Learning

Spectral Diagnostics of Solar Plasma

Solar Atmosphere Structure → CHIANTI Atomic Database

This learning path equips graduate students in solar physics with the knowledge and skills to diagnose plasma conditions in the solar atmosphere using spectroscopic observations. It covers the essential atomic physics, radiative transfer, and line formation theory, followed by practical diagnostics for temperature, density, velocity, and elemental abundances. The path emphasizes the physical principles underlying each diagnostic technique and the interpretation of spectral observations.