Hydromagnetic stability of a rotating baroclinic star

The magnetohydrodynamic stability of a rotating baroclinic star has been studied in the presence of poloidal and toroidal magnetic fields taking into account the diffusive effects. Necessary conditions for stability have been found by normal mode analysis under small wavelength approximation.

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Bibliographische Detailangaben
Veröffentlicht in:	Astrophysics and space science 1984-03, Vol.100 (1-2), p.85-93
1. Verfasser:	RAGHAVACHAR, M. R
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology Star formation Stars Stellar characteristics and properties
Online-Zugang:	Volltext
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Beschreibung
Zusammenfassung:	The magnetohydrodynamic stability of a rotating baroclinic star has been studied in the presence of poloidal and toroidal magnetic fields taking into account the diffusive effects. Necessary conditions for stability have been found by normal mode analysis under small wavelength approximation.
ISSN:	0004-640X 1572-946X
DOI:	10.1007/BF00651587