Confinedness of an X3.1 class solar flare occurred in NOAA 12192: Analysis from multi-instruments observations

The non-association of coronal mass ejections with high energetic flares is sparse. For this reason, the magnetic conditions required for the confinedness of major flares is a topic of active research. Using multi-instrument observations, we investigated the evolution and effects of confinedness in an X3.1 flare, which occurred in active... Show more