Sun image in Mg II h line (NB4): Similar to NB3, NB4 shows the bright active regions on the Solar disk. The active regions signify magnetically active regions on the Sun’s surface. Solar flares may originate in these active regions due to changes in magnetic fields. The Sun is moving towards solar maximum, giving rise to enhanced activity. So, there are several active regions visible around the equatorial region.
X (@ISRO_ADITYAL1)