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• W2597765910 abstract "A method for computing the ideal magnetohydrodynamic (MHD) stability boundaries in three-dimensional equilibria is employed. Following Hegna and Nakajima [Phys. Plasmas 5, 1336 (1998)], a two-dimensional family of equilibria is constructed by perturbing the pressure and rotational-transform profiles in the vicinity of a flux surface for a given stellarator equilibrium. The perturbations are constrained to preserve the MHD equilibrium condition. For each perturbed equilibrium, the infinite-n ballooning stability is calculated. Marginal stability diagrams are thus constructed that are analogous to (s,α) diagrams for axisymmetric configurations. A quasiaxisymmetric stellarator is considered. Calculations of stability boundaries generally show regions of instability can occur for either sign of the average magnetic shear. Additionally, regions of second-stability are present." @default.
• W2597765910 created "2017-04-07" @default.
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• W2597765910 date "2003-12-01" @default.
• W2597765910 modified "2023-09-26" @default.
• W2597765910 title "Marginal stability boundaries for infinite-<i>n</i>ballooning modes in a quasiaxisymmetric stellarator" @default.
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• W2597765910 doi "https://doi.org/10.1063/1.1622669" @default.
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