Finite Volume simulation of the Kelvin-Helmholtz Instability
Astrophysics MHD simulation code optimized for large cluster of GPU
Navier-Stokes-Simulations
conditional flow matching based surrogate model for KHI
Reproducible theory and numerical tools for subresolution inference from photospheric Kelvin–Helmholtz modes, including MURaM stress tests and multimode recovery.
Physics-informed neural networks for compressible Kelvin–Helmholtz spectral branches, eigenvalues and eigenmodes.
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