Bellot Rubio (2003)
Based on SIR, this code is designed to invert Stokes profiles from sunspot penumbrae using uncombed penumbral models.
The model consists of a background component and a flux tube component which is constructed by adding gaussian perturbations to the stratifications of the background. The amplitudes of the gaussian perturbation are different for the different physical quantities, but the perturbation is located at the same height and has the same width for all the physical quantities.
Coming soon!
For questions, please contact Luis Bellot