Liu, Y. Q.Bondeson, A.Chu, M. S.Favez, J. Y.Gribov, Y.Gryaznevich, M.Hender, T. C.Howell, D. R.La Haye, R. J.Lister, J. B.de Vries, P.2008-04-162008-04-162008-04-16200510.1088/0029-5515/45/9/013https://infoscience.epfl.ch/handle/20.500.14299/22171WOS:0002323501000137446Different 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.ITERJETtext::journal::journal article::research article