Steady-state axisymmetric configurations of a weakly ionized plasma in the field of a rotating magnetized spherical body

被引:7
|
作者
Soldatkin, AO [1 ]
Chugunov, YV [1 ]
机构
[1] Russian Acad Sci, Inst Appl Phys, Nizhnii Novgorod 603950, Russia
关键词
Magnetic Field; Anisotropy; Density Distribution; Plasma Density; Angular Frequency;
D O I
10.1134/1.1538503
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Self-consistent steady-state axisymmetric configurations of a plasma envelope with a uniform anisotropic conductivity around a rotating magnetized spherical body are considered. A set of electrodynamic and magnetohydrodynamic equations is analyzed under the assumption that the mass velocity of a moving weakly ionized plasma has only the azimuthal component. The equations describing the profile of the angular frequency of the rotating plasma envelope, the magnetic field, the conduction currents, and the plasma density distribution are solved in the limit of a strong anisotropy of the conductivity of a weakly ionized gas. The applicability of the results obtained to a qualitative interpretation of the phenomena occurring in the plasmaspheres of magnetized planets is discussed. (C) 2003 MAIK "Nauka/Interperiodica".
引用
收藏
页码:65 / 77
页数:13
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