Circumbinary disk simulations

I simulate the gas disk of a binary star system to investigate temperature distributions and compare them to the specific physical system IRAS 16293-2422 A. I run a parallelized, static mesh refined simulation of the system using the magnetohydrodynamics code Athena++. To identify the relevant physical processes to be included in the simulation, I have adapted the original code to the specific needs. I have learned a lot about numerical solvers and mesh refinement. I run the code on the institute cluster with Slurm. The output of the simulation then has to be analysed and visualised, for which I use Python specific tools.