Welcome to PATMO

PATMO is a flexible code aimed at modelling 1D planetary atmospheres including (photo)chemistry, molecular/eddy diffusion, and multi-frequency radiative transfer.
It is partially based on KROME, as it produces optimized problem-dependent Fortran code by using a Python pre-processor.

Getting Started

Check the Wiki (Currently maintained by Patrick and is always under construction)

Credits

PATMO is developed and mantained by Tommaso Grassi
Niels Bohr Insitute, Starplan Center, University of Copenhagen
Contributors: E.Simoncini, A.Chiavassa, J.Ramsey, N.Vaytet, A.Popovas, T.Haugbølle, S.Bovino.