2D/3D Model of Steady Corotating Solar Wind Streams

A Reduced-Physics Hydrodynamic Model of Steady Corotating Solar Wind Streams [Pizzo 1979, Pizzo 1980].

Dependencies

1. Python >= 3.7
2. numpy >= 1.19.1
3. matplotlib >= 3.3.1
4. scipy >= 1.5.0
5. pyhdf >= 0.10.2
6. psipy >= 0.1.1
7. heliopy >= 0.15.3
8. sunpy >= 3.0.1

Data

All data from MAS MHD model results can be downloaded using PsiPy and HelioPy.

Correspondence

Opal Issan (PhD student), University of California, San Diego. oissan@ucsd.edu

License

MIT