Image Details
Caption: Figure 2.
Panel (a): HMI magnetogram of the AR 12975 at ∼11:10 UT. Panel (b): EUV observation from AIA-304 of the filament at ∼11:16 UT. Panel (c): initial tracking of the filament performed in A. Sahade et al. (2025) and used as an initial condition for the CORHEL-CME run. Panel (d): yellow axes show the initial location of the eruptive filament in the CORHEL-CME simulation. The colored dots represent the tracked filament.
© 2025. The Author(s). Published by the American Astronomical Society.