Commits

Author Commit Message Labels Comments Date
John Wise
Fixed misspelling of Kepler! from long ago.
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[svn r2588] Check in Problem Parameter files. The new one is HDMHD2DCheckOddEvenCouplingOfRiemannSolver.enzo which does exactly that.
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Ji-hoon Kim
First compilable version after adding USE_HDF4 (doing nothing yet)
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Matthew Turk
Couple more fixes, and backported the home directory makefile include
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John Wise
Changing FlaggingField back to integer from boolean.
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[svn r2587] Added DrivenTurbulence.enzo test in doc/examples/ . It illustrates how to simulate decaying hydro turbulence and also allows for fixed force pattern driving with HydroMethods 3 & 4 Hd/MHD. Also DualEnergyFormalism now works for the new solvers. ReadUnits writes out to stderr if it modifies the TimeUnits using the correct Gravitational Constant.
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Ji-hoon Kim
added some features
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Matthew Turk
Fixed the r/p stuff here to be the config vars
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John Wise
Corrected logic in which processor allocates the potential field. This if-statement was incorrectly set when I was trying to solve some memory leaks.
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[svn r2584] Added little warning that we set TimeUnits when only DensityUnits are set. Good idea, Brian!
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John Wise
We don't need this!
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[svn r2583] Fixed units to work with new solvers. Also added an option that if you only specify Length and Density Units that the TmeUnits get calcualted for you given the correct gravitational constant. usually this works well. I also documented this on the Internal Units guide on the wiki.
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John Wise
Adding Volker Springel's parallel halo finder that has been modified to read Enzo data.
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[svn r2574] Added test problem setup files in doc/examples to test the Stanford MHD module.
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John Wise
Added mpgrafic, a parallel version of the cosmological initial conditions generator, grafic.
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[svn r2572] Ok more changes to the MHD module which should now have most of the terms done right and also consider the field when comuting the timestep.
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John Wise
Fixed non-optimized version of CTP to work with the new particle handling in RebuildHierarchy.
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[svn r2571] MHD works with and without AMR. Dual Energy Formalism is not fully tested yet with the MHD. Beware. Look at MHD2DBlastWave.enzo in the doc/examples directory to test.
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Matthew Turk
Fixing my bad merge, I believe this now brings it up to date with James's version
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[svn r2569] Stanford Hydro Solvers work. With AMR/FLuxcorrection etc. Tried the ImplosionProblemTest. Should do more. Had to take out a line in Grid.h: CommunicationMehtodShouldExit which exited if NumberofProcessors==1 which leads to problem with Grid_GetProjectedBoundaryfluxes not allocating the refinedFluxes...
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Matthew Turk
Automated merge with file:///Users/matthewturk/enzo/svn-wok
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Matthew Turk
Automated merge with file:///Users/matthewturk/enzo/week-of-code
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[svn r2568] IdentifyPhysical quantities added for all the places where its needed in the MHD solver
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Matthew Turk
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[svn r2567] MUSCL Solver for Hydro work (at least on the Unigrid Sedov Problem)
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Britton Smith
Added OutputTemperature and OutputCoolingTime parameters to CoolingTest problem type parameter file.
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David Collins
Finalized OutputFromEvolveLevel.C
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[svn r2566] Corrected Identifying the correct fields for the Stanford MUSCL solvers
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jw...@red.slac.stanford.edu
bs2
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Matthew Turk
Automated merge with file:///Users/matthewturk/enzo/svn-wok
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