Rees-Sergienko-Ivanov Auroral model
Rees-Sergienko-Ivanov model of excitation rates, relevant to auroral optical emissions inspired/based upon Gustavsson / Brandstrom et al AIDA_Tools
Model designed for 100 - 10,000 eV, and is essentially a parameter fit to more advanced models, making for convenient computation in this energy range with the PCs of the early 1990s. Today, much more advanced physics-based models are tractable on a PC.
Uses MSISE-00 to generate O, O
2, N 2 densities, and models outcome of
primary electron precipitation on this neutral background.
Requires a Fortran compiler, such as
Any Fortran compiler should work:
pip install -e .
ReesSergienkoIvanov -t 2011-03-15T12:34:56 -c 65 -148
-ospecify output file (HDF5)
-cspecify geographic lat,lon