Flare differentially rotates sunspot on Sun’s surface
Sunspots are concentration of magnetic field visible on the solar surface, which were thought to be unaffected by solar flares that take place in the solar corona. Here the authors report evidence of a flare-induced rotation of a sunspot, showing nonuniform acceleration following the peaks of X-ray...
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2016-10-01
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Online Access: | https://doi.org/10.1038/ncomms13104 |
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doaj-504814b990d04ef1ac2f0904bb79121a2021-05-11T10:56:25ZengNature Publishing GroupNature Communications2041-17232016-10-01711910.1038/ncomms13104Flare differentially rotates sunspot on Sun’s surfaceChang Liu0Yan Xu1Wenda Cao2Na Deng3Jeongwoo Lee4Hugh S. Hudson5Dale E. Gary6Jiasheng Wang7Ju Jing8Haimin Wang9Space Weather Research Laboratory, New Jersey Institute of Technology, University HeightsSpace Weather Research Laboratory, New Jersey Institute of Technology, University HeightsBig Bear Solar Observatory, New Jersey Institute of TechnologySpace Weather Research Laboratory, New Jersey Institute of Technology, University HeightsSpace Weather Research Laboratory, New Jersey Institute of Technology, University HeightsSchool of Physics and Astronomy, University of GlasgowCenter for Solar-Terrestrial Research, New Jersey Institute of Technology, University HeightsSpace Weather Research Laboratory, New Jersey Institute of Technology, University HeightsSpace Weather Research Laboratory, New Jersey Institute of Technology, University HeightsSpace Weather Research Laboratory, New Jersey Institute of Technology, University HeightsSunspots are concentration of magnetic field visible on the solar surface, which were thought to be unaffected by solar flares that take place in the solar corona. Here the authors report evidence of a flare-induced rotation of a sunspot, showing nonuniform acceleration following the peaks of X-ray emissions.https://doi.org/10.1038/ncomms13104 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Chang Liu Yan Xu Wenda Cao Na Deng Jeongwoo Lee Hugh S. Hudson Dale E. Gary Jiasheng Wang Ju Jing Haimin Wang |
spellingShingle |
Chang Liu Yan Xu Wenda Cao Na Deng Jeongwoo Lee Hugh S. Hudson Dale E. Gary Jiasheng Wang Ju Jing Haimin Wang Flare differentially rotates sunspot on Sun’s surface Nature Communications |
author_facet |
Chang Liu Yan Xu Wenda Cao Na Deng Jeongwoo Lee Hugh S. Hudson Dale E. Gary Jiasheng Wang Ju Jing Haimin Wang |
author_sort |
Chang Liu |
title |
Flare differentially rotates sunspot on Sun’s surface |
title_short |
Flare differentially rotates sunspot on Sun’s surface |
title_full |
Flare differentially rotates sunspot on Sun’s surface |
title_fullStr |
Flare differentially rotates sunspot on Sun’s surface |
title_full_unstemmed |
Flare differentially rotates sunspot on Sun’s surface |
title_sort |
flare differentially rotates sunspot on sun’s surface |
publisher |
Nature Publishing Group |
series |
Nature Communications |
issn |
2041-1723 |
publishDate |
2016-10-01 |
description |
Sunspots are concentration of magnetic field visible on the solar surface, which were thought to be unaffected by solar flares that take place in the solar corona. Here the authors report evidence of a flare-induced rotation of a sunspot, showing nonuniform acceleration following the peaks of X-ray emissions. |
url |
https://doi.org/10.1038/ncomms13104 |
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