The stability of magnetohydrostatic atmospheres

Details The stability of magnetohydrostatic atmospheres The stability of magnetohydrostatic atmospheres

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...89..235h&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 89, Dec. 1983, p. 235-242.

Other

11

Magnetohydrodynamic Stability, Solar Atmosphere, Solar Magnetic Field, Displacement, Isothermal Processes, Lines Of Force, Magnetic Field Configurations, Photosphere

Scientific paper

The 'local' stability of Zweibel (1981) is extended, through the application of an analysis developed by Schindler et al. (1983) and Hood (1983), to include the previously neglected magnetic tension terms. It is noted that, for a sufficiently small value of the parameter 2beta(H), a particular magnetohydrostatic field is stable in contradiction to the previous 'local' analysis. It is stressed that a local analysis employed for the prediction of instability cannot neglect any positive terms in the energy integrals.

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