MHD stability of sheet equilibria relevant for quiescent prominences

Details MHD stability of sheet equilibria relevant for quiescent prominences MHD stability of sheet equilibria relevant for quiescent prominences

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...277..422g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 277, Feb. 1, 1984, p. 422, 423. Research supported by the Deutsche Forschun

Astronomy and Astrophysics

Astrophysics

20

Magnetohydrodynamic Stability, Plasma Equilibrium, Solar Prominences, Solar Magnetic Field

Scientific paper

The authors consider a special class of MHD equilibria and analyze their
stability against arbitrary MHD perturbations by using the MHD energy
principle. These equilibria are shown to be stable. A particular member
of this class of equilibria corresponds to the prominence model of
Kippenhahn and Schlüter.

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