π A parallelized numerical solver for magnetohydrodynamics (MHD) equations, developed using finite volume methods to simulate π jets in the interstellar medium. This code is optimized for large-scale astrophysical simulations with β‘ MPI-based parallelism, making it suitable for high-performance computing environments π₯οΈ. Perfect for exploringβ¦
β16Jan 18, 2025Updated last year
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