diff options
| author | jthorn <jthorn@f88db872-0e4f-0410-b76b-b9085cfa78c5> | 2003-07-25 11:52:38 +0000 |
|---|---|---|
| committer | jthorn <jthorn@f88db872-0e4f-0410-b76b-b9085cfa78c5> | 2003-07-25 11:52:38 +0000 |
| commit | d05fe9cac0ba64f77a2b163949278a400c5c1dc8 (patch) | |
| tree | 22905ba51f577d7965fd5f9f4cbc8feecb5944d3 /param.ccl | |
| parent | 09bf945c4c079b3f81dc748d1974596a1de34f16 (diff) | |
add +xz quadrant (mirrored) patch system type
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/AHFinderDirect/trunk@1141 f88db872-0e4f-0410-b76b-b9085cfa78c5
Diffstat (limited to 'param.ccl')
| -rw-r--r-- | param.ccl | 3 |
1 files changed, 2 insertions, 1 deletions
@@ -740,7 +740,7 @@ real origin_z[11] "global z coordinate of patch system origin" # # The "(rotating)" patch system types are ok for evaluating Theta(h), -# but don't work yet for apparent horizon finding +# but alas they don't work yet for apparent horizon finding # (the Jacobian computation doesn't yet grok the nonlocal rotation BCs). # keyword patch_system_type[11] "what type of patch system should we use?" @@ -755,6 +755,7 @@ keyword patch_system_type[11] "what type of patch system should we use?" "+xy quadrant (rotating)" :: "90 degree periodic rotation symmetry about z axis" "+xy quadrant (mirrored)" :: "mirror symmetry across x=0 and y=0 planes" +"+xz quadrant (mirrored)" :: "mirror symmetry across x=0 and z=0 planes" "+xz quadrant (rotating)" :: \ "180 degree periodic rotation symmetry about z axis \ and mirror symmetry across z=0 plane" |