I'm interested in astrophysical fluid dynamics and magnetohydrodymanics, particularly as it applies to the interior of the Sun and other stars. Most of my recent work focuses on high-resolution numerical simulations of convection, turbulence, and shear in the solar interior and the implications all this has for solar dynamo theory and for detectable surface flows such as differential rotation and solar sub-surface weather. I've also done some work on turbulence and waves in interstellar molecular clouds.

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