This is the SDC pipeline code for performing inversions of GRIS spectropolarimeteric data.<br>
The code currently uses the [Very Fast Inversion of the Stokes Vector (VFISV)](https://gitlab.leibniz-kis.de/borrero/vfisv_spec) code v5.0 (node for spectrograph data)<br>
as the main backend to carry out a Milne-Eddington Stokes inversion for individual spectral lines.
The manual for the original code can be found here: [manual_vfisv](https://gitlab.leibniz-kis.de/borrero/vfisv_spec/-/blob/master/manual_vfisv.pdf)
as the main backend to carry out a Milne-Eddington Stokes inversion for individual spectral lines.<br>
The manual for the original code can be found here: [manual_vfisv](https://gitlab.leibniz-kis.de/borrero/vfisv_spec/-/blob/master/manual_vfisv.pdf)<br>
This is an implementation of VFISV code to facilitate a seamless processing of the data provided by the SDC.