Gravitational stability of finitely conducting two-component plasma through porous medium

DOI10.1007/BF00644363zbMath0644.76055OpenAlexW2094095292MaRDI QIDQ1102801

D. S. Vaghela, R. K. Chhajlani

Publication date: 1987

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

Full work available at URL: https://doi.org/10.1007/bf00644363

zbMATH Keywords

porous mediumnormal mode analysisgravitational stabilityHurwitz criterionDispersion relationsmagnetized self-gravitating two-component plasma of finite conductivity flowing

Mathematics Subject Classification ID

Flows in porous media; filtration; seepage (76S05) Multiphase and multicomponent flows (76T99) Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (1)

The flow of a two-component plasma model in a porous rotating hot sphere

Cites Work

• The gravitational instability of flow through porous medium for some systems of astrophysical interest
• Larmor radius effects on the instability of a rotating layer of a self- gravitating plasma
• Magnetogravitational stability of self-gravitating plasma with thermal conduction and finite Larmor radius through porous medium

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