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.

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Detalles Bibliográficos
Autores principales: Wensi Wang, Rui Liu, Yuming Wang, Qiang Hu, Chenglong Shen, Chaowei Jiang, Chunming Zhu
Formato: article
Lenguaje:EN
Publicado: Nature Portfolio 2017
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Acceso en línea:https://doaj.org/article/3a7104d13f5542b7a6e728447236dd7c
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