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Open source code to model astrophysical systems, featuring self-gravitating, magnetised, compressible, radiative fluid flows.
Open source code to model astrophysical systems, featuring self-gravitating, magnetised, compressible, radiative fluid flows. Based on Adaptive Mesh Refinement (AMR) on a fully-threaded graded octree, written in Fortran 90 with intensive MPI library use.
Platforms, integrations, and language support vary by plan and region. Confirm final requirements with the vendor.
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Compliance claims are normalized from current vendor documentation and independently reviewed by SOTA2.