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Qt-based C++ library and tools for DCP

Access HMI, AIA and MDI data with Python

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.

Common configuration stuff such as the python environment

BIOSPI python software package

Unet model for solar granular segmentation

Sample files for different instruments at KIS. Contains data as well as python classes for simple access

These are the slides, homeworks, hands-on exercises (including the code), for the course on theoretical astrophysics II: polarized radiative transfer

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

Code for Cassda GUI

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

Merged routines for data reduction of GRIS data. Mirrored to the reduction machine on tenerife.

Library of standard keyword definitions, instrument header templates and patches

Template for python projects