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The generation of proton beams in two-ribbon flaresIt is shown that, in the current sheet at the top of the arcade of postflare loops in a two-ribbon solar flare, particle beams are generated by direct electric-field acceleration. The acceleration process is completely collisionless and is limited only by the gyromotion along the component of the magnetic field perpendicular to the sheet. This mechanism is similar to the particle acceleration in the geomagnetic tail. Neutral beams emanate from the sheet with almost zero pitch angle, making protons the main carriers of the beam energy. Approximately 10 to the 35th protons/sec are generated with a typical energy of 200 keV. Their energy distribution is a single power law, with an upper and lower energy cut-off. Such a population is capable of simultaneously generating the observed impulsive-phase hard X-rays and the gamma rays.
Document ID
19880058924
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Martens, P. C. H.
(NASA Goddard Space Flight Center Greenbelt, MD; Harvard Smithsonian Center for Astrophysics, Cambridge, MA, United States)
Date Acquired
August 13, 2013
Publication Date
July 15, 1988
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters
Volume: 330
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
88A46151
Funding Number(s)
CONTRACT_GRANT: NAGW-112
Distribution Limits
Public
Copyright
Other

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