A neural-network magnetic field reconstruction shows that a 500 Mm filament's pre-eruption flux rope had an extended eastern footprint connected to the flare ribbon and coronal dimming, explaining the asymmetric eruption.
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Magnetic structure and asymmetric eruption of a 500 Mm filament rooted in weak-field regions
A neural-network magnetic field reconstruction shows that a 500 Mm filament's pre-eruption flux rope had an extended eastern footprint connected to the flare ribbon and coronal dimming, explaining the asymmetric eruption.