Photochem is a photochemical and climate model of planet's atmospheres. Given inputs, like the stellar UV flux, the atmospheric temperature structure, etc., this code will find the steady-state chemical composition of an atmosphere, or evolve atmospheres through time. The code also contains 1-D climate models.
conda install -c conda-forge photochem
You need a Fortran compiler (gfortran>=9.30, install instructions here) and C compiler (e.g. install with conda install -c conda-forge clang)
Create a conda environment with all dependencies
conda create -n photochem -c conda-forge python numpy scipy pyyaml numba scikit-build cython cmake ninja pip hdf5 fyppClone this Gitub repository:
git clone --depth=1 --recursive https://github.com/Nicholaswogan/photochem.gitNavigate to the root directory with a terminal, activate your new conda environment, then install with pip:
conda activate photochem
python -m pip install --no-deps --no-build-isolation .Check out the examples directory.
In the 1980s Kevin Zahnle and Jim Kasting wrote the Atmos photochemical model in Fortran 77. An updated version of this code is maintained at this link by some excellent people at NASA Goddard. In December 2020, I reworked the Atmos photochemical model in Fortran 90, and made a Python wrapper to it using numpy.f2py. This resulted in PhotochemPy. PhotochemPy has several fundamental limitations that makes it challenging to build upon. So, starting Spring 2021, I began re-writing the model in Modern Fortran (2008) which resulted in this package.
If you have questions email me: wogan@uw.edu
Funding for the development of Photochem comes from
This model was build in collaboration with
- David Catling
- Kevin Zahnle
- Mark Claire
- Sandra Bastelberger
- Shawn Domagal-Goldman
- Josh Krissansen-Totton