Hydromagnetic stability of a rotating baroclinic star

DOI10.1007/BF00651587zbMath0545.76057OpenAlexW2077461655MaRDI QIDQ798191

M. R. Raghavachar

Publication date: 1984

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00651587

zbMATH Keywords

conditions for stabilitydiffusive effectspoloidal and toroidal magnetic fieldsrotating baroclinic starsmall wavelength approximation

Mathematics Subject Classification ID

Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25)

Cites Work

• Do eddington–sweet circulations exist?

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