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authorschnetter <schnetter@b2a53a04-0f4f-0410-87ed-f9f25ced00cf>2004-06-09 09:44:45 +0000
committerschnetter <schnetter@b2a53a04-0f4f-0410-87ed-f9f25ced00cf>2004-06-09 09:44:45 +0000
commit2a6ef5d0a1aa7aa1ca8c90a1d17ce3ed4abe5327 (patch)
tree110c6dfa21eda5a3de1adfadd0aead834dc1ab0c /param.ccl
parent11d2c9bd36b4085f47ec675fa34f615c7cf4e052 (diff)
Introduce a parameter that allows choosing between Taylor expansion
and interpolation to fill the 3D grid. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/TwoPunctures/trunk@13 b2a53a04-0f4f-0410-87ed-f9f25ced00cf
Diffstat (limited to 'param.ccl')
-rw-r--r--param.ccl8
1 files changed, 8 insertions, 0 deletions
diff --git a/param.ccl b/param.ccl
index ca2fc22..f1a90a6 100644
--- a/param.ccl
+++ b/param.ccl
@@ -30,6 +30,14 @@ BOOLEAN keep_u_around "Keep the variable u around after solving"
+KEYWORD grid_setup_method "How to fill the 3D grid from the spectral grid"
+{
+ "Taylor expansion" :: "use a Taylor expansion about the nearest collocation point (fast, but might be inaccurate)"
+ "interpolation" :: "interpolate using all spectral coefficients (slow)"
+} "Taylor expansion"
+
+
+
INT npoints_A "Number of coefficients in the compactified radial direction"
{
4:* :: ""