diff options
| author | jthorn <jthorn@f88db872-0e4f-0410-b76b-b9085cfa78c5> | 2003-07-07 19:31:59 +0000 |
|---|---|---|
| committer | jthorn <jthorn@f88db872-0e4f-0410-b76b-b9085cfa78c5> | 2003-07-07 19:31:59 +0000 |
| commit | 0d62911e384b04a166bdc81a1cacf4b31d6e7b6e (patch) | |
| tree | 8d4c5332d322ae0e41ce6b4a6bc2c130058d6914 /param.ccl | |
| parent | 101e5d509acfc2505178d0e7e928a324f6f810e5 (diff) | |
point to AEILocalInterp, not LocalInterp,
since we need some AEILocalInterp features that LocalInterp doesn't have
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/AHFinderDirect/trunk@1128 f88db872-0e4f-0410-b76b-b9085cfa78c5
Diffstat (limited to 'param.ccl')
| -rw-r--r-- | param.ccl | 3 |
1 files changed, 1 insertions, 2 deletions
@@ -961,8 +961,7 @@ keyword geometry_method "how do we compute the slice's geometry?" # would be even better, but in practice a ($C^1$) Hermite interpolant # works well. # In practice the default values for these parameters should work fine -# (so long as you compile with CactusBase/LocalInterp and activate that -# thorn). +# (with the AEIThorns/AEILocalInterp local interpolator). # string coordinate_system_name \ |