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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Vydané v:	The Astrophysical journal Ročník 884; číslo 1; s. 73 - 88
Hlavní autori:	Duan, Aiying, Jiang, Chaowei, He, Wen, Feng, Xueshang, Zou, Peng, Cui, Jun
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	Philadelphia The American Astronomical Society 10.10.2019 IOP Publishing
Predmet:	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
On-line prístup:	Získať plný text
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