Image Details
Caption: Figure 4.
Evolution of the distances from the region’s fronts to the flaring PILs in all cases, with red (green) for the B h -increase region (flare ribbons). The subcaptions indicate case numbers in Table 1. The vertical lines mark the flare’s start. The shaded regions mark the coexistence duration of the B h increase and flare ribbons.
© 2022. The Author(s). Published by the American Astronomical Society.