Abstract
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, 2 βH, is small enough. This is in contradiction to the previous 'local' analysis.
Original language | English |
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Pages (from-to) | 235-242 |
Number of pages | 8 |
Journal | Solar Physics |
Volume | 89 |
Issue number | 2 |
DOIs | |
Publication status | Published - 1 Dec 1983 |