ASCL Code Record
[ascl:2504.009]
SWAMPE: 2D spectral-core shallow-water exoplanet atmosphere model
SWAMPE models the dynamics of exoplanetary atmospheres; it is an intermediate-complexity, two-dimensional shallow-water general circulation model. Benchmarked for synchronously rotating hot Jupiters and sub-Neptunes, the code is modular and can be modified to model dissimilar space objects, from Brown Dwarfs to terrestrial, potentially habitable exoplanets. SWAMPE can be easily run on a personal laptop.
- Code site:
- https://github.com/kathlandgren/SWAMPE
- Used in:
- https://ui.adsabs.harvard.edu/abs/2023PSJ.....4..106L
- Described in:
- https://ui.adsabs.harvard.edu/abs/2022JOSS....7.4872L
- Bibcode:
- 2025ascl.soft04009L
Preferred citation method:
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