A Model of Solar Magnetic Flux Rope Eruption Initiated Primarily by Magnetic Reconnection

There is a heated debate regarding the specific roles played by ideal magnetohydrodynamic (MHD) instability and magnetic reconnection in the causes of solar eruptions. In the context with a pre-existing magnetic flux rope (MFR) before an eruption, it is widely believed that an ideal MHD instability,...

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Veröffentlicht in:	arXiv.org 2024-02
Hauptverfasser:	Liu, Qingjun, Jiang, Chaowei, Bian, Xinkai, Feng, Xueshang, Zuo, Pingbing, Wang, Yi
Format:	Artikel
Sprache:	eng
Schlagworte:	Current sheets Magnetic flux Magnetohydrodynamic stability Magnetohydrodynamics Stability Toruses
Online-Zugang:	Volltext
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