Thermosolutal-convective instability of a stellar atmosphere in the presence of suspended particles

Details Thermosolutal-convective instability of a stellar atmosphere in the presence of suspended particles Thermosolutal-convective instability of a stellar atmosphere in the presence of suspended particles

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.183..183s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 183, no. 2, Sept. 1991, p. 183-191.

Astronomy and Astrophysics

Astrophysics

1

Convection, Flow Stability, Magnetic Effects, Perturbation Theory, Stellar Atmospheres, Thermal Stability, Coriolis Effect, Equations Of Motion, Gas Dynamics, Maxwell Equation, Suspending (Mixing)

Scientific paper

Thermosolutal-convective instability of a stellar atmosphere is considered in the presence of suspended particles. The criteria for monotonic instability are derived which are found to hold good in the presence of uniform rotation and uniform magnetic field, separately, on the thermosolutal-convective instability in the presence of suspended particles.

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