One dimensional transport equations based on a 16 moment approximation for ionized and neutral species.
All data and routines you need for coronal and heliospheric stuff.
If you think something is missing, complain to peter.parker@irap.omp.eu
Computes the magnetic connectivity point at the solar surface for different spacecrafts, times and magnetograms.
For a given magnetogram, compute magnetic field lines from Sun surface to source surface (2.5 Rs).
Use PFSS method.