Magnetorotational instability in a two-fluid model

被引:13
作者
Ren, Haijun [1 ,2 ]
Cao, Jintao [2 ]
Wu, Zhengwei [1 ,2 ]
Chu, Paul K. [1 ]
机构
[1] City Univ Hong Kong, Dept Phys & Mat Sci, Kowloon, Hong Kong, Peoples R China
[2] Univ Sci & Technol China, CAS Key Lab Basic Plasma Phys, Hefei 230026, Peoples R China
基金
中国国家自然科学基金; 中国博士后科学基金;
关键词
WEAKLY MAGNETIZED DISKS; LOCAL SHEAR INSTABILITY; KELVIN-HELMHOLTZ INSTABILITY; ACCRETION DISKS; PROTOPLANETARY DISKS; LINEAR-ANALYSIS; STABILITY; TURBULENCE; TRANSPORT; PLASMA;
D O I
10.1088/0741-3335/53/6/065021
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 magnetorotational instability (MRI) is investigated using a two-fluid model. Electrons and singly charged ions are supposed to have the same angular velocity to eliminate the equilibrium current. The linear dispersion relation governing local MRI is derived. The instability criteria in the non-magnetized and weakly magnetized cases differ remarkably from those predicted by the one-fluid model. Based on the general magnetized case, we present the critical conditions for the occurrence of instability. Gyroeffects significantly alter the instability criterion and introduce four unstable regions, one of which is reduced to the magnetohydrodynamic result when the angular frequency is much less than the ion gyrofrequency. When the angular frequency is much less than the electron gyrofrequency, the ion gyroeffect contributes to the instability criterion and induces the Hall term.
引用
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页数:14
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