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Investigations of turbulent motions and particle acceleration in solar flaresInvestigations of X-raya spectra of solar flares show that intense random (turbulent) motions are present in hot flare plasma. Here it is argued that the turbulent motions are of great importance for flare development. They can efficiently enhance flare energy release and accelerate particles to high energies.
Document ID
19870052739
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0273-1177(86)90143-2
Authors
Jakimiec, J. (Wroclaw Univ. Poland)
Fludra, A. (Wroclaw Uniwersytet, Poland)
Lemen, J. R. (London, University College, Dorking, United Kingdom)
Dennis, B. R. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Sylwester, J. (Polska Akademiia Nauk Centrum Badan Kosmicznych, Wroclaw, Poland)
Date Acquired
August 13, 2013
Publication Date
January 1, 1986
Publication Information
Publication: Advances in Space Research
Volume: 6
Issue: 6, 19
ISSN: 0273-1177
Subject Category
Solar Physics
Accession Number
87A40013
Distribution Limits
Public
Copyright
Other

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