Transient rotation of photospheric vector magnetic fields associated with a solar flare

The violent solar eruptions known as flares are caused by magnetic reconnection. Here, the authors identify a sudden 12°–20° counter clockwise rotation of vector magnetic fields in photosphere, associated with the emissions of moving flare ribbons.

Bibliographic Details
Main Authors: Yan Xu, Wenda Cao, Kwangsu Ahn, Ju Jing, Chang Liu, Jongchul Chae, Nengyi Huang, Na Deng, Dale E. Gary, Haimin Wang
Format: Article
Language:English
Published: Nature Publishing Group 2018-01-01
Series:Nature Communications
Online Access:https://doi.org/10.1038/s41467-017-02509-w
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spelling doaj-d1a981c6c1d5413ea0c77e9e43dddcbb2021-05-11T09:43:57ZengNature Publishing GroupNature Communications2041-17232018-01-01911810.1038/s41467-017-02509-wTransient rotation of photospheric vector magnetic fields associated with a solar flareYan Xu0Wenda Cao1Kwangsu Ahn2Ju Jing3Chang Liu4Jongchul Chae5Nengyi Huang6Na Deng7Dale E. Gary8Haimin Wang9Space Weather Research Lab, New Jersey Institute of TechnologyBig Bear Solar Observatory, New Jersey Institute of TechnologyBig Bear Solar Observatory, New Jersey Institute of TechnologySpace Weather Research Lab, New Jersey Institute of TechnologySpace Weather Research Lab, New Jersey Institute of TechnologyAstronomy Program, Department of Physics and Astronomy, Seoul National UniversitySpace Weather Research Lab, New Jersey Institute of TechnologySpace Weather Research Lab, New Jersey Institute of TechnologyCenter for Solar-Terrestrial Research, New Jersey Institute of TechnologySpace Weather Research Lab, New Jersey Institute of TechnologyThe violent solar eruptions known as flares are caused by magnetic reconnection. Here, the authors identify a sudden 12°–20° counter clockwise rotation of vector magnetic fields in photosphere, associated with the emissions of moving flare ribbons.https://doi.org/10.1038/s41467-017-02509-w
collection DOAJ
language English
format Article
sources DOAJ
author Yan Xu
Wenda Cao
Kwangsu Ahn
Ju Jing
Chang Liu
Jongchul Chae
Nengyi Huang
Na Deng
Dale E. Gary
Haimin Wang
spellingShingle Yan Xu
Wenda Cao
Kwangsu Ahn
Ju Jing
Chang Liu
Jongchul Chae
Nengyi Huang
Na Deng
Dale E. Gary
Haimin Wang
Transient rotation of photospheric vector magnetic fields associated with a solar flare
Nature Communications
author_facet Yan Xu
Wenda Cao
Kwangsu Ahn
Ju Jing
Chang Liu
Jongchul Chae
Nengyi Huang
Na Deng
Dale E. Gary
Haimin Wang
author_sort Yan Xu
title Transient rotation of photospheric vector magnetic fields associated with a solar flare
title_short Transient rotation of photospheric vector magnetic fields associated with a solar flare
title_full Transient rotation of photospheric vector magnetic fields associated with a solar flare
title_fullStr Transient rotation of photospheric vector magnetic fields associated with a solar flare
title_full_unstemmed Transient rotation of photospheric vector magnetic fields associated with a solar flare
title_sort transient rotation of photospheric vector magnetic fields associated with a solar flare
publisher Nature Publishing Group
series Nature Communications
issn 2041-1723
publishDate 2018-01-01
description The violent solar eruptions known as flares are caused by magnetic reconnection. Here, the authors identify a sudden 12°–20° counter clockwise rotation of vector magnetic fields in photosphere, associated with the emissions of moving flare ribbons.
url https://doi.org/10.1038/s41467-017-02509-w
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