Dust-induced instability in a rotating plasma

被引:11
作者
Mikhailovskii, A. B. [1 ]
Vladimirov, S. V. [2 ]
Lominadze, J. G. [3 ]
Tsypin, V. S. [4 ]
Churikov, A. P. [5 ]
Erokhin, N. N. [1 ]
Galvao, R. M. O. [4 ,6 ]
机构
[1] Russian Res Ctr, Kurchatov Inst, Inst Nucl Fus, Moscow 123182, Russia
[2] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia
[3] Kharadze Abastumani Natl Astrophys Observ, GE-0160 Tbilisi, Georgia
[4] Brazilian Ctr Phys Res, BR-22290180 Rio De Janeiro, Brazil
[5] Samara Tech Univ, Syzran Branch, Syzran 446001, Samara Region, Russia
[6] Univ Sao Paulo, Inst Phys, BR-05508900 Sao Paulo, Brazil
基金
巴西圣保罗研究基金会; 俄罗斯基础研究基金会; 澳大利亚研究理事会;
关键词
D O I
10.1063/1.2813188
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
The effect of immobile dust on stability of a magnetized rotating plasma is analyzed. In the presence of dust, a term containing an electric field appears in the one-fluid equation of plasma motion. This electric field leads to an instability of the magnetized rotating plasma called the dust-induced rotational instability (DRI). The DRI is related to the charge imbalance between plasma ions and electrons introduced by the presence of charged dust. In contrast to the well-known magnetorotational instability requiring the decreasing radial profile of the plasma rotation frequency, the DRI can appear for an increasing rotation frequency profile. (c) 2008 American Institute of Physics.
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页数:3
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