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On magnetic field stochasticity and nonthermal line broadening in solar flaresObservations of nonthermal line broadening seen in solar flares by the Solar Maximum Mission satellite are discussed in light of recent results on the generation of magnetic field stochasticity. It is shown that a consistent model for the data can be constructed by assuming that the observations signal the destruction of an ambient magnetohydrodynamic equilibrium.
Document ID
19860046054
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Antonucci, E.
(Torino, Universita Turin, Italy)
Rosner, R.
(Turin Univ. Italy)
Tsinganos, K.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 12, 2013
Publication Date
February 15, 1986
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 301
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
86A30792
Funding Number(s)
CONTRACT_GRANT: NAGW-112
CONTRACT_GRANT: NAGW-79
Distribution Limits
Public
Copyright
Other

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