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Currently, when running on the GPU, the different integrators do not print out the failures. But we now have standardized error codes, which we can add to the burn_t. Then we can store these in Castro to output once we leave the GPU kernel.
In an ideal world, we'd setup a vector<burn_t> in Castro outside of the loop over the MF and then push back the burn_t of any zone that fails. Then outside of the GPU kernel, we'd loop over the vector and print out the failures.
Currently, when running on the GPU, the different integrators do not print out the failures. But we now have standardized error codes, which we can add to the
burn_t
. Then we can store these in Castro to output once we leave the GPU kernel.Some of this is discussed here:
AMReX-Astro/Microphysics#705
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