Shear-flow stability within the atmosphere of Venus

Details Shear-flow stability within the atmosphere of Venus Shear-flow stability within the atmosphere of Venus

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974jfm....66..267c&link_type=abstract

Journal of Fluid Mechanics, vol. 66, Nov. 6, 1974, p. 267-272.

Physics

Flow Stability, Radiative Transfer, Shear Flow, Stratosphere, Venus Atmosphere, Atmospheric Stratification, Destabilization, Gray Gas, Richardson Number, Shear Layers, Thermal Radiation

Scientific paper

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.

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