Solar particle events with anomalously large relative abundance of He-3
Author(s) -
Aristides T. Serlemitsos,
V. K. Balasubrahmanyan
Publication year - 1975
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/153592
Subject(s) - physics , solar energetic particles , astrophysics , solar flare , abundance (ecology) , solar physics , astronomy , particle acceleration , radiation , particle (ecology) , electron , nuclear physics , coronal mass ejection , solar wind , plasma , oceanography , fishery , biology , geology
Energetic particle data are presented from a series of solar flares with a relative abundance of He-3 much higher than that of any previous events. The abundance of protons relative to He nuclei was significantly low in these events; not more than four H-2 and three H-3 were detected during the entire period under study, compared with 1110 He-3 nuclei. Results from these experiments are compared with data available from other investigations, and the limitations the former observations place on theoretical models to explain He-3-rich flares are discussed.
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