Thermosolutal-convective instability of a composite plasma in a stellar atmosphere including the effects of variable magnetic field and rotation

Computer Science – Numerical Analysis

Scientific paper

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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.

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