Chapter 3: MHD stability, operational limits and disruptions

Hender, T. C.; Wesley, J. C.; Bialek, J.; Bondeson, A.; Boozer, A. H.; Buttery, R. J.; Garofalo, A.; Goodman, T. P.; Granetz, R. S.; Gribov, Y.; Gruber, O.; Gryaznevich, M.; Giruzzi, G.; Günter, S.; Hayashi, N.; Helander, P.; Hegna, C. C.; Howell, D. F.; Humphreys, D. A.; Huysmans, G. T. A.; Hyatt, A. W.; Isayama, A.; Jardin, S. C.; Kawano, Y.; Kellman, A.; Kessel, C.; Koslowski, H. R.; La Haye, R. J.; Lazzaro, E.; Liu, Y. Q.; Lukash, V.; Manickam, J.; Medvedev, S.; Mertens, V.; Mirnov, S. V.; Nakamura, Y.; Navratil, G.; Okabayashi, M.; Ozeki, T.; Paccagnella, R.; Pautasso, G.; Porcelli, F.; Pustovitov, V. D.; Riccardo, V.; Sato, M.; Sauter, O.; Schaffer, M. J.; Shimada, M.; Sonato, P.; Strait, E. J.; Sugihara, M.; Takechi, M.; Turnbull, A. D.; Westerhof, E.; Whyte, D. G.; Yoshino, R.; Zohm, H.; ITPA MHD, Disruption and Magnetic Control Topical Group

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Chapter 3: MHD stability, operational limits and disruptions

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Gruber, O.
Tokamak Scenario Development (E1), Max Planck Institute for Plasma Physics, Max Planck Society;

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Günter, S.
Tokamak Theory (TOK), Max Planck Institute for Plasma Physics, Max Planck Society;

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Helander, P.
Stellarator Theory (ST), Max Planck Institute for Plasma Physics, Max Planck Society;

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Mertens, V.
Tokamak Scenario Development (E1), Max Planck Institute for Plasma Physics, Max Planck Society;

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Pautasso, G.
Tokamak Theory (TOK), Max Planck Institute for Plasma Physics, Max Planck Society;

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Sugihara, M.
Experimental Plasma Physics 2 (E2), Max Planck Institute for Plasma Physics, Max Planck Society;

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Zohm, H.
Tokamak Scenario Development (E1), Max Planck Institute for Plasma Physics, Max Planck Society;

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Hender, T. C., Wesley, J. C., Bialek, J., Bondeson, A., Boozer, A. H., Buttery, R. J., et al. (2007). Chapter 3: MHD stability, operational limits and disruptions. Progress in the ITER Physics Basis, S128-S202. Retrieved from http://dx.doi.org/10.1088/0029-5515/47/6/S03.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0027-06D8-E

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