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authorhinder <hinder@4f5cb9a8-4dd8-4c2d-9bbd-173fa4467843>2013-10-09 17:56:35 +0000
committerhinder <hinder@4f5cb9a8-4dd8-4c2d-9bbd-173fa4467843>2013-10-09 17:56:35 +0000
commitcc6f1736ebf7da34c2b9b147a5196a97d6f501d4 (patch)
tree4235a588fbbb03810f7f2526fe7b264ed843f92b /param.ccl
parent13f3a1c28489d6b4e0b78df1e277073f1a42b2a7 (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.ccl1
1 files changed, 1 insertions, 0 deletions
diff --git a/param.ccl b/param.ccl
index b8ed861..85ec3d6 100644
--- a/param.ccl
+++ b/param.ccl
@@ -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"