Interaction of sound waves with Solar granulation
The energy transport near the surface of the Sun and other Sun-like stars is dominated by convection, leading to the granulation visible at the solar surface. The near surface convection also excites sound waves traveling throughout the stars, allowing us to study their interiors. Unfortunately the interaction between these phenomena is poorly understood.
In this project we will study this interaction using hydrodynamic simulations and look at some of the observable effects on the Sun and other stars. This work is important, not just because it presents an interesting physical problem, but also because it will allow us to make better use of solar observations.