External reconnection on an erupting solar flux rope removes flux and decelerates the structure, preventing escape under strong magnetic confinement.
H.et al.The Helioseismic and Magnetic Imager (HMI) Investigation for the Solar Dynamics Observatory (SDO).Sol
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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.