Learning

Plasma Physics in Astrophysics

Classical Electrodynamics → Plasma in Accretion Disks

This graduate-level learning path systematically covers the essential plasma physics concepts applied to astrophysical environments. It begins with foundational physics and progresses through single-particle motion, fluid descriptions, waves, instabilities, shocks, magnetic reconnection, and finally applications to stars, the interstellar medium, and accretion disks. The path emphasizes the physical principles and mathematical tools necessary to understand and model astrophysical plasmas.