Reconstruction of a Highly Twisted Magnetic Flux Rope for an Inter-active-region X-Class Solar Flare

Reconstruction of a Highly Twisted Magnetic Flux Rope for an Inter-active-region X-Class Solar Flare

Solar eruptions are manifestation of explosive release of magnetic energy in the Sun's corona. Large solar eruptions originate mostly within active regions, where strong magnetic fields concentrate on the solar surface. Here we studied the magnetic field structure for an exception, which is a p...

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Bibliographic Details
Main Authors: Chaowei Jiang, Aiying Duan, Xueshang Feng, Peng Zou, Pingbing Zuo, Yi Wang
Format: Article
Language:English
Published: Frontiers Media S.A. 2019-10-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
magnetic fields
methods: numerical
sun: corona
sun: flares
sun: filaments
Online Access:https://www.frontiersin.org/article/10.3389/fspas.2019.00063/full

Internet

https://www.frontiersin.org/article/10.3389/fspas.2019.00063/full

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