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| author | schnetter <schnetter@20f44201-0f4f-0410-9130-e5fc2714a787> | 2006-10-28 17:53:09 +0000 |
|---|---|---|
| committer | schnetter <schnetter@20f44201-0f4f-0410-9130-e5fc2714a787> | 2006-10-28 17:53:09 +0000 |
| commit | d0735c187c48d07e6c6fa30194a7649c07b4a4a2 (patch) | |
| tree | 96501fd04bbca8426cf0f4e7b110b218240c7c98 /test/Kerr.par | |
| parent | 98f2a11583f4947f502776b371372c384c98aa02 (diff) | |
Use information from ghost zones when applying the symmetry. This is
necessary at edges and corners with mesh refinement boundaries. This
in turn requires that grid functions be synchronised _before_ this
symmetry is applied.
git-svn-id: http://svn.cactuscode.org/arrangements/CactusNumerical/RotatingSymmetry180/trunk@39 20f44201-0f4f-0410-9130-e5fc2714a787
Diffstat (limited to 'test/Kerr.par')
0 files changed, 0 insertions, 0 deletions