A Study of Pre-flare Solar Coronal Magnetic Fields: Magnetic Flux Ropes

Magnetic flux ropes (MFRs) are thought to be the central structures of solar eruptions, and their ideal MHD instabilities can trigger the eruption. Here we performed a study of all the MFR configurations that lead to major solar flares, either eruptive or confined, from 2011 to 2017 near the solar d...

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Bibliographic Details
Published in:	The Astrophysical journal Vol. 884; no. 1; pp. 73 - 88
Main Authors:	Duan, Aiying, Jiang, Chaowei, He, Wen, Feng, Xueshang, Zou, Peng, Cui, Jun
Format:	Journal Article
Language:	English
Published:	Philadelphia The American Astronomical Society 10.10.2019 IOP Publishing
Subjects:	Astrophysics Control stability Coronal magnetic fields Magnetic fields Magnetic flux Magnetic reconnection Magnetism Magnetohydrodynamics Parameters Solar active region magnetic fields Solar corona Solar coronal mass ejections Solar filament eruptions Solar flares Solar magnetic field Solar magnetic fields Solar prominences Three dimensional models Toruses
ISSN:	0004-637X, 1538-4357
Online Access:	Get full text
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