The magneto-gravitational instability of an infinite homogeneous, finitely conducting, viscous rotating plasma through porous medium is investignted in view of its relevance to certain stellar atmospheres. The dispersion relation has been obtained from the relevant linearized perturbntion equations
โฆ LIBER โฆ
Gravitational stability of finitely conducting two-component plasma through porous medium
โ Scribed by R. K. Chhajlani; D. S. Vaghela
- Publisher
- Springer Netherlands
- Year
- 1987
- Tongue
- English
- Weight
- 627 KB
- Volume
- 139
- Category
- Article
- ISSN
- 0004-640X
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The problem of stability of self gravitating magnetized plasma in porous medium is studied incorporating electrical resistivity, thermal conduction and FLR corrections. Normal mode analysis is applied to derive the dispersion relation. Wave propagation is discussed for parallel and perpendicular dir