Hydromagnetic stability of a rotating baroclinic star

Details Hydromagnetic stability of a rotating baroclinic star Hydromagnetic stability of a rotating baroclinic star

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.100...85r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 100, no. 1-2, March 1984, p. 85-93.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Baroclinic Instability, Magnetohydrodynamic Stability, Stellar Rotation, Magnetic Field Configurations, Partial Differential Equations, Perturbation Theory, Stellar Magnetic Fields

Scientific paper

The magnetohydrodynamic stability of 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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