SolRaT Documentation
====================

SolRaT (Solar Radiative Transfer) is a flexible, forward-modeling, non-LTE radiative transfer code for stellar atmospheres. It implements the statistical equilibrium and radiative transfer equations within the multi-term atom model, enabling detailed synthesis of Stokes profiles in magnetic fields of arbitrary strength, from the Zeeman to the Paschen-Back regimes.

`GitHub Repository Link <https://github.com/yakovkinii/SolRaT/>`_

.. image:: https://www.yakovkinii.com/solrat/media/solrat_profiles.png
   :width: 600
   :alt: Model of He I D3 emission in a limb event under different magnetic fields
   :align: center

Browse
------
Check out the :doc:`introduction` for SolRaT description, the :doc:`quickstart` guide for basic usage examples,
or dive straight into the full API reference reference starting with the :doc:`api`.

.. toctree::
   :maxdepth: 1

   introduction
   quickstart

API Reference
-------------

.. toctree::
   :maxdepth: 1
   :caption: Api Reference:

   api