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[ascl:1509.006] FARGO3D: Hydrodynamics/magnetohydrodynamics code

A successor of FARGO (ascl:1102.017), FARGO3D is a versatile HD/MHD code that runs on clusters of CPUs or GPUs, with special emphasis on protoplanetary disks. FARGO3D offers Cartesian, cylindrical or spherical geometry; 1-, 2- or 3-dimensional calculations; and orbital advection (aka FARGO) for HD and MHD calculations. As in FARGO, a simple Runge-Kutta N-body solver may be used to describe the orbital evolution of embedded point-like objects. There is no need to know CUDA; users can develop new functions in C and have them translated to CUDA automatically to run on GPUs.

Code site:
http://fargo.in2p3.fr/
Described in:
http://adsabs.harvard.edu/abs/2016arXiv160202359B
Bibcode:
2015ascl.soft09006B

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ascl:1509.006
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