Using the National Science Foundation's Daniel K. Inouye Solar Telescope on Maui, an international team recorded the highest-resolution images of the solar photosphere to date. In those images, they found dense fields of small, vortex-like structures along the edges of magnetic regions. The team focused on a magnetically active area near a sunspot, where convection cells, or granules, constantly rise and sink and magnetic fields are concentrated. On the sun, it had been predicted and hinted at in the outer corona, but direct confirmation in the photosphere required the resolution now available from the Inouye Solar Telescope. Kelvin-Helmholtz structures can mix magnetized and non-magnetized plasma efficiently, speeding up the diffusion of magnetic fields through the lower solar atmosphere.