Physics of compact stellarators

被引:28
作者
Hirshman, SP [1 ]
Spong, DA
Whitson, JC
Nelson, B
Batchelor, DB
Lyon, JF
Sanchez, R
Brooks, A
Fu, GY
Goldston, RJ
Ku, LP
Monticello, DA
Mynick, H
Neilson, GH
Pomphrey, N
Redi, M
Reiersen, W
Reiman, AH
Schmidt, J
White, R
Zarnstorff, MC
Miner, WH
Valanju, RM
Boozer, A
机构
[1] Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA
[2] Princeton Plasma Phys Lab, Princeton, NJ 08543 USA
[3] Univ Texas, Austin, TX 78712 USA
[4] Columbia Univ, Dept Appl Phys, New York, NY 10027 USA
关键词
D O I
10.1063/1.873489
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
Recent progress in the theoretical understanding and design of compact stellarators is described. Hybrid devices, which depart from canonical stellarators by deriving benefits from the bootstrap current which flows at finite beta, comprise a class of low aspect ratio A<4 stellarators. They possess external kink stability (at moderate beta) in the absence of a conducting wall, possible immunity to disruptions through external control of the transform and magnetic shear, and they achieve volume-averaged ballooning beta limits (4%-6%) similar to those in tokamaks. In addition, bootstrap currents can reduce the effects of magnetic islands (self-healing effect) and lead to simpler stellarator coils by reducing the required external transform. Powerful physics and coil optimization codes have been developed and integrated to design experiments aimed at exploring compact stellarators. The physics basis for designing the national compact stellarator will be discussed. [S1070-664X(99)95405-8].
引用
收藏
页码:1858 / 1864
页数:7
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