Sunspot RGN 4366: Flares Observed, CMEs Pending

The region RGN 4366 has developed into a complex sunspot group. This sunspot has generated solar flares ranging from M1 to X1 levels, which are classified as R1 (Minor) to R3 (Strong).

As of the current report, there is no definitive evidence of associated coronal mass ejections (CMEs).

The RGN 4366 region continues to be monitored for further activity.