Two–Current‐Sheet Reconnection Model of Interdependent Flare and Coronal Mass Ejection
Author(s) -
Y. Z. Zhang,
Jingang Wang,
Yin Hu
Publication year - 2006
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 - 10.1086/500424
Subject(s) - current sheet , physics , rope , magnetic reconnection , coronal mass ejection , flare , flux (metallurgy) , solar flare , astrophysics , breakout , magnetohydrodynamics , magnetic flux , mechanics , transverse plane , current (fluid) , magnetic field , structural engineering , solar wind , engineering , materials science , finance , quantum mechanics , economics , metallurgy , thermodynamics
Time-dependent resistive magnetohydrodynamic simulations are carried out tostudy a flux rope eruption caused by magnetic reconnection with implication incoexistent flare-CME (coronal mass ejection) events. An early result obtainedin a recent analysis of double catastrophe of a flux rope system is used as theinitial condition, in which an isolated flux rope coexists with two currentsheets: a vertical one below and a transverse one above the flux rope. The fluxrope erupts when reconnection takes place in the current sheets, and the fluxrope dynamics depends on the reconnection sequence in the two current sheets.Three cases are discussed: reconnection occurs (1) simultaneously in the twocurrent sheets, (2) first in the transverse one and then in the vertical, and(3) in an order opposite to case 2. Such a two-current-sheet reconnectionexhibits characteristics of both magnetic breakout for CME initiation andstandard flare model. We argue that both breakout-like and tether-cuttingreconnections may be important for CME eruptions and associated surfaceactivities.Comment: 10 pages, 4 figures, Accepted for publication in ApJ 200
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