The GLobal airglOW Model, independently and easily accessed from Fortran 2003 compiler. Optionally available from Python ≥ 3.7.
A Fortran compiler is REQUIRED.
Note: This version uses meson
and ninja
as the build system, and does not rely on distutils
,
and is Python 3.12 compatible.
Note: For macOS Big Sur and above, add the following line to your environment script (~/.zshrc
if using ZSH, or the relevant shell init script):
export LIBRARY_PATH="$LIBRARY_PATH:/Library/Developer/CommandLineTools/SDKs/MacOSX.sdk/usr/lib"
Then reopen the terminal. This fixes the issue where -lSystem
fails for gfortran
. Additionally,
installation of gfortran
using homebrew
is required.
Direct installation using pip:
$ pip install glowpython
Install from source repository by:
$ git clone https://github.com/sunipkm/glowpython
$ cd glowpython && pip install .
Requires (and installs) geomagdata for timezone aware geomagnetic parameter retrieval.
Then use examples such as:
Examples/Maxwellian.py
: Maxwellian precipitation, specify Q (flux) and E0 (characteristic energy).Examples/NoPrecipitation.py
: No precipitating electrons.
These examples are also available on the command line: GlowMaxwellian
and GlowNoPrecip
.
Or, use GLOW in your own Python program by:
import glowpython as glow
iono = glow.maxwellian(time, glat, glon, Nbins, Q, Echar)
iono
is a
xarray.Dataset
containing outputs from GLOW, including:
- number densities of neutrals, ions and electrons
- Pedersen and Hall currents
- volume emission rate vs. wavelength and altitude
- precipitating flux vs. energy
- production and loss rates
- solar flux and wavelength ranges
- electron energy deposition
All available keys carry unit and description.