Magnetorotational instability in a rotating liquid metal annulus

被引:133
|
作者
Ji, HT
Goodman, J
Kageyama, A
机构
[1] Princeton Plasma Phys Lab, Princeton, NJ 08543 USA
[2] Princeton Univ Observ, Princeton, NJ 08544 USA
[3] Natl Inst Fus Sci, Gifu 5095292, Japan
关键词
accretion; accretion discs; instabilities; magnetic fields; MHD; planetary systems : protoplanetary discs; Galaxy : disc;
D O I
10.1046/j.1365-8711.2001.04647.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Although the magnetorotational instability (MRI) has been widely accepted as a powerful accretion mechanism in magnetized accretion discs, it has not been realized in, the laboratory. The possibility of studying MRI in a rotating liquid metal annulus (Couette flow) is explored by local and global stability analysis. Stability diagrams are drawn in dimensionless parameters, and also in terms of the-angular velocities at the inner and outer cylinders. It is shown that MRI can be triggered in a moderately rapidly rotating table-top apparatus, using easy-to-handle metals such as gallium. Practical issues of this proposed experiment are discussed.
引用
收藏
页码:L1 / L5
页数:5
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