Larmor radius effects on the instability of a rotating layer of a self- gravitating plasma

DOI10.1007/BF00653810zbMath0581.76059OpenAlexW2069321155MaRDI QIDQ1067908

P. K. Bhatia, R. P. S. Chhonkar

Publication date: 1985

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

Full work available at URL: https://doi.org/10.1007/bf00653810

zbMATH Keywords

stability analysisdispersion relationsvariational methodsHall currentCoriolis forcesuniform horizontal magnetic fieldfinite Larmor radiusrotating, viscous, finitely conducting, self-gravitating, incompressible plasmastratified layertransverse mode of wave propagation

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (7)

Magnetic resistivity and Hall currents effects on the stability of a self-gravitating plasma of varying density in variable magnetic field ⋮ Gravitational stability of finitely conducting two-component plasma through porous medium ⋮ Magnetogravitational stability of self-gravitating plasma with thermal conduction and finite Larmor radius through porous medium ⋮ Effects of Hall currents and Coriolis forces on the instability of a self-gravitating plasma of variable density ⋮ Stability of thermally conducting plasma in a variable magnetic field ⋮ Instability of a gravitating partially-ionized plasma ⋮ Gravitational instability of partially-ionized plasma in an oblique magnetic field

Cites Work

• Effects of gyroviscosity and Hall currents on the stability of a stratified rotating self-gravitating plasma
• Magnetohydrodynamic Equations for Finite Larmor Radius

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