We compare the zonal flow pattern in subsurface layers of the Sun with the
distribution of surface magnetic features like sunspots and polar faculae. We
demonstrate that in the activity belt, the butterfly pattern of sunspots
coincides with the fast stream of zonal flows, although part of the sunspot
distribution does spill over to the slow stream. At high latitudes, the polar
faculae and zonal flow bands have similar distributions in the spatial and
temporal domains.Comment: To appear in Solar Physic
