Feedback and rotational stabilization of resistive wall modes in ITER

被引:63
作者
Liu, YQ [1 ]
Bondeson, A
Chu, MS
Favez, JY
Gribov, Y
Gryaznevich, M
Hender, TC
Howell, DR
La Haye, RJ
Lister, JB
de Vries, P
机构
[1] Chalmers Univ Technol, EURATOM, Dept Appl Mech, VR Fus Assoc, S-41296 Gothenburg, Sweden
[2] Gen Atom Co, San Diego, CA USA
[3] Ecole Polytech Fed Lausanne, Assoc Euratom Confederat Suisse, CRPP, CH-1015 Lausanne, Switzerland
[4] ITER Naka Joint Work Site, Phys Unit, Naka, Ibaraki, Japan
[5] UKAEA Euratom Fus Assoc, Culham Sci Ctr, Abingdon OX14 3DB, Oxon, England
关键词
D O I
10.1088/0029-5515/45/9/013
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
Different models have been introduced in the stability code MARS-F in order to study the damping effect on resistive wall modes (RWM) in rotating plasmas. Benchmarks of MARS-F calculations with RWM experiments on JET and DIII-D indicate that the semi-kinetic damping model is a good candidate for explaining the damping mechanisms. Based on these results, the critical rotation speeds required for RWM stabilization in advanced ITER scenarios are predicted. Active feedback control of the n = 1 RWM in ITER is also studied using the MARS-F code.
引用
收藏
页码:1131 / 1139
页数:9
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