The ULSA implementation of the NE2001 electron model using in 3D emissivity of galaxy to produce a sky map below 10MHz.
The output can be stored either in memory by means of a numpy array, or in a HDF5 format file.
You need a Fortran compiler (something that implements f77 - gfortran is fine). You need an MPI implementation installed (e.g. libmpich or OpenMPI - see https://github.com/mpi4py/mpi4py. You probably want OpenMPI.
You probably want a Python virtual environment so you might need the venv Python package installed.
Otherwise be bold and ignore the first two lines.
python3 -m venv --system-site-packages venv
source venv/bin/activate
pip install .
This creates a venv in the venv subdirectory. If you don't want it there, just change that last
venv and also change the source line.
Look at example/example.py. You probably want to run this using mpirun to take advantage of multiple
cores on your system (e.g. mpirun python3 example.py).
NOTE: The NE2001 input files (everything ending in .inp or .dat) in that directory are required to run any ULSA program. They have to be located in that directory.
Documentation can be found at https://ulsa.readthedocs.io/en/latest/.
If this code helps you, please refer to the 