Statistics – Computation
Scientific paper
May 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.112..391s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 112, no. 2, May 1985, p. 391-395.
Statistics
Computation
2
Computational Astrophysics, Hall Effect, Magnetohydrodynamic Stability, Space Plasmas, Thermal Instability, Collisions, Plasma Heating
Scientific paper
Thermal instability of a finitely conducting hydromagnetic composite medium is considered including the effects of Hall currents and the collisions with neutrals. The equilibrium magnetic field is assumed to be uniform and vertical. For stationary convection, the collisions have no effect, while the Hall currents are found to have a destabilizing effect on thermal instability. It is further shown that when M is finite and Q tends to infinity, the asymptotic behaviors of the critical Rayleigh number, the critical wave number, and the critical temperature gradient remain the same as those obtained Chandrasekhar (1961), where M is a nondimensional number which includes the Hall current effects and Q stands for the Chandrasekhar number.
Sharma K. C.
Sharma Sanjeev
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