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

On thermosolutal-convective instability in a stellar atmosphere. I. Effect of rotation and magnetic field (Q1084994)

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scientific article; zbMATH DE number 3980755
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English
On thermosolutal-convective instability in a stellar atmosphere. I. Effect of rotation and magnetic field
scientific article; zbMATH DE number 3980755

    Statements

    On thermosolutal-convective instability in a stellar atmosphere. I. Effect of rotation and magnetic field (English)
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    1986
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    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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    Schwarzschild criterion
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    Thermosolutal-convective instability
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    stellar atmosphere
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    monotonic instability
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    variable horizontal magnetic field
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    uniform rotation
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    uniform horizontal magnetic field
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