On the thermal instability of a nonuniformly rotating fluid layer heated from below

Details On the thermal instability of a nonuniformly rotating fluid layer heated from below On the thermal instability of a nonuniformly rotating fluid layer heated from below

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001soph..202....1e&link_type=abstract

Solar Physics, v. 202, Issue 1, p. 1-9 (2001).

Physics

Scientific paper

The thermal instability both as stationary convection and overstability of a nonuniformly rotating fluid layer of vertical extent is considered. It is shown that in both types of instability the effect of the variation of the rate of rotation is to introduce a new branch to the marginal instability curves of uniform rotation which departs from them towards a zero of the Rayleigh number as the horizontal wavenumber approaches zero. The relevance to the solar interior is discussed.

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