Atmospheric convection plays a key role in the climate of tidally-locked terrestrial exoplanets: insights from high-resolution simulations
Denis E. Sergeev, F. Hugo Lambert, Nathan J. Mayne, Ian Boutle, James Manners, and Krisztian Kohary 2020 Astrophysical Journal, 894:84 (19pp)
Code used to process and visualise the model output. Model data are available upon request (raw data O(100 Gb)).
page/
directory is for hosting an HTML page with an interactive version of Fig. 1.
To recreate the same conda environment for running Python code, follow these steps:
- Install conda
- Git-checkout or download this repository
- (on Linux/OSX) Navigate to the repository folder and run
make env
- Activate the environment
conda activate sergeev2020
- Run the notebooks manually or use
make
shortcuts (typemake help
for help)
Notebooks for each individual figure as well as for two data tables are in the code/
directory, while the figures themselves are in the plots/
directory.
@article{SergeevEtAl2020,
archivePrefix = {arXiv},
arxivId = {2004.03007},
author = {Sergeev, Denis E. and Lambert, F. Hugo and Mayne, Nathan J. and Boutle, Ian A. and Manners, James and Kohary, Krisztian},
doi = {10.3847/1538-4357/ab8882},
eprint = {2004.03007},
issn = {1538-4357},
journal = {The Astrophysical Journal},
number = {2},
pages = {84},
publisher = {IOP Publishing},
title = {Atmospheric convection plays a key role in the climate of tidally-locked terrestrial exoplanets: insights from high-resolution simulations},
url = {https://iopscience.iop.org/article/10.3847/1538-4357/ab8882},
volume = {894},
year = {2020}
}