Thermal-convective instability of a rotating plasma in stellar atmospheres with Hall effect

DOI10.1007/BF00645991zbMATH Open0661.76036OpenAlexW1974927149MaRDI QIDQ1113751

K. C. Sharma, Deshbir Singh Pathania

Publication date: 1989

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

Full work available at URL: https://doi.org/10.1007/bf00645991

zbMATH Keywords

Hall currentsstellar atmosphereThermal-convective instabilityhydromagnetic, composite, rotating, inviscid, and infinitely conducting plasma

Mathematics Subject Classification ID

Absolute and convective instability and stability in hydrodynamic stability (76E15) General theory of rotating fluids (76U05) Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Ionized gas flow in electromagnetic fields; plasmic flow (76X05) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

• Title not available (Why is that?)
• Thermal-convective instability of a composite plasma in a stellar atmosphere with rotation and magnetic field

Related Items (3)

On thermosolutal-convective instability in a stellar atmosphere. I. Effect of rotation and magnetic field ⋮ Thermosolutal-convective instability of a composite stellar atmosphere in the presence of a variable magnetic field ⋮ ROLE OF THE HALL EFFECT ON THE MAGNETOROTATIONAL INSTABILITY

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