diff options
| author | knarf <knarf@b6729ddc-ac74-4bd1-908c-9dc7244c52a1> | 2010-01-12 05:11:15 +0000 |
|---|---|---|
| committer | knarf <knarf@b6729ddc-ac74-4bd1-908c-9dc7244c52a1> | 2010-01-12 05:11:15 +0000 |
| commit | 05daf480983476ac9d8fd45aed64a54f5b6d1aca (patch) | |
| tree | 795431ce9e157ef53d4731def283cbc0d6f27e40 /interface.ccl | |
| parent | 7961ed107c0f89543ac3a0bd3de7852c95a48ef4 (diff) | |
Implement primitive maximum density search ala Whisky. This should be fine most
of the time, but might break without notice if unlucky. Ideas of a safer neutron
star tracking exist, but are not implemented here.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/Hydro_Analysis/trunk@26 b6729ddc-ac74-4bd1-908c-9dc7244c52a1
Diffstat (limited to 'interface.ccl')
| -rw-r--r-- | interface.ccl | 5 |
1 files changed, 5 insertions, 0 deletions
diff --git a/interface.ccl b/interface.ccl index 53b88d0..a5b27b7 100644 --- a/interface.ccl +++ b/interface.ccl @@ -2,3 +2,8 @@ implements: Hydro_Analysis +inherits: Grid, HydroBase + +CCTK_REAL Hydro_Analysis_rho_max type = SCALAR tags='checkpoint="no"' "value of the maximum of rho" + +CCTK_REAL Hydro_Analysis_rho_max_loc[3] type = SCALAR tags='checkpoint="no"' "coordinate location of the maximum of rho" |