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.
Main Authors: | Satoshi Inoue, Kanya Kusano, Jörg Büchner, Jan Skála |
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Format: | Article |
Language: | English |
Published: |
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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