Differential Measures for Magnetic Field Strength in Turbulent - Dmitri Pogosyan
Kavli Institute for Theoretical Physics via YouTube
Overview
Explore differential measures for magnetic field strength in turbulent environments through this 25-minute conference talk by Dmitri Pogosyan from the University of Alberta. Recorded as part of the "Turbulence in the Universe" conference at the Kavli Institute for Theoretical Physics, delve into advanced concepts in astrophysical turbulence. Gain insights into the latest research on magnetic field strength measurements in turbulent conditions, applicable to various cosmic environments from stellar interiors to intergalactic spaces. Understand how these measures contribute to our knowledge of astrophysical processes, magnetic dynamos, and the evolution of cosmic structures. Benefit from interdisciplinary discussions that bridge observational techniques, theoretical models, and numerical simulations in the study of magnetized turbulence across different scales of the universe.
Syllabus
Differential Measures for Magnetic Field Strength in Turbulent â–¸ Dmitri Pogosyan (U. Alberta)
Taught by
Kavli Institute for Theoretical Physics