Resistive wall mode stabilization in toroidal geometry

被引:24
作者
Bondeson, A [1 ]
Gimblett, CG
Hastie, RJ
机构
[1] Chalmers Univ Technol, Dept Electromagnet, Euratom NFR Fus Assoc, S-41296 Gothenburg, Sweden
[2] EURATOM, Culham Sci Ctr, Abingdon OX14 3DB, Oxon, England
关键词
D O I
10.1063/1.873346
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 possibility of stabilizing ideal magnetohydrodynamical (MHD) instabilities by resistive walls and slow plasma rotation (rotation frequencies comparable to resistive tearing growth rates) was proposed recently by Finn [Phys. Plasmas 2, 3782 (1995)] on the basis of cylindrical theory. In the present paper we analyze toroidal effects (pressure gradients and favorable averaged curvature) [Glasser et al., Phys. Fluids 18, 875 (1975)] on this "resistive window.'' It is found that in toroidal geometry the resistive window for the distance of the wall from the plasma scales as S-1/ 3 (S is the ratio of resistive to Alfvenic time scales) and thus becomes very small in large tokamaks. Other differences between toroidal and cylindrical theories of resistive wall mode stability are discussed. (C) 1999 American Institute of Physics. [S1070-664X(99)00203-7].
引用
收藏
页码:637 / 640
页数:4
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