![Samuel Sam van Kooten](/aps/sites/default/files/styles/small/public/people/van_kooten_sam.png?itok=6MxURDtr)
I'm investigating the motion of magnetic bright points between the granules on the Sun's surface. This motion produces Alfven waves that heat the corona, and a better understanding here will benefit models of coronal heating as well as provide predictions for DKIST.