Image Details
Caption: Figure 1.
The evolutionary trends of: flare events of various classes (panel (a)), the green line emissions at different latitudes (panel (b)), and sunspot numbers with F10.7 cm radio flux (panel (c)). The X-class flare curve, in panel (a), is scaled by a factor of 10 for better visualization.
© 2025. The Author(s). Published by the American Astronomical Society.