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[ascl:2306.014] AIOLOS: Planetary atmosphere accretion and escape simulations

AIOLOS solves differential equations for hydrodynamics, friction, (thermal) radiation transport and (photo)chemistry for simulating accretion onto, and hydrodynamic escape from, planetary atmospheres. The 1-D multispecies, multiphysics hydrodynamics code, written in C++, compiles in a flexible mode that runs problems with any number of input species, and can be sped up by setting the number of species at compile time, and allows the user to provide initial conditions or boundary conditions if desired. AIOLOS provides output and diagnostic files that give snapshots in time of the state of the simulation. Output files are specific to each species, and diagnostic files contain summary as well as detailed information for, for example, the radiation transport, opacities for all species, and optical cell depths per band, in addition to other information.

Code site:
https://github.com/Schulik/aiolos
Used in:
https://ui.adsabs.harvard.edu/abs/2023MNRAS.518.1761B
Described in:
https://ui.adsabs.harvard.edu/abs/2023MNRAS.523..286S
Bibcode:
2023ascl.soft06014S

Views: 893

ascl:2306.014
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