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author | jthorn <jthorn@f88db872-0e4f-0410-b76b-b9085cfa78c5> | 2002-10-17 03:46:20 +0000 |
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committer | jthorn <jthorn@f88db872-0e4f-0410-b76b-b9085cfa78c5> | 2002-10-17 03:46:20 +0000 |
commit | 3053ef54e0b8be5923e486e454ef9324ce6e4fd7 (patch) | |
tree | 3696298f861d268db45c8512ac6bac293f114aaf /par/README | |
parent | 53c7b66d3dfa5684d867ef5576f19914d9981df1 (diff) |
demo par files
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/AHFinderDirect/trunk@839 f88db872-0e4f-0410-b76b-b9085cfa78c5
Diffstat (limited to 'par/README')
-rw-r--r-- | par/README | 16 |
1 files changed, 16 insertions, 0 deletions
diff --git a/par/README b/par/README new file mode 100644 index 0000000..0f3f353 --- /dev/null +++ b/par/README @@ -0,0 +1,16 @@ +This directory contains sample parameter files. + +Kerr.par is a good one to start with if you want a simple example +of AHFinderDirect usage. It's my standard "sanity-check" test case +for AHFinderDirect, and runs in a < 10 seconds on a laptop. It sets +up Kerr/Kerr-Schild initial data and finds the apparent horizon in +it, with the coordinate origin and initial guess offset to make this +a nontrivial test of the apparent horizon finder. + +misner-init.par is another fairly simple parameter file, which sets up +Misner initial data and then finds the apparent horizons in it. + +misner-run.par is a more complicated parameter file, which sets up the +same Misner initial data, but now time-evolves it, finding the apparent +horizons at each time step. (It also runs AHFinder every 20 time steps +for comparison.) It takes a lot of cpu and memory to run. |