[cig-commits] r14043 - seismo/3D/SPECFEM3D_SESAME/trunk/UTILS/external_mesh

[nlegoff at geodynamics.org]

Author: nlegoff
Date: 2009-02-12 01:39:30 -0800 (Thu, 12 Feb 2009)
New Revision: 14043

Modified:
   seismo/3D/SPECFEM3D_SESAME/trunk/UTILS/external_mesh/readme
Log:
updated UTILS/external_mesh/readme.

Modified: seismo/3D/SPECFEM3D_SESAME/trunk/UTILS/external_mesh/readme
===================================================================
--- seismo/3D/SPECFEM3D_SESAME/trunk/UTILS/external_mesh/readme	2009-02-11 18:56:51 UTC (rev 14042)
+++ seismo/3D/SPECFEM3D_SESAME/trunk/UTILS/external_mesh/readme	2009-02-12 09:39:30 UTC (rev 14043)
@@ -9,6 +9,7 @@
 # Those files were based on HOMO_3D_lisse_300, which is the abaqus export of a CUBIT mesh courtesy of Celine Blitz (celine.blitz<AT>univ-pau<DOT>fr) representing the EROS asteroid, and extracted using tail, head, and awk commands.
 #
 # A code named sub.f90 can be used to subdivide the mesh. It should ultimately be included in meshfem3D (see TODO list), as if the decimation is done prior to partitioning, METIS will have a hard time partioning it (NSUB in file constants.h is the number by which we decimate in all deirections).
+# Be careful with constants provided in constants_pre_meshfem3D.h, nsize and max_neighbour. There is currently no check as to whether the given mesh will be within those bounds. We should adress this issue shortly.
 #
 #
 # 2- we partition this mesh using the METIS software. pre_meshfem_asteroid_subdivide contains a stand alone program that makes the call to METIS, and extracts the faces/edges/nodes which NGLL points will fill the communication buffers. This should ultimately be done inside meshfem3D (see TODO list).