Magnetogravitational instability of an infinite homogeneous rotating plasma through a porous medium with finite electrical and thermal conductivities

DOI10.1007/BF00643533zbMath0674.76030OpenAlexW1963797507MaRDI QIDQ1121723

R. K. Chhajlani, M. K. Vyas

Publication date: 1988

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

Full work available at URL: https://doi.org/10.1007/bf00643533

zbMATH Keywords

porous mediumuniform magnetic fieldthermal conductivitiesgravitational instability of an infinite homogeneous rotating plasmaJeans's condition of instability

Mathematics Subject Classification ID

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

Related Items (4)

Gravitational instability of a thermally-conducting plasma flowing through a porous medium in the presence of suspended particles ⋮ The gravitational instability of a non-uniformly rotating heat conducting medium in the presence of non-uniform magnetic field ⋮ Self-gravitational instability of rotating viscous Hall plasma with arbitrary radiative heat-loss functions and electron inertia ⋮ Effect of rotation and FLR corrections with radiative heat-loss functions on transverse thermal instability of astrophysical porous plasma in interstellar medium (ISM)

Cites Work

• The gravitational instability of flow through porous medium for some systems of astrophysical interest
• Finite Larmor radius and Hall current effects on magneto-gravitational instability of a plasma in the presence of suspended particles

This page was built for publication: Magnetogravitational instability of an infinite homogeneous rotating plasma through a porous medium with finite electrical and thermal conductivities