MHD Turbulence - What the 3D Magnetic Field Observations Are Revealing - Mehrnoosh Tahani

Explore a 32-minute conference talk on magnetohydrodynamic (MHD) turbulence and its revelations through 3D magnetic field observations. Delve into the latest findings presented by Mehrnoosh Tahani from Stanford University at the Turbulence in the Universe conference. Gain insights into the importance of turbulence in various astrophysical environments, from stellar interiors to the intra-cluster medium. Discover how recent advances in observational and theoretical studies have impacted multiple branches of astronomy. Learn about topics such as turbulent dynamo, magnetic reconnection, plasma physics, and astrophysical applications of magnetized turbulence. Understand the interdisciplinary nature of this research and its implications for star formation, cosmic rays, accretion, and galaxy formation and evolution.

MHD turbulence: What the 3D magnetic field observations are revealing ▸ Mehrnoosh Tahani (Stanford)