Introduction (definitions), Absorption and emission coefficient, Transfer equation, Radioactive equilibrium, Grey atmosphere, Continuum absorption coefficient, Model atmosphere (hydrostatic equilibrium, temperature distribution, …), Line absorption coefficient, Behavior of spectral lines, Chemical analysis, Stellar rotation, Turbulence in stellar atmospheres.

Type of methodology: Combination of lecture and hands-on

Participants receive the certificate of attendance: Yes

Paid training activity for participants: Yes, for all

Participants prerequisite knowledge: Numerical methods (linear algebra, statistics); Domain-specific background knowledge