Lateral Deformation of Large-scale Coronal Mass Ejections during the Transition from Non-radial to Radial Propagation
Huidong Hu (1), Chong Chen (2), Yiming Jiao (1), Bei Zhu (3), Rui Wang (1), Xiaowei Zhao (4), Liping Yang (1) ((1) NSSC, CAS, (2) HUTB, China (3) Space Eng. U., China (4) NSMC, CMA)

TL;DR
This study investigates how large-scale coronal mass ejections deform laterally during their transition from non-radial to radial propagation in the low corona, revealing the deformation process and magnetic influences involved.
Contribution
It provides the first detailed analysis of lateral deformation during CME directional transition in the low corona, enhancing understanding of CME evolution.
Findings
CMEs transition from non-radial to radial by bulging their upper flanks.
Magnetic tension from overlying loops constrains CME expansion during transition.
Part of the filament shifts southward, indicating complex CME features.
Abstract
Many coronal mass ejections (CMEs) initially propagate non-radially, and then transition to radial propagation in the corona. This directional transition is a significant process that determines a CME's space weather effects but remains poorly understood. Based on multi-wavelength observations, we investigate the transition from non-radial to radial propagation in the low corona for two large-scale CMEs from the same active region on the solar limb. In the beginning, both CMEs move in a non-radial direction, beneath a system of overlying loops that are roughly parallel to the flux-rope axis. The CMEs laterally deform by bulging their upper flanks in the non-radial stage toward the higher corona, which results in the transition to a radial propagation direction approximately 25 away from the eruption site. After the directional transition, the non-radial-stage upper flank becomes…
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