Observing the release of twist by magnetic reconnection in a solar filament eruption

Magnetic reconnection is a fundamental process giving rise to topology change and energy release in plasmas, of particular relevance for the Sun. Here the authors report the observation of fast reconnection in a solar filament eruption, which occurs between a set of ambient fibrils and the filament...

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Autores principales:	Zhike Xue, Xiaoli Yan, Xin Cheng, Liheng Yang, Yingna Su, Bernhard Kliem, Jun Zhang, Zhong Liu, Yi Bi, Yongyuan Xiang, Kai Yang, Li Zhao
Formato:	article
Lenguaje:	EN
Publicado:	Nature Portfolio 2016
Materias:	Science Q
Acceso en línea:	https://doaj.org/article/4c46274c8e9341a68ac51204e8df65f2
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spelling	oai:doaj.org-article:4c46274c8e9341a68ac51204e8df65f22021-12-02T15:34:10ZObserving the release of twist by magnetic reconnection in a solar filament eruption10.1038/ncomms118372041-1723https://doaj.org/article/4c46274c8e9341a68ac51204e8df65f22016-06-01T00:00:00Zhttps://doi.org/10.1038/ncomms11837https://doaj.org/toc/2041-1723Magnetic reconnection is a fundamental process giving rise to topology change and energy release in plasmas, of particular relevance for the Sun. Here the authors report the observation of fast reconnection in a solar filament eruption, which occurs between a set of ambient fibrils and the filament itself.Zhike XueXiaoli YanXin ChengLiheng YangYingna SuBernhard KliemJun ZhangZhong LiuYi BiYongyuan XiangKai YangLi ZhaoNature PortfolioarticleScienceQENNature Communications, Vol 7, Iss 1, Pp 1-11 (2016)
institution	DOAJ
collection	DOAJ
language	EN
topic	Science Q
spellingShingle	Science Q Zhike Xue Xiaoli Yan Xin Cheng Liheng Yang Yingna Su Bernhard Kliem Jun Zhang Zhong Liu Yi Bi Yongyuan Xiang Kai Yang Li Zhao Observing the release of twist by magnetic reconnection in a solar filament eruption
description	Magnetic reconnection is a fundamental process giving rise to topology change and energy release in plasmas, of particular relevance for the Sun. Here the authors report the observation of fast reconnection in a solar filament eruption, which occurs between a set of ambient fibrils and the filament itself.
format	article
author	Zhike Xue Xiaoli Yan Xin Cheng Liheng Yang Yingna Su Bernhard Kliem Jun Zhang Zhong Liu Yi Bi Yongyuan Xiang Kai Yang Li Zhao
author_facet	Zhike Xue Xiaoli Yan Xin Cheng Liheng Yang Yingna Su Bernhard Kliem Jun Zhang Zhong Liu Yi Bi Yongyuan Xiang Kai Yang Li Zhao
author_sort	Zhike Xue
title	Observing the release of twist by magnetic reconnection in a solar filament eruption
title_short	Observing the release of twist by magnetic reconnection in a solar filament eruption
title_full	Observing the release of twist by magnetic reconnection in a solar filament eruption
title_fullStr	Observing the release of twist by magnetic reconnection in a solar filament eruption
title_full_unstemmed	Observing the release of twist by magnetic reconnection in a solar filament eruption
title_sort	observing the release of twist by magnetic reconnection in a solar filament eruption
publisher	Nature Portfolio
publishDate	2016
url	https://doaj.org/article/4c46274c8e9341a68ac51204e8df65f2
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Observing the release of twist by magnetic reconnection in a solar filament eruption

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