On Statistical Signatures of ISM Turbulence in Dust Polarization Maps - Alexei Kritsuk

Explore statistical signatures of interstellar medium (ISM) turbulence in dust polarization maps through this 28-minute conference talk by Alexei Kritsuk from UCSD. Delivered at the Kavli Institute for Theoretical Physics' "Turbulence in the Universe" conference, delve into the complexities of astrophysical turbulence across various cosmic environments. Gain insights into recent advancements in observational and theoretical studies, and understand the impact of turbulence on different branches of astronomy. Examine topics such as turbulent dynamo, magnetic reconnection, plasma physics, and astrophysical applications of magnetized turbulence, while engaging with interdisciplinary discussions on connecting observations with models and new diagnostic techniques for turbulence.

On statistical signatures of ISM turbulence in dust polarization maps ▸ Alexei Kritsuk (UCSD)