diff options
| author | rhaas <rhaas@ac85fae7-cede-4708-beff-ae01c7fa1c26> | 2013-07-06 18:12:15 +0000 |
|---|---|---|
| committer | rhaas <rhaas@ac85fae7-cede-4708-beff-ae01c7fa1c26> | 2013-07-06 18:12:15 +0000 |
| commit | acb151ad12413f3f0ef74476f500002f46777d79 (patch) | |
| tree | c3c13c928ab07e88edb0a5add40e444026fa5a06 /schedule.ccl | |
| parent | b8e52dfff0076cd76576ab1eecd8a0d4abdd57bf (diff) | |
GRHydro_InitData: Reschedule to make things work with multipatch. Spit out a compile-time warning since
poloidal ID B-field routine is not yet adapted to MP.
From: Christian Reisswig <reisswig@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@215 ac85fae7-cede-4708-beff-ae01c7fa1c26
Diffstat (limited to 'schedule.ccl')
| -rw-r--r-- | schedule.ccl | 6 |
1 files changed, 4 insertions, 2 deletions
diff --git a/schedule.ccl b/schedule.ccl index b0a1dbb..6d97e4a 100644 --- a/schedule.ccl +++ b/schedule.ccl @@ -270,11 +270,13 @@ SCHEDULE GRHydro_BondiM_Boundary IN HydroBase_Boundaries BEFORE HydroBase_Select if (CCTK_EQUALS(initial_Bvec, "poloidalmagfield") || CCTK_EQUALS(initial_Avec, "poloidalmagfield")) { # SCHEDULE GRHydro_PoloidalMagFieldM AT CCTK_INITIAL AFTER IN HydroBase_Initial AFTER rnsid_init AFTER TOV_Initial_Data after CCCC_StarMapper_InitialData - SCHEDULE GRHydro_PoloidalMagFieldM AT CCTK_POSTINITIAL +# SCHEDULE GRHydro_PoloidalMagFieldM AT CCTK_POSTINITIAL + SCHEDULE GRHydro_PoloidalMagFieldM AT CCTK_INITIAL AFTER HydroBase_Initial BEFORE GRHydroTransformPrimToLocalBasis { LANGUAGE: Fortran } "Set up a poloidal magnetic field. It expects the other fluid variables already to be set, as for example in the TOV solution" - SCHEDULE group HydroBase_Boundaries IN HydroBase_Initial AFTER GRHydro_PoloidalMagFieldM +# SCHEDULE group HydroBase_Boundaries IN HydroBase_Initial AFTER GRHydro_PoloidalMagFieldM + SCHEDULE group HydroBase_Boundaries IN CCTK_INITIAL AFTER GRHydro_PoloidalMagFieldM BEFORE GRHydroTransformPrimToLocalBasis { } "Call boundary conditions after magnetic field initial data setup" } |