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Stability of a one-dimensional plasma in slab geometry

Journal Article · · Phys. Fluids; (United States)
DOI:https://doi.org/10.1063/1.866431· OSTI ID:5998096
Stability of a one-dimensional slab of plasma is considered for the simplest case of a static equilibrium with negligible pressure. A special class of deformations is considered that satisfies a magnetohydrodynamic (MHD) constraint except in a particular surface. These deformations, which resemble those considered for tearing modes, form a continuous path away from the equilibrium. The deformed configurations are not equilibria and their magnetic energies are, therefore, always larger than those of associated equilibria. It is shown that except for a special class of equilibria (previously discussed by Taylor, Phys. Rev. Lett. 33, 1139 (1974)) there exist deformations for which the magnetic energy is continuously decreasing, a result that is interpreted as showing that only this class is stable. The arguments, though asymptotic, are simple, essentially geometric, and do not require linearization. The results differ from those of the traditional linear tearing mode calculation (Furth, Killeen, and Rosenbluth, Phys. Fluids 6, 459 (1963)), making the class of stable equilibria smaller.
Research Organization:
GA Technologies Inc., P. O. Box 85608, San Diego, California 92138
OSTI ID:
5998096
Journal Information:
Phys. Fluids; (United States), Journal Name: Phys. Fluids; (United States) Vol. 30:11; ISSN PFLDA
Country of Publication:
United States
Language:
English

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