Thermosolutal-convective instability of a composite plasma in a stellar atmosphere including the effects of finite Larmour radius and Hall currents

DOI10.1007/BF02111194zbMath0741.76022OpenAlexW1965867440MaRDI QIDQ1183016

R. C. Sharma, K. C. Sharma, Urvashi Gupta

Publication date: 28 June 1992

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

Full work available at URL: https://doi.org/10.1007/bf02111194

zbMATH Keywords

Hall currentsuniform horizontal magnetic fieldThermosolutal-convective instabilityfinite Larmor radiuscomposite plasma

Mathematics Subject Classification ID

Multiphase and multicomponent flows (76T99) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

• On thermosolutal-convective instability in a stellar atmosphere. I. Effect of rotation and magnetic field
• Thermosolutal-convective instability of a composite plasma in a stellar atmosphere including the effects of variable magnetic field and rotation
• Magnetohydrodynamic Equations for Finite Larmor Radius

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