Thermal-convective instability of a composite plasma in a stellar atmosphere with rotation and magnetic field

Details Thermal-convective instability of a composite plasma in a stellar atmosphere with rotation and magnetic field Thermal-convective instability of a composite plasma in a stellar atmosphere with rotation and magnetic field

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.137..297s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 137, no. 2, Oct. 1987, p. 297-302.

Astronomy and Astrophysics

Astrophysics

1

Free Convection, Magnetohydrodynamic Stability, Stellar Atmospheres, Stellar Magnetic Fields, Stellar Oscillations, Stellar Rotation, Convective Heat Transfer, Stellar Models, Thermodynamics

Scientific paper

The thermal-convective instability of a composite plasma in a stellar atmosphere is studied, taking into account the effects of a uniform rotation and a uniform magnetic field. The case in which both the boundaries are free and the medium adjoining the fluid is nonconducting is considered. The criterion for monotonic instability is found to be the same in the presence or absence of a uniform rotation and a uniform magnetic field.

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