On thermosolutal-convective instability in a stellar atmosphere. I - Effect of rotation and magnetic field

Details On thermosolutal-convective instability in a stellar atmosphere. I - Effect of rotation and magnetic field On thermosolutal-convective instability in a stellar atmosphere. I - Effect of rotation and magnetic field

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.126...21s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 126, no. 1, Oct. 1986, p. 21-28.

Astronomy and Astrophysics

Astrophysics

5

Convection, Stellar Atmospheres, Stellar Magnetic Fields, Stellar Rotation, Thermal Stability, Dispersion, Magnetic Effects, Perturbation Theory, Rotating Fluids

Scientific paper

Thermosolutal-convective instability of a stellar atmosphere is considered. The criteria for monotonic instability are derived. The effects of a variable horizontal magnetic field and the simultaneous presence of a uniform rotation and a uniform horizontal magnetic field have been considered on the thermosolutal-convective instability. The criteria derived for monotonic instability are found to hold good in the presence of a variable horizontal magnetic field as well as in the presence of a uniform rotation and a uniform horizontal magnetic field.

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