RAMSES was developped in Saclay to study large scale structure and galaxy formation.
It is now a rather flexible package to be used for general purpose simulations in self-gravitating fluid dynamics.
It is written in Fortran 90 with extensive use of the MPI library.
The current version is 1.0: it is a free software for non-commercial use only.
This code is a grid-based hydro solver with adaptive mesh refinement. The data structure is called a "fully threaded tree". As opposed to "patch-based AMR", cells are refined on a cell by cell basis: it is therefore called a "tree-based AMR". A very simple interface based on "Fortran namelists" can be used to specify runtime parameters. A few routines can be modified to set more complex initial or boundary conditions. The 4 main modules are:
- the AMR module with grid refinement, parallel communications and time steping.
- the hydro module with a second-order unsplit Godunov solver with various slope limiters and Riemann solvers.
- the N body module for colisionneless particles dynamics
- the Poisson module with a multigrid solver for the coarse grid and a Conjugate-Gradient solver on the fine grids.
Go to the Download Page .
RAMSES was written by Romain TEYSSIER, and is under CEA Copyright.
This software is governed by the CeCILL license under French law and abiding by the rules of distribution of free software. You can use, modify and/or redistribute the software under the terms of the CeCILL license as circulated by CEA, CNRS and INRIA (see http://www.cecill.info ).
As a counterpart to the access to the source code and rights to copy, modify and redistribute granted by the license, users are provided only with a limited warranty and the software's author, the holder of the economic rights, and the successive licensors have only limited liability. In this respect, the user's attention is drawn to the risks associated with loading, using, modifying and/or developing or reproducing the software by the user in light of its specific status of free software, that may mean that it is complicated to manipulate, and that also therefore means that it is reserved for developers and experienced professionals having in-depth IT knowledge. Users are therefore encouraged to load and test the software's suitability as regards their requirements in conditions enabling the security of their systems and/or data to be ensured and, more generally, to use and operate it in the same conditions as regards security.
The fact that you are presently reading this means that you have had knowledge of the CeCILL license and that you accept its terms.
http://irfu.cea.fr/projets/site_ramses
maj : 16-03-2010 (904)
Détection des rayonnements Simulation et traitement des données
Le Service d'Astrophysique et le Laboratoire AIM
The Astrophysics Division
![]() |
04 octobre 2010
La plus célèbre collision de galaxies décodée par des simulations 'haute résolution'
Des simulations numériques ‘haute résolution’ réalisées par des chercheurs du Service d'Astrophysique du CEA-Irfu/AIM viennent de révéler que la plus célèbre collision de galaxies, la collision des Antennes, produit beaucoup plus d'étoiles que ne le laissaient penser les observations. Lors d'une rencontre entre deux galaxies, la compression du gaz entraine l'allumage de nouvelles étoiles. Jusqu'ici, il semblait que ces ... Lire la suite » |
![]() |
Les simulations numériques dévoilent l'impact dynamique des protons sur leurs accélérateurs
Des chercheurs du Laboratoire d'Étude des Phénomènes Cosmiques de Haute Énergie et des experts en simulations numériques du groupe COAST, ont réalisé le couplage entre un code hydrodynamique 3D et un modèle d'accélération de particules, permettant pour la première fois d'étudier de façon réaliste les signatures morphologiques des protons accélérés par l'onde de choc d'un reste de ... Lire la suite » |