SolRaT Documentation¶
SolRaT (Solar Radiative Transfer) is a forward-modeling code for the polarized, non-LTE transfer of spectral-line radiation in magnetized stellar atmospheres. It solves the statistical-equilibrium and radiative-transfer equations in the density-matrix formalism of Landi Degl’Innocenti & Landolfi (2004), with interchangeable multi-term and multi-level atoms, for magnetic fields of arbitrary strength from the Zeeman through the Hanle and Paschen-Back regimes.
Browse¶
Check out the SolRaT: Introduction for SolRaT description, the Quick Start & Examples guide for basic usage examples, or dive straight into the full API reference starting with the Built-in Models.