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Magnetohydrodynamic instabilityThere have been major advances in the theory of magnetic reconnection and of magnetic instability, with important implications for the observations, as follows: (1) Fast and slow magnetic shock waves are produced by the magnetohydrodynamics of reconnection and are potential particle accelerators. (2) The impulsive bursty regime of reconnection gives a rapid release of magnetic energy in a series of bursts. (3) The radiative tearing mode creates cool filamentary structures in the reconnection process. (4) The stability analyses imply that an arcade can become unstable when either its height or twist of plasma pressure become too great.
Document ID
19870009896
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Priest, E. R.
(Saint Andrew's Univ. United Kingdom)
Cargill, P.
(Maryland Univ. College Park, United States)
Forbes, T. G.
(New Hampshire Univ. Durham, United States)
Hood, A. W.
(Saint Andrew's Univ. United Kingdom)
Steinolfson, R. S.
(California Univ. Berkeley, United States)
Date Acquired
September 5, 2013
Publication Date
December 1, 1986
Publication Information
Publication: NASA. Goddard Space flight Center Energetic Phenomena on the Sun. The Solar Maximum Mission Flare Workshop. Proceedings
Subject Category
Solar Physics
Accession Number
87N19329
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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