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This document investigates the transition of large-scale coronal mass ejections (CMEs) from non-radial to radial propagation, focusing on two CMEs from the same active region. The study highlights the lateral deformation of CMEs during this transition, revealing that the upper flank of the CME bulges toward the higher corona, resulting in a change of direction approximately 25° from the eruption site. This research contributes to a better understanding of CME evolution and its implications for space weather

Author
proninja234
Language
EN