Developing Predictive Models of Turbulent Heating in Space and Astrophysical Plasmas

Explore a detailed physics colloquium that delves into the development of predictive models for understanding turbulent plasma heating in space and astrophysical environments. Learn how these models are crucial for interpreting observations from the Event Horizon Telescope, particularly regarding supermassive black holes in M87 and Sagittarius A*. Discover the fundamental role of turbulence in space and astrophysical plasmas, examining how it facilitates energy transport from large-scale magnetic fields to smaller scales. Understand the innovative field-particle correlation technique and its application in both kinetic numerical simulations and spacecraft measurements of weakly collisional plasma turbulence. Gain insights into the mechanisms controlling plasma turbulence dissipation and the distribution of energy among different plasma species. Follow the progress toward developing turbulent heating prescriptions that can enhance global modeling of astrophysical systems and their evolution.