The AstroBEAR Code

AstroBEAR is an Adaptive Mesh Refinement (AMR) distributed-memory parallel Eulerian code written in FORTRAN 90 which supports hydro- or magnetohydrodynamics in two or three dimensions. AstroBEAR is derived from the ​BEARCLAW AMR package written by Sorin Mitran. Users write their own project modules in AstroBEAR by specifying initial conditions and any continual processes, such as an inflow condition. There exists a variety of modules already built; users are encouraged to use these as a starting point for their own module(s).

Once a module has been written and the executable is ready to be run, users specify simulation parameters—-such as the resolution, how many levels of AMR are desired, source term physics such as radiative cooling, and so forth—-in the data files. The code is most commonly run on Beowulf-type computing clusters, though it has been successfully ported to the BlueGene/P architecture.

AstroBEAR Code Topics

• Introducing AstroBEAR 2.0

• How AstroBEAR Works

• Testing

• Troubleshooting AstroBEAR

• Development Team

• Development Procedure — Proper procedure for altering or adding new code to AstroBEAR

• Documenting AstroBEAR with Doxygen

• What is Scrambler and how does it work

• Alternate distribution algorithms — A summary of the communication/distribution systems used by other codes.

• Scaling (other codes) — A summary of scaling tests for other codes.

• Scaling on AstroBEAR — A summary of scaling tests for AstroBEAR 2.0.

• [ProjectStatistics] — A table to collect revision/module/machine information from group members

• [GoldenVersion] — Modules/Features should go to Golden Version AstroBEAR2.0

• [ProjectRuns] — Project runs for XSEDE allocation

Wiki Code Topics

Discussion relating to the AstroBEAR wiki itself may be found here: AstroWikiCode.

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