Vorticity is ubiquitous in turbulent fluids and the Sun is no exception. This ghostly image shows the enstrophy, which is the magnitude of the vorticity vector squared, in a numerical simulation of solar convection. A Molleweide projection is shown near the middle of the convection zone, about 100 Mm below the solar surface. The enstrophy is very intermittent, confined to very strong downflow plumes and lanes which produce vortex rings and sheets through the entrainment of surrounding plasma.