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, O2, N2 densities, and models outcome of
primary electron precipitation on this neutral background.
Install
Requires a Fortran compiler, such as gfortran.
Any Fortran compiler should work:
pip install -e .
Example
ReesSergienkoIvanov -t 2011-03-15T12:34:56 -c 65 -148
-ospecify output file (HDF5)-cspecify geographic lat,lon
1 maintainer
Release files for reesaurora 1.0.5
For a detailed explanation of source distributions (sdists) and built distributions (wheels), please see the package formats documentation.
Source distribution (sdist)
| File | Size | Uploaded | |
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| reesaurora-1.0.5.tar.gz | 7.8 kB | Details |
Release files / reesaurora-1.0.5.tar.gz
| Download URL | reesaurora-1.0.5.tar.gz |
|---|---|
| Size | 7.8 kB |
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