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* GRHydro_InitData: magnetized Bondi par file.rhaas2012-11-09
| | | | | | From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@175 ac85fae7-cede-4708-beff-ae01c7fa1c26
* GRHydro_InitData: Bondi works when matter is coupled to spacetime too.rhaas2012-09-17
| | | | | | From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@170 ac85fae7-cede-4708-beff-ae01c7fa1c26
* GRHydro_InitData: par file for bondi evolution on a smoothed puncture datarhaas2012-09-17
| | | | | | From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@169 ac85fae7-cede-4708-beff-ae01c7fa1c26
* GRHydro_InitData/par/advectedloop3D_vz.par: changes to run w/storage for Tmunurhaas2012-09-17
| | | | | | From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@161 ac85fae7-cede-4708-beff-ae01c7fa1c26
* GRHydro and GRHydro_InitData: Tmunu requires storage since 454e99d6a717.rhaas2012-09-17
| | | | | | | | | | | | | Since commit 454e99d6a717433c523ec7074302fc1fc7c01dbe it is not possible to run SRMHD tests anymore without assigning storage to Tmunu. This commit change changes advectedloop3D.par to reflect that and suggests a possible solution in GRHydro/src/GRHydro_RegisterVars.cc. This solution doesn't work yet due to inadequate scheduling. A trac ticket will be filed soon to discuss this issue more broadly. From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@160 ac85fae7-cede-4708-beff-ae01c7fa1c26
* GRHydro_InitData: advectedloop3D par files: allow larger number of constr. vrbs.rhaas2012-09-17
| | | | | | From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@159 ac85fae7-cede-4708-beff-ae01c7fa1c26
* GRHydro_InitData: Fix advectedloop3D boundary map.rhaas2012-09-17
| | | | | | From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@158 ac85fae7-cede-4708-beff-ae01c7fa1c26
* * add a hot shocktube to run shocktube tests with the nuclear EOSrhaas2012-09-04
| | | | | | From: Christian Ott <cott@bethe.tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@156 ac85fae7-cede-4708-beff-ae01c7fa1c26
* high resolution advectedloop2D par files.rhaas2012-08-09
| | | | | | From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@147 ac85fae7-cede-4708-beff-ae01c7fa1c26
* update balsara par filesrhaas2012-08-09
| | | | | | From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@146 ac85fae7-cede-4708-beff-ae01c7fa1c26
* GRHydro_InitData: update balsara1_2d par files.rhaas2012-08-09
| | | | | | From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@145 ac85fae7-cede-4708-beff-ae01c7fa1c26
* GRHydro_InitData: par file for advectedloop test with v^z \= 0.rhaas2012-08-09
| | | | | | From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@144 ac85fae7-cede-4708-beff-ae01c7fa1c26
* update advectedloop2D.parrhaas2012-08-09
| | | | | | From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@143 ac85fae7-cede-4708-beff-ae01c7fa1c26
* GRHydro_InitData: adapt rotor parfile to current coderhaas2012-08-09
| | | | | | From: Roland Haas <roland.haas@physics.gatech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@141 ac85fae7-cede-4708-beff-ae01c7fa1c26
* Introduce a better treatment of the shocktube boundaries.rhaas2012-08-09
| | | | | | | | | | | | | | | | | | | | | | * The 2d diagonal boundary conditions are correctly applied when using multiprocessors. * The ymin (ymax) surfaces have their points in the region indsum < minsum (indsum > maxsum) fixed after a first sync operation. A second sync guarantees the neighbour grid receives the correct value of the boundary on those regions. * Mirror symmetries applied at the faces intercepting the upper right corner assumed cubic local domain. However, rectangular local domains are common after domain decomposition. This commit fixes the indexes applying this symmetry for these cases. * Upper right corner/edge/surface condition should use sten instead of stenp1. Thanks for catching this Josh! * Attempt at a 3d diagonal boundary treatment (Josh's commit) git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@135 ac85fae7-cede-4708-beff-ae01c7fa1c26
* Snapshot of ET GRHydro_InitData rev. 132 with a poloidal magnetic field routinerhaas2012-08-09
| | | | | | added. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@134 ac85fae7-cede-4708-beff-ae01c7fa1c26
* Magnetized diagonal shock parameter file.bmundim2011-11-02
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@132 ac85fae7-cede-4708-beff-ae01c7fa1c26
* RIT MHD dev:bmundim2011-04-27
| | | | | | | Balsara's and Komissarov's shock tube tests. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@123 ac85fae7-cede-4708-beff-ae01c7fa1c26
* Add a few parameter files for MHD testing purposes.bmundim2011-01-01
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@120 ac85fae7-cede-4708-beff-ae01c7fa1c26