature, vol. 257, Sept. 11, 1975, p. 110-112.

Mathematics

5

Atmospheric Heating, Atmospheric Models, Convective Heat Transfer, Temperature Gradients, Venus Atmosphere, Vertical Distribution, Atmospheric Stratification, Benard Cells, Heat Generation, Internal Energy, Mathematical Models, Solar Radiation

Scientific paper

The possibility is considered that the cellular convection observed by Mariner 10 in the subsolar region of the atmosphere of Venus may be related to laboratory studies of convection with internal heat generation. It appears probably that the basic dynamics of the Venusian convection and of the convection observed in the laboratory experiments are similar. The Venusian cells have highly structured interiors. In the laboratory, cells with an elongation of greater than about two develop an internal structure.

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