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(TH3/2) Recent Progress in MHD Stability Calculations of Compact Stellarators

G. Y. Fu¹⁾, L. P. Ku¹⁾, M. H. Redi¹⁾, C. Kessel¹⁾, D. Monticello¹⁾, A. Reiman¹⁾, W. A. Cooper²⁾, C. Nührenberg³⁾, R. Sanchez⁴⁾, A. Ware⁵⁾, S. Hirshman⁶⁾, D. A. Spong^6)
 
1) Princeton Plasma Physics Laboratory, Princeton, NJ 08543, U.S.A.
²⁾ Center of Research for Plasma Physics, EPFL, Lausanne, Switzerland
³⁾ Max-Planck-Institute for Plasma Physics, Greifswald, Germany
⁴⁾ Universidad Carlos III de Madrid, Madrid, Spain
⁵⁾ University of Montana, Missoula, MT 59812, U.S.A.
⁶⁾ Oak Ridge National Laboratory, Oak Ridge, TN 37831, U.S.A.

Abstract.  A key issue for compact stellarators is the stability of beta-limiting MHD modes, such as external kink modes driven by bootstrap current and pressure gradient. We report here recent progress in MHD stability studies for low-aspect-ratio Quasi-Axisymmetric Stellarators (QAS) and Quasi-Omnigeneous Stellarators (QOS). We find that the N = 0 periodicity-preserving vertical mode is significantly more stable in stellarators than in tokamaks because of the externally generated rotational transform. It is shown that both low-n external kink modes and high-n ballooning modes can be stabilized at high beta by appropriate 3D shaping without a conducting wall. The stabilization mechanism for external kink modes in QAS appears to be an enhancement of local magnetic shear due to 3D shaping. The stabilization of ballooning mode in QOS is related to a shortening of the normal curvature connection length.

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