Castro
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Castro (Compressible Astrophysics): An adaptive mesh, astrophysical compressible (radiation-, magneto-) hydrodynamics simulation code for massively parallel CPU and GPU architectures.
In the job_info file, we report the CPU time, e.g.: ``` CPU time used since start of simulation (CPU-hours): 181.756 ``` This is just # of MPI * # of...
we need to come up with a scheme to do the ghost cell fill for the intermediate stages (which is not trivial with RK integration). we also need to address...
There are a number of changes we need to do to support 4th order in 2-d axisymmetric coords: * the transformation from cell-centers to cell-averages changes * the interpolant we...
For the diffusion to 4th order, we can just set the diffusive flux on the domain boundary to 0, due to symmetry.
The derived variables in the plotfiles are only computed to second-order accuracy. We may want to handle this via AMReX directly.
Optimal subcycling is done in Nyx, and I want to implement this as an option in Castro. This involves two steps: 1) during timestep estimation, call the Amr function which...
For plane parallel geometries, the radial sponge should only depend on the vertical direction.
We should look into adding subsonic outflow boundaries. Maybe we can adapt the code from here: https://ccse.lbl.gov/people/motheau/Manuscripts_website/2017_AIAA_CFD_Motheau.pdf
Currently in the construction of the diffusion term, we do a FillPatch on the full state. But for the predictor (with CTU) or with any MOL-based hydro, we come into...
It would be a useful diagnostic to compute and store / report the average number of RHS steps taken by the reaction network integrator each step.