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Extreme Horizon

Extreme Horizon

Resolving galactic disks in their cosmic environment

Orion

Orion

Molecular cloud fragmentation and evolution, formation of prestellar cores

Fragdisk

Fragdisk

Fragmentation of self-gravitating disks

Synthetic disk populations

Synthetic disk populations

Resolving protoplanetary disks in massive protostellar clumps

Wind of HD189733

Wind of HD189733

Unveiling the magnetic link between stars and planets

Dusty collapses

Dusty collapses

Understanding the dynamics of dust during the protostellar collapse

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  4. ramses3

Acknowledgement

Galactica database acknowledgement

If you use it in your own work, you may acknowledge the origin of the data obtained on the Galactica database like so:

This work reused datasets available on the Galactica simulations database
(http://www.galactica-simulations.eu)
                            
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ramses3

RAMSES was developed 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. It is a free software for non-commercial use only.

This code is a grid-based hydro solver with adaptive mesh refinement. As opposed to patch-based AMR, cells are refined on a cell by cell basis: is therefore called a tree-based AMR.

A very simple interface based on Fortran namelist can be used to specify runtime parameters.

A few routines can be modified to set more complex initial or boundary conditions.

Domain decomposition in RAMSES
Examples of domain decomposition used in
RAMSES to perform parallel computing.

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