Abstract: A successor of <a href="http://ascl.net/1102.017">FARGO</a> (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.
Credit: Benítez Llambay, Pablo; Masset, Frédéric
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2016ApJS..223...11B; please see additional citation information here: http://fargo.in2p3.fr/Download