Formation of Magnetic Flux Rope During Solar Eruption. I. Evolution of Toroidal Flux and Reconnection Flux

Formation of Magnetic Flux Rope During Solar Eruption. I. Evolution of Toroidal Flux and Reconnection Flux

Magnetic flux ropes (MFRs) constitute the core structure of coronal mass ejections (CMEs), but hot debates remain on whether the MFR forms before or during solar eruptions. Furthermore, how flare reconnection shapes the erupting MFR is still elusive in three dimensions. Here we studied a new MHD sim...

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Bibliographic Details
Main Authors: Chaowei Jiang, Jun Chen, Aiying Duan, Xinkai Bian, Xinyi Wang, Jiaying Li, Peng Zou, Xueshang Feng
Format: Article
Language:English
Published: Frontiers Media S.A. 2021-10-01
Series:Frontiers in Physics
Subjects:
magnetic fields
magnetohydrodynamics (MHD)
methods: numerical
sun: corona
sun: flares
Online Access:https://www.frontiersin.org/articles/10.3389/fphy.2021.746576/full

Internet

https://www.frontiersin.org/articles/10.3389/fphy.2021.746576/full

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