Explore projects

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 = MonteCarlo simulation
Updated 
Updated

Updated

SDC:GRIS Inversion Pipeline
(uses VFISV version 5.0., node for spectrograph data.)
Updated 
Forward and Inverse solver for the polarized radiative transfer equation in geometrical scale "dz". F90, MPI. Dependencies: LAPACK, FFTW
Updated 
Wrapper to calculate synthetic profiles from 3D MHS cubes (i.e. MURAM, CO5BOLD). F90, openMP. Dependencies: SIR
Updated 
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.
Updated 
Very Fast Inversion of the Stokes Vector (VFISV) version 5.0. Node for spectrograph data. Uses: F90, MPICH, LAPACK, CFITSIO
Updated 
Very Fast Inversion of the Stokes Vector (VFISV) version 5.0. Node for Fabry Perot data. Uses: F90, MPICH, LAPACK, CFITSIO
Updated 
MHS module for FIRTEZ inversion code. Clone from mhs_invdata_git Dependencies: openMP, LAPACK, FISHPACK, BLAS
Updated