An energy method for the stability of solar magneto hydrostatic atmospheres
作者:
A.W. Hood,
期刊:
Geophysical & Astrophysical Fluid Dynamics
(Taylor Available online 1984)
卷期:
Volume 28,
issue 3-4
页码: 223-241
ISSN:0309-1929
年代: 1984
DOI:10.1080/03091928408230365
出版商: Taylor & Francis Group
数据来源: Taylor
摘要:
The energy method of Bernsteinet al.(1958) was used by Schindleret al.(1983) to derive a useful form of the linearised potential energy for coronal arcades. The basic state magnetic field and plasma are assumed to be in magnetohydrostatic equilibrium and independent of variations along the length of the arcade. A sufficient condition for stability is derived and is applied to two particular magnetic structures. When the axial field component vanishes, this condition becomes necessary and suficient.
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