000120204 001__ 120204
000120204 005__ 20181203021216.0
000120204 020__ $$a0029-5515
000120204 0247_ $$2doi$$a10.1088/0029-5515/45/9/013
000120204 022__ $$a0029-5515
000120204 02470 $$2DAR$$a7446
000120204 02470 $$2ISI$$a000232350100013
000120204 037__ $$aARTICLE
000120204 245__ $$aFeedback and rotational stabilization of resistive wall modes in ITER
000120204 260__ $$c2005
000120204 269__ $$a2005
000120204 336__ $$aJournal Articles
000120204 520__ $$aDifferent 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.
000120204 6531_ $$aITER
000120204 6531_ $$aJET
000120204 700__ $$aLiu, Y. Q.
000120204 700__ $$aBondeson, A.
000120204 700__ $$aChu, M. S.
000120204 700__ $$0241656$$aFavez, J. Y.$$g108759
000120204 700__ $$aGribov, Y.
000120204 700__ $$aGryaznevich, M.
000120204 700__ $$aHender, T. C.
000120204 700__ $$aHowell, D. R.
000120204 700__ $$aLa Haye, R. J.
000120204 700__ $$0240108$$aLister, J. B.$$g105676
000120204 700__ $$ade Vries, P.
000120204 773__ $$j45$$k9$$q1131-1139$$tNuclear Fusion
000120204 909C0 $$pCRPP
000120204 909C0 $$0252028$$pSPC
000120204 909CO $$ooai:infoscience.tind.io:120204$$pSB$$particle
000120204 937__ $$aCRPP-ARTICLE-2005-046
000120204 973__ $$aEPFL$$rREVIEWED$$sPUBLISHED
000120204 980__ $$aARTICLE