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.
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2018-01-01
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Online Access: | https://doi.org/10.1038/s41467-017-02509-w |
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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 |
work_keys_str_mv |
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