Learning

Spectroscopic Diagnostics of Astrophysical Plasma Conditions

Atomic Structure and Energy Levels → Case Studies in Plasma Diagnostics

This path equips graduate students in astrophysics with the knowledge and skills to use spectroscopy for diagnosing plasma conditions such as temperature, density, and chemical abundances. It covers the essential atomic physics, radiative transfer, and collisional processes, then applies them to diagnostic line ratios and photoionization modeling.