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SIR - Multiple Guesses This code uses the inversion code SIR and is parallelized with OpenMPI. There are three different modes: 1C, 2C and MC 1C = 1 Component Inversion with Real Data; 2C = 2 Components Inversion with Real Data; MC = Monte-Carlo simulation

Collection of tools for KIS SDC: (Meta)Data Access wrappers, fits header reformatting, plotting

SDC:GRIS Inversion Pipeline

(uses VFISV version 5.0., node for spectrograph data.)

Forward and Inverse solver for the polarized radiative transfer equation in geometrical scale "dz". F90, MPI. Dependencies: LAPACK, FFTW

Wrapper to calculate synthetic profiles from 3D MHS cubes (i.e. MURAM, CO5BOLD). F90, openMP. Dependencies: SIR

F90+MPI wrapper that reads the output from MuRAM cubes and calculates synthetic Stokes spectra using the SIR code. The conversion to optical depth is done using the same routines as SIR (gas, pe_frompg) to keep consistency between opacity packages.

Very Fast Inversion of the Stokes Vector (VFISV) version 5.0. Node for spectrograph data. Uses: F90, MPICH, LAPACK, CFITSIO

Very Fast Inversion of the Stokes Vector (VFISV) version 5.0. Node for Fabry Perot data. Uses: F90, MPICH, LAPACK, CFITSIO

MHS module for FIRTEZ inversion code. Clone from mhs_invdata_git Dependencies: openMP, LAPACK, FISHPACK, BLAS