A code for fast, massively-parallel direct numerical simulations (DNS) of canonical flows
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Updated
Jul 22, 2024 - Fortran
A code for fast, massively-parallel direct numerical simulations (DNS) of canonical flows
Program for Simulation of Turbulent Flows
Object-oriented multi-mesh version of the classic reacting turbulent multiphase flow solver
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second- /fourth-order finite-difference direct numerical simulation (DNS) solver with versatile viscous treatments
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This repository is dedicated to the individual research project by International Master's in Turbulence (IMP-Turbulence) 2019 batch.
Embedding 3D Turbulence into 1D Core-Collapse Supernovae with ML
Old version of our solver for the incompressible Navier-Stokes equations (no longer actively developed, please use the latest version of Incompact3d
Spectral code to solve a stratified Ekman boundary layer. A canonical setup to study atmospheric turbulence where the influence of the Earth rotation and the nocturnal surface cooling is included.
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