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Neutral beams in two-ribbon flares and in the geomagnetic tailThe current sheet created in the wake of an erupting filament during a two-ribbon flare is studied. A comparison with the geomagnetic tail shows that the physics of these systems is very similar, and therefore the existence of super Dreicer fields and the generation of netural beams traveling down the postflare loops with small pitch angles may be expected. The observational evidence for neutral beams in flares is reviewed and found to be generally supportive, while contracting the widely held hypothesis of electron beams. A dimensional analysis further demonstrates that the results for self-consistent numerical simulations of the current sheet in the geomagnetic tail can directly be scaled to the coronal current sheet, and the scaling parameters are derived.
Document ID
19900052376
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Martens, P. C. H.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Young, A.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 14, 2013
Publication Date
June 1, 1990
Publication Information
Publication: Astrophysical Journal Supplement Series
Volume: 73
ISSN: 0067-0049
Subject Category
Solar Physics
Accession Number
90A39431
Funding Number(s)
CONTRACT_GRANT: NAGW-112
Distribution Limits
Public
Copyright
Other

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