Computer Science – Numerical Analysis
Scientific paper
Oct 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.184..261s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 184, no. 2, Oct. 1991, p. 261-271.
Computer Science
Numerical Analysis
1
Rotating Fluids, Stellar Atmospheres, Stellar Magnetic Fields, Thermal Stability, Convection, Numerical Analysis, Perturbation Theory, Solutes
Scientific paper
Thermosolutal-convective instability of a composite plasma in a stellar atmosphere is considered. The effect of a variable horizontal magnetic field and the simultaneous effect of a uniform rotation and a variable horizontal magnetic field have been considered on the thermosolutal-convective instability. Sufficient conditions for the existence of monotonic instability were derived. It is found that the criteria for monotonic instability hold good in the presence of a variable horizontal magnetic field as well as in the presence of a uniform rotation and a variable horizontal magnetic field.
Gupta Urvashi
Sharma K. C.
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