Using the analysis of Schindler et al. (1983) and Hood (1983), the ‘local’ stability of Zweibel (1981) is extended to include the previously neglected magnetic tension terms. A particular magnetohydrostatic field is shown to be stable if the parameter, 2βH, is small enough. This is in contradiction to the previous ‘local’ analysis.
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Bernstein, I. B., Frieman, E. A., Kruskal, M. D., and Kulsrud, R. M.: 1958, Proc. Roy. Soc. London A244, 17.
Hood, A. W.: 1983, Geophys. Astrophys. Fluid Dynamics, submitted.
Schindler, K., Birn, J., and Janicke, L.: 1983, Solar Phys. 87, 103.
Zweibel, E. G.: 1981, Astrophys. J. 249, 731.
Zweibel, E. G. and Hundhausen, A. J.: 1982, Solar Phys. 76, 261.
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Hood, A.W. The stability of magnetohydrostatic atmospheres. Sol Phys 89, 235–242 (1983). https://doi.org/10.1007/BF00217247
- Tension Term
- Magnetic Tension