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Castro (Compressible Astrophysics): An adaptive mesh, astrophysical compressible (radiation-, magneto-) hydrodynamics simulation code for massively parallel CPU and GPU architectures.

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A non-subcycling AMR version of our code (in the Strang build, not the simplified SDC build) would do the following (assumes two levels for simplicity, and ignores burning for now):...

study
driver

We should use a reference count-like system to keep track of the EOS state. Anytime an operation does something that we believe breaks thermodynamic consistency, we increment the counter. If...

## PR summary This update makes the mass_fluxes array hold the full timestep's worth of mass fluxes at the end of finalize_advance. (This subtlety only matters if there were multiple...

Right now, we create a MF `fluxes` where we add the fluxes during a subcycle, eventually copying them into the flux register. The hydro routines do not operate on the...

Right now, we do the transverse correction to the conserved state + p. This way we don't need to use the EOS to get p on the interface when we...

hydro

## PR summary ## PR motivation ## PR checklist - [ ] test suite needs to be run on this PR - [ ] this PR will change answers in...

see this doc: https://amrex-codes.github.io/amrex/docs_html/GPU.html#async-arena

There is a Sphinx `. include:: ` directive to include the `yt_example.rst` page that is generated via `nbconvert` at build time. This works on a local machine, but it is...

Clang 12.x supports `-Wheader-guard` that ensure that the header guard matches the define immediate after. We caught one instance of a mismatch in Microphysics via ROCm. We should have the...

test coverage

PR #2039 turned tiling back on in the MHD solver. We previously disabled it (#289), but that was back when the solver was in Fortran and not ported to the...

hackathon
mhd