Version 49 (modified by 10 years ago) ( diff ) | ,
---|
-
AstroBEAR 2.0 Developer's Guide
- Chapter 0. Managing Code Repositories
- Chapter 1. The structure of AstroBEAR
- Chapter 2. The Adaptive Mesh Refinement Engine in AstroBEAR
- Chapter 3. Communication in AstroBEAR
- Chapter 4. Parallelism
- Chapter 5. Objects in AstroBEAR
- Chapter 6. The Hyperbolic Solvers
- Chapter 7. The Elliptic/Parabolic Solvers
- Chapter 8. Line Transfer in AstroBEAR
- Chapter 9. Source Terms in AstroBEAR
- Chapter 10. Lagrangian Particles in AstroBEAR
- Chapter 11. IO
- Chapter 12. Special Topics
- Chapter 13. Legacy documentation
AstroBEAR 2.0 Developer's Guide
Chapter 0. Managing Code Repositories
Chapter 1. The structure of AstroBEAR
Using Doxygen to view and create documentation within AstroBEAR
Chapter 2. The Adaptive Mesh Refinement Engine in AstroBEAR
Chapter 3. Communication in AstroBEAR
Chapter 4. Parallelism
Chapter 5. Objects in AstroBEAR
Chapter 6. The Hyperbolic Solvers
A brief overview of the numerical integration options in AstroBEAR How magnetic fields are handled
Information about additional dissipation mechanisms useful for higher order schemes
Chapter 7. The Elliptic/Parabolic Solvers
Chapter 8. Line Transfer in AstroBEAR
[LineTransfer How line transfer is solved in AstroBEAR
Chapter 9. Source Terms in AstroBEAR
SourceTerms The main page on how source terms are implemented in AstroBEAR (under construction)
A discussion on methods of handling (simple) cooling functions.
Chapter 10. Lagrangian Particles in AstroBEAR
Chapter 11. IO
Chapter 12. Special Topics
Chapter 13. Legacy documentation
The original doxygen-like effort. All hand crafted from the finest ones and zeroes.
Attachments (1)
-
AstroBEAR_Plan.doc
(42.5 KB
) - added by 15 years ago.
The current plan for improving AstroBEAR and the development process.
Download all attachments as: .zip
Note:
See TracWiki
for help on using the wiki.