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Welcome to the AstroBEAR Wiki
AstroBEAR is a parallelized hydrodynamic/MHD simulation code suitable for a variety of astrophysical problems. Derived from the BearCLAW package written by Sorin Mitran, AstroBEAR is designed for 2D and 3D adaptive mesh refinement (AMR) simulations. Users write their own project modules by specifying initial conditions and continual processes (such as an inflow condition). In addition, AstroBEAR comes with a number of pre-built physical phenomena such as clumps and winds that can be loaded into a user module.
New Users
- Download — Instructions for downloading AstroBEAR.
- User Guide — Information on using AstroBEAR
- FAQ — Frequently asked questions about AstroBEAR
Advanced Users
- Developer Guide — The portal to information on AstroBEAR's algorithms and source code.
- Tutorials — Editing Trac pages, using Mercurial, and visualization guides.
- Debugging — Information about debugging
- Testing — Information about testing
- Development — Information about ongoing development]
Publications and External Links
- Publications using AstroBear — A list of publications using AstroBEAR
- Image Gallery — Selected images produced by AstroBEAR simulations.
- Collaborators & Projects — How AstroBEAR is currently being employed, and by whom.
- External Links and Literature — Links to some of the concepts and technologies used by AstroBEAR.
Group Members
- Member Pages — Current Member Pages.
- Teams — Group management and organization
For trouble-shooting AstroBEAR, please refer to the ticket system on the menu bar at the top of the page (accessible via Login). There, users can review past tickets and solutions, as well as post new tickets detailing novel errors. Such requests will be assigned to AstroBEAR's debugging team, and will be reposted to the ticket system with the status "closed" as they are rectified.
