MHD Turbulence From Idealized Boxes to the ICM - Philipp Grete

Explore magnetohydrodynamic (MHD) turbulence across various scales in this 30-minute conference talk by Philipp Grete from the University of Hamburg. Delivered as part of the "Turbulence in the Universe" conference at the Kavli Institute for Theoretical Physics, delve into the complexities of turbulence in astrophysical environments, from idealized simulation boxes to the intracluster medium (ICM). Gain insights into the latest advancements in observational and theoretical studies of astrophysical turbulence, and understand its significant impact on various branches of astronomy. Discover how this interdisciplinary field connects topics such as turbulent dynamo, magnetic reconnection, plasma physics, and numerical simulations, with applications ranging from star formation to galaxy evolution.