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author | schnetter <schnetter@b2a53a04-0f4f-0410-87ed-f9f25ced00cf> | 2004-06-09 09:44:45 +0000 |
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committer | schnetter <schnetter@b2a53a04-0f4f-0410-87ed-f9f25ced00cf> | 2004-06-09 09:44:45 +0000 |
commit | 2a6ef5d0a1aa7aa1ca8c90a1d17ce3ed4abe5327 (patch) | |
tree | 110c6dfa21eda5a3de1adfadd0aead834dc1ab0c /param.ccl | |
parent | 11d2c9bd36b4085f47ec675fa34f615c7cf4e052 (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.ccl | 8 |
1 files changed, 8 insertions, 0 deletions
@@ -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:* :: "" |