Explore projects

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.

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.

Unet model for solar granular segmentation

BIOSPI python software package

code for spectroscopic version of Cassda-GUI

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

Code for Cassda GUI

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

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.

Template for python projects

SDC:GRIS Inversion Pipeline

(uses VFISV version 5.0., node for spectrograph data.)