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Ramses is an open source code to model astrophysical systems, featuring self-gravitating, magnetised, compressible, radiative fluid flows. It is based on the Adaptive Mesh Refinement (AMR) technique on a fully-threaded graded octree. ramses is written in Fortran 90 and is making intensive use of the Message Passing Interface (MPI) library.

You can go to the user's guide in PDF here and in the WIKI here.

Check regularly the automatic test page. Visit the code web site here.

Download the code by cloning the git repository using

$ git clone https://bitbucket.org/rteyssie/ramses

This is the development branch. To get the last stable release do the following

$ git clone --branch stable_18_09 https://bitbucket.org/rteyssie/ramses

Please register also to the mailing list.

To generate idealised initial conditions of galaxies, check out the DICE code.

To generate cosmological initial conditions, check out the MUSIC code.

To visualize RAMSES data, we encourage you to use the OSYRIS or the PYNBODY codes.