,1,This video shows a section from a 3D simulation with a dynamo magnetic field at a resolution of 5 kilometres. The section is taken near the base of the chromosphere, where the flow is dominated by shock waves. The part on the left shows the vertical velocity of the plasma; the video on the right shows the magnetic field. In both representations, bright regions indicate flows towards the viewer; black regions are flows towards the Sun’s interior. In this side-by-side view, the connection between the magnetic field and the plasma becomes apparent, for instance when looking at the vortexes forming near the upper edge of the section. Such vortexes are, in fact, facilitating heat transfer from the magnetic field to the plasma, as the simulation results showed. Video credit: E. Khomenko
