Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.149..323v&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 149, no. 2, Nov. 1988, p. 323-342.
Astronomy and Astrophysics
Astrophysics
3
Gravitational Effects, Magnetohydrodynamic Stability, Plasma Conductivity, Plasma Waves, Porosity, Rotating Plasmas, Larmor Radius, Star Formation, Thermal Conductivity, Wave Propagation
Scientific paper
The magnetogravitational instability of a thermally-conducting rotating plasma flowing through a porous medium with finite conductivity and finite Larmor radius (FLR) in the presence of suspended particles is studied. The modified Jeans criterion determines the instability condition. It is found that the effects of rotation and FLR are decreased by the porosity and the suspended particles, and that finite conductivity removes the Alfven velocity from the Jeans condition.
Chhajlani R. K.
Vyas M. K.
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