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Shear-flow stability within the atmosphere of Venus

Published online by Cambridge University Press:  29 March 2006

R. D. Cess  and
Harshvardhan
R. D. Cess
Affiliation:
Department of Mechanics, State University of New York, Stony Brook
Harshvardhan
Affiliation:
Department of Mechanics, State University of New York, Stony Brook
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Abstract

Employing a linear stability analysis, Dudis (1973) has recently suggested that shear-flow instability might exist within the upper stratosphere of Venus owing to destabilization by radiative transfer. We have incorporated a more realistic formulation for radiative transfer into his stability analysis and conclude that such an instability is unlikely.

Type
Research Article
Information
Journal of Fluid Mechanics , Volume 66 , Issue 2 , 6 November 1974 , pp. 267 - 272
Copyright
© 1974 Cambridge University Press

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References

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