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- W2783286350 abstract "Abstract Solar eruptions are well-known drivers of extreme space weather, which can greatly disturb the Earth’s magnetosphere and ionosphere. The triggering process and initial dynamics of these eruptions are still an area of intense study. Here we perform a magnetohydrodynamic simulation taking into account the observed photospheric magnetic field to reveal the dynamics of a solar eruption in a real magnetic environment. In our simulation, we confirmed that tether-cutting reconnection occurring locally above the polarity inversion line creates a twisted flux tube, which is lifted into a toroidal unstable area where it loses equilibrium, destroying the force-free state, and driving the eruption. Consequently, a more highly twisted flux tube is built up during this initial phase, which can be further accelerated even when it returns to a stable area. We suggest that a nonlinear positive feedback process between the flux tube evolution and reconnection is the key to ensure this extra acceleration." @default.
- W2783286350 created "2018-01-26" @default.
- W2783286350 creator A5041690054 @default.
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- W2783286350 date "2018-01-12" @default.
- W2783286350 modified "2023-10-16" @default.
- W2783286350 title "Formation and dynamics of a solar eruptive flux tube" @default.
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- W2783286350 doi "https://doi.org/10.1038/s41467-017-02616-8" @default.
- W2783286350 hasPubMedCentralId "https://www.ncbi.nlm.nih.gov/pmc/articles/5766525" @default.
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- W2783286350 hasPublicationYear "2018" @default.
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