MAGNETOHYDRODYNAMIC MODELING FOR FUSION PLASMAS

被引:1
作者
Keppens, R. [1 ,2 ,3 ]
Goedbloed, J. P. [1 ,3 ]
Blokland, J. W. S. [1 ]
机构
[1] Katholieke Univ Leuven, FOM Inst Plasma Phys Rijnhuizen, Louvain, Belgium
[2] Katholieke Univ Leuven, Ctr Plasma Astrophys, Louvain, Belgium
[3] Univ Utrecht, Astron Inst, NL-3508 TC Utrecht, Netherlands
关键词
ASTROPHYSICAL PLASMAS; MHD; EQUILIBRIA; SIMULATION; STABILITY;
D O I
10.13182/FST10-A9404
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 magnetohydrodynamic model for fusion plasma dynamics governs the large-scale equilibrium properties, and sets the most stringent constraints on the parameter space accessible without violent disruptions. In conjunction with linear stability analysis in the complex tokamak geometry, the MHD paradigm is also routinely being used to diagnose recurring wave modes and identify potential MHD mode triggers of consequent non-MHD phenomena. On the other hand, it is currently computationally feasible to perform fully nonlinear simulations in tokamak geometry, and determine nonlinear, long-term (i.e. on resistive time scales) evolutions for individual MHD dominated plasma scenarios. It can be expected that this success continues its evolution towards a fully integrated computational analysis of the experimental campaigns, certainly in view of the desired steady-state self-burning plasmas.
引用
收藏
页码:137 / 147
页数:11
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