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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

A test repository

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.

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

Unet model for solar granular segmentation

Public wiki for all topics related to the KIS Science Data Centre. This Wiki should contain useful information for Users, Developers as well as PI's who want to know how to get their data ingested into the archive.

Template for python projects

Template for python projects

Some IDL and Python routines for working with PcoGui FITS files