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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

Set of routines and wrappers used for calibrating and splitting GRIS data at KIS This project is outdated! All development is done in the new grisred repo!

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

Quality estimation for ChroTel data using simple descriptive statistics and unsupervised learning techniques.

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

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

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

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