Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption

Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption

Solar eruptions heavily influence space weather, but what are their causes remains an open question. Here the authors present a magnetohydrodynamic model of a solar eruption directly driven by solar magnetograms, following the transition from pre-eruptive to eruptive state.

Bibliographic Details
Main Authors: Chaowei Jiang, S. T. Wu, Xuesheng Feng, Qiang Hu
Format: Article
Language:English
Published: Nature Publishing Group 2016-05-01
Series:Nature Communications
Online Access:https://doi.org/10.1038/ncomms11522
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spelling doaj-259a9df3d88e4fa19404175f2578dcdc2021-05-11T10:58:39ZengNature Publishing GroupNature Communications2041-17232016-05-017111110.1038/ncomms11522Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruptionChaowei Jiang0S. T. Wu1Xuesheng Feng2Qiang Hu3SIGMA Weather Group, State Key Laboratory for Space Weather, National Space Science Center, Chinese Academy of Sciences, No.1 Nan-Er-Tiao, Zhong-Guan-Cun, Hai-Dian District, Beijing 100190, ChinaCenter for Space Plasma & Aeronomic Research, The University of Alabama in HuntsvilleSIGMA Weather Group, State Key Laboratory for Space Weather, National Space Science Center, Chinese Academy of Sciences, No.1 Nan-Er-Tiao, Zhong-Guan-Cun, Hai-Dian District, Beijing 100190, ChinaCenter for Space Plasma & Aeronomic Research, The University of Alabama in HuntsvilleSolar eruptions heavily influence space weather, but what are their causes remains an open question. Here the authors present a magnetohydrodynamic model of a solar eruption directly driven by solar magnetograms, following the transition from pre-eruptive to eruptive state.https://doi.org/10.1038/ncomms11522
collection DOAJ
language English
format Article
sources DOAJ
author Chaowei Jiang
S. T. Wu
Xuesheng Feng
Qiang Hu
spellingShingle Chaowei Jiang
S. T. Wu
Xuesheng Feng
Qiang Hu
Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption
Nature Communications
author_facet Chaowei Jiang
S. T. Wu
Xuesheng Feng
Qiang Hu
author_sort Chaowei Jiang
title Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption
title_short Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption
title_full Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption
title_fullStr Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption
title_full_unstemmed Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption
title_sort data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption
publisher Nature Publishing Group
series Nature Communications
issn 2041-1723
publishDate 2016-05-01
description Solar eruptions heavily influence space weather, but what are their causes remains an open question. Here the authors present a magnetohydrodynamic model of a solar eruption directly driven by solar magnetograms, following the transition from pre-eruptive to eruptive state.
url https://doi.org/10.1038/ncomms11522
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AT stwu datadrivenmagnetohydrodynamicmodellingofafluxemergingactiveregionleadingtosolareruption
AT xueshengfeng datadrivenmagnetohydrodynamicmodellingofafluxemergingactiveregionleadingtosolareruption
AT qianghu datadrivenmagnetohydrodynamicmodellingofafluxemergingactiveregionleadingtosolareruption
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