Asteroseismology with 3D magneto-hydrodynamical simulations of stellar convection
The last decade has seen a rapid development in asteroseismology thanks to the CoRoT and Kepler missions. With more detailed asteroseismic observations available, it is becoming possible to infer exactly how oscillations are driven and dissipated in solar-type stars. To study this problem from a theoretical perspective, I carried out three-dimensional (3D) stellar atmosphere simulations together with one-dimensional (1D) stellar structural models of the Sun as well as key benchmark turn-off and...[Show more]
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