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author | hinder <hinder@4f5cb9a8-4dd8-4c2d-9bbd-173fa4467843> | 2013-10-09 17:56:35 +0000 |
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committer | hinder <hinder@4f5cb9a8-4dd8-4c2d-9bbd-173fa4467843> | 2013-10-09 17:56:35 +0000 |
commit | cc6f1736ebf7da34c2b9b147a5196a97d6f501d4 (patch) | |
tree | 4235a588fbbb03810f7f2526fe7b264ed843f92b /param.ccl | |
parent | 13f3a1c28489d6b4e0b78df1e277073f1a42b2a7 (diff) |
Make trapezoidal integration method available via parameter
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/Multipole/trunk@98 4f5cb9a8-4dd8-4c2d-9bbd-173fa4467843
Diffstat (limited to 'param.ccl')
-rw-r--r-- | param.ccl | 1 |
1 files changed, 1 insertions, 0 deletions
@@ -31,6 +31,7 @@ KEYWORD integration_method "How to do surface integrals" STEERABLE=always { "midpoint" :: "Midpoint rule (1st order)" "Simpson" :: "Simpson's rule (4th order) [requires even ntheta and nphi]" + "trapezoidal" :: "Trapezoidal rule (2nd order)" "DriscollHealy" :: "Driscoll & Healy (exponentially convergent) [requires even ntheta]" } "midpoint" |