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author | bmundim <bmundim@c83d129a-5a75-4d5a-9c4d-ed3a5855bf45> | 2012-01-03 22:13:04 +0000 |
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committer | bmundim <bmundim@c83d129a-5a75-4d5a-9c4d-ed3a5855bf45> | 2012-01-03 22:13:04 +0000 |
commit | 5f7c0eab512bdded50d093a3d40f331c008c8ed4 (patch) | |
tree | 7d79a3b08197058e414ff707888f355fbc7907eb /src/make.code.defn | |
parent | 6c6dde52a11ba3b7841fdbbff4f7f3cfc120c077 (diff) |
Add a routine to calculate mag pressure/comoving field
* When Tmunu is not calculated, ie when no storage is selected,
the comoving magnetic field/magnetic pressure wasn't calculated
at all. This commit allows that now.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@310 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
Diffstat (limited to 'src/make.code.defn')
-rw-r--r-- | src/make.code.defn | 1 |
1 files changed, 1 insertions, 0 deletions
diff --git a/src/make.code.defn b/src/make.code.defn index 414313b..50cd1bb 100644 --- a/src/make.code.defn +++ b/src/make.code.defn @@ -5,6 +5,7 @@ SRCS = Utils.F90 \ GRHydro_Boundaries.F90 \ + GRHydro_CalcBcom.F90 \ GRHydro_CalcUpdate.F90 \ GRHydro_Con2Prim.F90 \ GRHydro_DivergenceClean.F90 \ |