The flow of a two-component plasma model in a porous rotating hot sphere

Details The flow of a two-component plasma model in a porous rotating hot sphere The flow of a two-component plasma model in a porous rotating hot sphere

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.197...61a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 197, no. 1, p. 61-76.

Physics

High Temperature Plasmas, Magnetohydrodynamic Flow, Porous Materials, Rotating Spheres, Stellar Physics, Asymptotic Methods, Magnetohydrodynamic Stability, Reynolds Number, Temperature Distribution

Scientific paper

The paper studies the flow of a two-component hot plasma in a porous rotating sphere. Asymptotic solutions are derived for small rotation Reynolds number (Re). The overall analysis of the study shows that the temperature distribution of the gas inside the sphere has a minimum value for the various values of the radiation parameter N-squared at a point where the radius of the solar sphere is 0.5r solar. The general result of the studies are discussed quantitatively. The problem has a lot of application in the understanding of the interior of astrophysical bodies.

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