Buildup of a highly twisted magnetic flux rope during a solar eruption
Solar eruptions provide opportunities to study magnetic flux ropes, a structure of fundamental importance for both plasma physics and space weather. Here the authors reveal the dynamic formation of a flux rope through its footprint on the solar surface, revealing a highly twisted core structure.
Enregistré dans:
Auteurs principaux: | Wensi Wang, Rui Liu, Yuming Wang, Qiang Hu, Chenglong Shen, Chaowei Jiang, Chunming Zhu |
---|---|
Format: | article |
Langue: | EN |
Publié: |
Nature Portfolio
2017
|
Sujets: | |
Accès en ligne: | https://doaj.org/article/3a7104d13f5542b7a6e728447236dd7c |
Tags: |
Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
|
Documents similaires
-
The role of non-axisymmetry of magnetic flux rope in constraining solar eruptions
par: Ze Zhong, et autres
Publié: (2021) -
Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption
par: Chaowei Jiang, et autres
Publié: (2016) -
Observing the release of twist by magnetic reconnection in a solar filament eruption
par: Zhike Xue, et autres
Publié: (2016) -
Direct evidence of secondary reconnection inside filamentary currents of magnetic flux ropes during magnetic reconnection
par: Shimou Wang, et autres
Publié: (2020) -
Statistical Study of Small-Scale Interplanetary Magnetic Flux Ropes in the Vicinity of the Heliospheric Current Sheet
par: Qiang Liu, et autres
Publié: (2021)