Poster presented at the NSF Office of Cyberinfrastructure CyberBridges CAREER PI workshop. This poster discusses the computational challenges involved in the modeling of complex relativistic astrophys
2D hydrodynamical simulations of a torus with alpha viscosity and Newtonian potential. Very similar to the setup of Stone et al. 1999 (MNRAS).Each file in the dataset contains 100 DBL with snapshots o
