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The magnetic field topology associated with two M flares

✍ Scribed by M.L. Luoni; C.H. Mandrini; G.D. Cristiani; P. Démoulin


Book ID
108065971
Publisher
Elsevier Science
Year
2007
Tongue
English
Weight
902 KB
Volume
39
Category
Article
ISSN
0273-1177

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On the assumption that solar flares are due to instabilities which occur in current sheets in the Sun's atmosphere, one may classiC, magnetic-field configurations associated with [lares into two types. One is characterized by 'closed' current sheets, magnetic-field lines adjacent to these sheets beg