Formation and dynamics of a solar eruptive flux tube
Solar eruptions are large explosions occurring in the solar atmosphere. Here, the authors perform magnetohydrodynamic simulations to unveil the dynamics of a solar eruption, and find that these are dominated by nonlinear processes involving flux tube evolution and reconnection.
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Nature Publishing Group
2018-01-01
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Series: | Nature Communications |
Online Access: | https://doi.org/10.1038/s41467-017-02616-8 |
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doaj-58e44c2c53864bb9a6b96371022cf9aa2021-05-11T10:29:44ZengNature Publishing GroupNature Communications2041-17232018-01-019111110.1038/s41467-017-02616-8Formation and dynamics of a solar eruptive flux tubeSatoshi Inoue0Kanya Kusano1Jörg Büchner2Jan Skála3Max-Planck Institute for Solar System ResearchInstitute for Space-Earth Environmental Research, Nagoya UniversityMax-Planck Institute for Solar System ResearchMax-Planck Institute for Solar System ResearchSolar eruptions are large explosions occurring in the solar atmosphere. Here, the authors perform magnetohydrodynamic simulations to unveil the dynamics of a solar eruption, and find that these are dominated by nonlinear processes involving flux tube evolution and reconnection.https://doi.org/10.1038/s41467-017-02616-8 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Satoshi Inoue Kanya Kusano Jörg Büchner Jan Skála |
spellingShingle |
Satoshi Inoue Kanya Kusano Jörg Büchner Jan Skála Formation and dynamics of a solar eruptive flux tube Nature Communications |
author_facet |
Satoshi Inoue Kanya Kusano Jörg Büchner Jan Skála |
author_sort |
Satoshi Inoue |
title |
Formation and dynamics of a solar eruptive flux tube |
title_short |
Formation and dynamics of a solar eruptive flux tube |
title_full |
Formation and dynamics of a solar eruptive flux tube |
title_fullStr |
Formation and dynamics of a solar eruptive flux tube |
title_full_unstemmed |
Formation and dynamics of a solar eruptive flux tube |
title_sort |
formation and dynamics of a solar eruptive flux tube |
publisher |
Nature Publishing Group |
series |
Nature Communications |
issn |
2041-1723 |
publishDate |
2018-01-01 |
description |
Solar eruptions are large explosions occurring in the solar atmosphere. Here, the authors perform magnetohydrodynamic simulations to unveil the dynamics of a solar eruption, and find that these are dominated by nonlinear processes involving flux tube evolution and reconnection. |
url |
https://doi.org/10.1038/s41467-017-02616-8 |
work_keys_str_mv |
AT satoshiinoue formationanddynamicsofasolareruptivefluxtube AT kanyakusano formationanddynamicsofasolareruptivefluxtube AT jorgbuchner formationanddynamicsofasolareruptivefluxtube AT janskala formationanddynamicsofasolareruptivefluxtube |
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1721448044709281792 |