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.
Main Authors: | Chaowei Jiang, S. T. Wu, Xuesheng Feng, Qiang Hu |
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Format: | Article |
Language: | English |
Published: |
Nature Publishing Group
2016-05-01
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Series: | Nature Communications |
Online Access: | https://doi.org/10.1038/ncomms11522 |
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