External reconnection on an erupting solar flux rope removes flux and decelerates the structure, preventing escape under strong magnetic confinement.
M.et al.Coronal dimmings and what they tell us about solar and stellar coronal mass ejections.Living Rev
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Multi-Viewpoint Observation of a Failed Prominence Eruption on the Sun
External reconnection on an erupting solar flux rope removes flux and decelerates the structure, preventing escape under strong magnetic confinement.