Nonlinear symmetric stability of planetary atmospheres.

Details Nonlinear symmetric stability of planetary atmospheres. Nonlinear symmetric stability of planetary atmospheres.

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995jfm...296..391b&link_type=abstract

Journal of Fluid Mechanics, Vol. 296, p. 391 - 407

Computer Science

4

Planetary Atmospheres: Stability

Scientific paper

The energy-Casimir method is applied to the problem of symmetric stability in the context of a compressible, hydrostatic planetary atmosphere with a general equation of state. Formal stability criteria for symmetric disturbances to a zonally symmetric baroclinic flow are obtained. In the special case of a perfect gas the results of Stevens (1983) are recovered. Finite-amplitude stability conditions are also obtained that provide an upper bound on a certain positive-definite measure of disturbance amplitude.

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