Kinetic Mechanisms for the Dissipation of Turbulence and Their Dependence on the Turbulence Parameters
Kavli Institute for Theoretical Physics via YouTube
Overview
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Explore a thought-provoking discussion led by Greg Howes from the University of Iowa on kinetic mechanisms for turbulence dissipation and their dependence on turbulence parameters. Recorded during the "Turbulence in the Universe" conference at the Kavli Institute for Theoretical Physics, this 1-hour 6-minute talk delves into the complex world of astrophysical turbulence. Gain insights into how turbulence impacts various cosmic environments, from stellar interiors to galaxy clusters. Discover recent advances in observational and theoretical studies of astrophysical turbulence and their implications for multiple branches of astronomy. Engage with interdisciplinary perspectives on topics such as turbulent dynamo, magnetic reconnection, plasma physics, and numerical simulations. Enhance your understanding of magnetized turbulence and its applications in star formation, cosmic rays, accretion, and galaxy evolution.
Syllabus
Discussion led by Greg Howes (Iowa): Kinetic Mechanisms for the Dissipation of Turbulence and...
Taught by
Kavli Institute for Theoretical Physics