| | 27 | |
| | 28 | |
| | 29 | = A few documentation things to fix = |
| | 30 | |
| | 31 | * contact us link on [AstroBearDownload Download Page] does not work if not logged in |
| | 32 | |
| | 33 | * [BuildingAstroBear Instructions] for installing AstroBEAR discuss using mercurial but don't mention where to check out the official 'repo' – which would of course only work for local folks anyways... |
| | 34 | |
| | 35 | * AstroBearStandardOut needs to be updated to describe elliptic time usage. It would be helpful to also show some common errors that are seen. |
| | 36 | |
| | 37 | * ModulesOnAstroBear |
| | 38 | * does not discuss the ProblemBeforeGlobalStep subroutine |
| | 39 | * Simulation data section should not encourage the use of numerical indices for things like px, or Energy as these will be dependent on equation of state, lMHD, nTracers, etc... |
| | 40 | * Dimensions section should be updated since 1D problems are possible |
| | 41 | * Dimensions section should also encourage the use of CellPos function to get (x,y,z from i,j,k) |
| | 42 | * Units and scaling section should not encourage the changing of physical scales |
| | 43 | * Initializing a Grid says that each infodef has a %dx which is not true |
| | 44 | * Initializing a grid has an incorrect expression for the number of ghost zones |
| | 45 | * Flagging cells for refinement implies that the errflag array extends into ghost zones – which it doesn't |
| | 46 | * AdditionalPhysics says that MaintainAuxArrays needs to be set to true which is no longer correct |
| | 47 | * Aux fields only need to be initialized if lMaintainAuxArrays is true (in 1D MHD it is false) |
| | 48 | * Also an example that shows how to calculate the location of aux field entries would be good – as well as an example showing how to initialize a divergence free auxfield using a vector potential. |
| | 49 | * It would be nice to stop storing the Cooling Objects in the chombo file – which would simplify the problem module. |
| | 50 | * Not sure if selfgravity still has a problem with a uniform density field... this should be checked – and it would only be a problem with peridiodic BC's for the potential – also a discussion (or link to a discussion) about what needs to bet set in global.data for self-gravity to work. |
| | 51 | * I believe you can have sink particles without self-gravity (ie just point gravity) |
| | 52 | |
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