Commits

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Author Commit Message Labels Comments Date
Matthew Turk
Merging from week-of-code into new_problem_types
Branches
new_problem_types
John Wise
Standalone P-GroupFinder can distiniguish star particles (just like the inline version). Fixed relative halo positioning bug in zoom-in calculations. This also caused the spin parameter to be off by a couple orders of magnitude (only in the stand-alone version -- long standing bug, but only got around to it now!)
Britton Smith
Merging conduction fixes into week-of-code.
Britton Smith
Fixed conduction units one more time, with Greg's help.
Branches
conduction
Britton Smith
Merged with week-of-code.
Branches
conduction
Britton Smith
Cleaned up conduction code a bit.
Branches
conduction
Britton Smith
Reopening conduction branch. Merged week-of-code changes into conduction branch.
Branches
conduction
Britton Smith
Merged.
Britton Smith
Fixed units in conduction routine and cleaned up a bit.
Britton Smith
Added NumberOfPythonTopGridCalls and NumberOfPythonSubcycleCalls to yt_parameter_file.
John Wise
Adding ability to read particle displacements to initialize cosmology simulations. Most useful for 2LPT initial conditions. Most done by Oliver Hahn. Use with the parameters CosmologySimulationParticleDisplacement[123]Name CosmologySimulationCalculatePositions = 1
Britton Smith
Added ability to call embedded python after top grid iterations independent of python calls made after sub-cycling. Also added WroteData to TopGridData structure so it can be placed in the yt_parameter_file dict. This allows for the possibility of running embedded python only when data has been written.
Britton Smith
Added ability to get temperature field with embedded yt. NumberOfPythonCalls now gets read and written for consistency with analsys across restarts.
John Wise
Changing some F90 notation to F77.
John Wise
These fortran routines are in F90 instead of F77. Changing to the right extension.
John Wise
Adding machine file for Trestles at SDSC/UCSD.
Brian O'Shea
updated the conduction with a possible bug fix.
Elizabeth Harper-Clark
Added a new parameter: RadiationPressureScale - to multiply the radiation pressure by a factor. To be used when only treating a stars radiation as monochromatic H ionizing but want to consider the radiation pressure from IR simplistically. Default = 1.0 (ie no change)
Elizabeth Harper-Clark
Corrections made to Turbulence Velocity normalisation. Compiles - sorry about the mess on Friday. No more Friday afternoon pushes for Libby
John Wise
compiles now. vel isn't defined. Using Vel[123]Num instead.
Elizabeth Harper-Clark
small changes to problem type 106
Elizabeth Harper-Clark
minor changes
Elizabeth Harper-Clark
Added metal density field to probelm type 106
Elizabeth Harper-Clark
Minor change to turbulence for problemtype 106
Elizabeth Harper-Clark
refining details for problem type 106
Elizabeth Harper-Clark
Altered cloud types 4 and 6 for Problem type 106
Elizabeth Harper-Clark
set pressure balence for cloud type 4 and 6 (Problem type 106) assuming mach 20 turbulence and altered BigStarFormation usage
Elizabeth Harper-Clark
merged
Elizabeth Harper-Clark
Set SimpleSource to smoothed feedback sphere after formation
Elizabeth Harper-Clark
SimpleSource star particle formation details changed, WORKS
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