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...
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: | |
Online Access: | https://www.frontiersin.org/article/10.3389/fspas.2019.00063/full |
Similar Items
-
Formation of Magnetic Flux Rope During Solar Eruption. I. Evolution of Toroidal Flux and Reconnection Flux
by: Chaowei Jiang, et al.
Published: (2021-10-01) -
Formation of Magnetic Flux Rope During Solar Eruption. I. Evolution of Toroidal Flux and Reconnection Flux
by: Bian, X., et al.
Published: (2021) -
Evolution of the Toroidal Flux of CME Flux Ropes during Eruption
by: Chen Xing, et al.
Published: (2020-11-01) -
Plasma Heating Induced by Tadpole-like Downflows in the Flaring Solar Corona
by: Tanmoy Samanta, et al.
Published: (2021-02-01) -
North-South Distribution and Asymmetry of GOES SXR Flares during Solar Cycle 24
by: Joshi Anita, et al.
Published: (2020-02-01)