Thermosolutal-convective instability in a stellar atmosphere

Details Thermosolutal-convective instability in a stellar atmosphere Thermosolutal-convective instability in a stellar atmosphere

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987japa....8..305s&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 8, Dec. 1987, p. 305-314.

Physics

1

Atmospheric Physics, Convective Heat Transfer, Stellar Atmospheres, Perturbation Theory, Radiative Transfer, Stellar Magnetic Fields, Stellar Rotation

Scientific paper

The thermosolutal-convective instability of a stellar atmosphere is studied in the presence of suspended particles. The criteria for monotonic instability are derived and are found to hold good also in the presence of uniform rotation and uniform magnetic field on the thermosolutal-convective instability. The thermosolutal-convective instability of a stellar atmosphere is also studied in the presence of suspended particles and radiative transfer effects and the criteria for monotonic instability are obtained in terms of source function.

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