How is the area of the convective zone beneath the sun spot different from the are beneath the granulation?

The area of the convective zone beneath a sunspot is characterized by reduced convection due to the intense magnetic fields associated with the sunspot, which suppress the upward flow of hot plasma. In contrast, the area beneath granulation exhibits active convection, where hot plasma rises and cool plasma sinks, creating a dynamic surface pattern. This difference in convective activity results in varying temperature and pressure profiles in these regions, influencing solar phenomena.