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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

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

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

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

Code for Cassda GUI

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