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[ascl:2312.011] PhotochemPy: 1-D photochemical model of rocky planet atmospheres

PhotochemPy finds the steady-state chemical composition of an atmosphere or evolves atmospheres through time. Given inputs such as the stellar UV flux and atmospheric temperature structure, the code creates a photochemical model of a planet's atmosphere. PhotochemPy is a distant fork of Atmos (ascl:2106.039). It provides a Python wrapper to Fortran source code but can also be used exclusively in Fortran.

Code site:
https://github.com/Nicholaswogan/PhotochemPy https://doi.org/10.5281/zenodo.6360737
Used in:
https://ui.adsabs.harvard.edu/abs/2022PNAS..11917933T
Bibcode:
2023ascl.soft12011W

Views: 338

ascl:2312.011
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