Transition from eruptive to confined flares in the same active region⋆

Author： Zuccarello F. P.   Chandra R.   Schmieder B.   Aulanier G.   Joshi R.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|601|issue|A26-A26

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.601, Iss.issue, 2017-04, pp. : A26-A26

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Abstract

Context. Solar flares are sudden and violent releases of magnetic energy in the solar atmosphere that can be divided into two classes: eruptive flares, where plasma is ejected from the solar atmosphere resulting in a coronal mass ejection (CME), and confined flares, where no CME is associated with the flare.

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