Astrophysics MHD simulation code optimized for large cluster of GPU
-
Updated
Mar 7, 2023 - C++
Astrophysics MHD simulation code optimized for large cluster of GPU
Create Your Own Finite Volume Fluid Simulation (With Python) Part 2: Boundary Conditions and Source Terms
A simple finite difference scheme for the Rayleigh-Bernard equations (buoyancy driven convection).
Add a description, image, and links to the rayleigh-taylor topic page so that developers can more easily learn about it.
To associate your repository with the rayleigh-taylor topic, visit your repo's landing page and select "manage topics."