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Isotopic overabundances and the energetic particle model of solar flaresAccording to the energetic particle model of solar flares particles are efficiently accelerated in the magnetic field loop of an active region (AR) by hydromagnetic turbulence. It is demonstrated that the isotopic overabundances observed in some flares are not a consequence of the flare itself but are characteristic of the plasma in the AR. Only when a flare releases the plasma into the interplanetary space it is possible to observe this anomalous composition at spacecraft locations.
Document ID
19850026483
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Perez-Enriquez, R.
(Universidad Nacional Autonoma de Mexico Villa Obregon, Mexico)
Bravo, S.
(Universidad Nacional Autonoma de Mexico Villa Obregon, Mexico)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 4
Subject Category
Solar Physics
Report/Patent Number
SH-2.2-1
Report Number: SH-2.2-1
Accession Number
85N34796
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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