Thermal instability in a two-component magnetized plasma

Details Thermal instability in a two-component magnetized plasma Thermal instability in a two-component magnetized plasma

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17.1031v&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, Nov. 1991, p. 1031-1038. In Russian.

Astronomy and Astrophysics

Astronomy

Energy Dissipation, Magnetohydrodynamic Stability, Plasma Dynamics, Solar Magnetic Field, Thermal Instability, Two Fluid Models, Magnetization, Maxwell Equation

Scientific paper

Attention is given to the origin of the discrepancies which arise in solving, either in the magnetohydrodynamic or two-fluid approximations, the problem of thermal instability in a radiating magnetized homogeneous plasma in the case of an arbitrary angle between the wave vector and the equilibrium magnetic field. In the former approximation the displacement current is disregarded, but this assumption is at variance with the system of two-fluid plasma equations. It is shown that, in the case of plasma motions approximately perpendicular to the magnetic field, the region of overstable perturbations may be wider than in the case of motions strictly perpendicular to the field.

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