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
Magnetogravitational Instability of a Thermally Conducting Rotating Plasma through a Porous Medium
โ Scribed by R. K. Chhajlani; M. K. Vyas
- Publisher
- John Wiley and Sons
- Year
- 1989
- Tongue
- English
- Weight
- 738 KB
- Volume
- 29
- Category
- Article
- ISSN
- 0005-8025
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