Thermal-convective instability of a composite rotating stellar atmosphere in the presence of a variable magnetic field, medium permeability and solute gradient

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Stellar Atmospheres, Stellar Convection, Stellar Magnetic Fields, Stellar Rotation, Thermal Stability, Magnetic Field Configurations, Permeability, Perturbation Theory, Porosity

Scientific paper

The thermal-convective instability of a composite rotating stellar atmosphere in a variable horizontal magnetic field is described taking into account the effects of medium permeability and solute gradient. The criteria for monotonic instability in each case is determined which generalize the Defouw (1970) criterion derived for the thermal-convective instability in the absence of the effects under consideration.

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