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| author | jthorn <jthorn@f88db872-0e4f-0410-b76b-b9085cfa78c5> | 2003-07-27 13:53:42 +0000 |
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| committer | jthorn <jthorn@f88db872-0e4f-0410-b76b-b9085cfa78c5> | 2003-07-27 13:53:42 +0000 |
| commit | dc62954d5bd7e17a5b032d85b8a225c969183c2e (patch) | |
| tree | 6bd0eefb65ca7157deae0e076c491da2965a9aa6 /README | |
| parent | 568744fb18e1e2fdd7453124e57c5c299251947e (diff) | |
update a few comments
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/AHFinderDirect/trunk@1148 f88db872-0e4f-0410-b76b-b9085cfa78c5
Diffstat (limited to 'README')
| -rw-r--r-- | README | 11 |
1 files changed, 6 insertions, 5 deletions
@@ -19,9 +19,10 @@ it does require an intitial guess for the apparent horizon position. Documentation ============= -The doc/ directory contains detailed documentation for this thorn. -There are also a lot of comments in the param.ccl file on how to set -the (many) parameters. +The doc/ directory contains detailed documentation for this thorn, +including a discussion of those parameters which you'll likely want +to set (or at least know about) in practice. For full information +on all the parameters, see the comments in the param.ccl file. The par/ directory contains some sample par files. @@ -98,8 +99,8 @@ grid functions which are defined in those thorns. By default this thorn uses various Cactus APIs which are supplied by other thorns: * This thorn uses CCTK_InterpGridArrays() for interpolating grid arrays. - This is supplied by a driver-specific thorn; at present PUGHInterp - it this for the PUGH driver. + This is supplied by a driver-specific thorn, such as PUGHInterp or + CarpetInterp. * This thorn uses CCTK_ReduceLocArrayToArray1D() for interprocessor communication in the multiprocessor Newton solver. [see src/driver/README.parallel for details] |