Ideal magnetohydrodynamic stability of the NCSX

被引:11
作者
Fu, G. Y.
Isaev, M.
Ku, L. P.
Mikhailov, M.
Redi, M. H.
Sanchez, R.
Subbotin, A.
Cooper, W. A.
Hirshman, S. P.
Monticello, D. A.
Reiman, A.
Zarnstorff, M.
机构
[1] Princeton Plasma Phys Lab, Princeton, NJ 08543 USA
[2] IV Kurchatov Atom Energy Inst, Moscow 123182, Russia
[3] Univ Carlos III Madrid, Madrid, Spain
[4] EURATOM, EPFL, CRPP, Lausanne, Switzerland
[5] Oak Ridge Natl Lab, Oak Ridge, TN USA
关键词
ideal magnetohydrodynamic stability; stellarators; quasi-axisymmetric stellarators;
D O I
10.13182/FST07-A1300
中图分类号
TL [原子能技术]; O571 [原子核物理学];
学科分类号
0827 ; 082701 ;
摘要
The ideal magnetohydrodynamic (MHD) stability of the National Compact Stellarator Experiment (NCSX) is extensively analyzed using the most advanced three-dimensional MHD codes. It is shown that the NCSX is stable to finite-n MHD modes, including the vertical mode, external kink modes and ballooning modes. However, high-n external kink modes that peak near the plasma edge are found to be weakly unstable. A global calculation shows that finite-n ballooning modes are significantly more stable than the local infinite-n modes.
引用
收藏
页码:218 / 231
页数:14
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