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author | Erik Schnetter <schnetter@cct.lsu.edu> | 2008-04-24 23:06:11 -0500 |
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committer | Erik Schnetter <schnetter@cct.lsu.edu> | 2008-04-24 23:06:11 -0500 |
commit | 4330bf4f6dc215b02c69671a555171af3b561de5 (patch) | |
tree | b9394133f61d8414efc1a170e3c5f721771e16c6 /Carpet/CarpetWeb/index.html | |
parent | fbc10fa5eed4d7979d7c8b2dec42e87b0b83a9ec (diff) |
CarpetWeb: Update to news item
Diffstat (limited to 'Carpet/CarpetWeb/index.html')
-rw-r--r-- | Carpet/CarpetWeb/index.html | 5 |
1 files changed, 3 insertions, 2 deletions
diff --git a/Carpet/CarpetWeb/index.html b/Carpet/CarpetWeb/index.html index 51438d109..a57f7adb9 100644 --- a/Carpet/CarpetWeb/index.html +++ b/Carpet/CarpetWeb/index.html @@ -113,8 +113,9 @@ <p><b>March 29, 2008:</b> We have benchmarked McLachlan, a new BSSN-type vacuum Einstein code, using Carpet for unigrid and AMR calculations. We compare several current large machines: - Franklin (NERSC), Queen Bee (LONI), and Ranger (TACC). These - machines have different architectures and interconnects.</p> + Franklin (NERSC), Queen Bee (LONI), and Ranger (TACC). + <!-- These machines have different architectures and + interconnects.--></p> </td><td valign="top"> <p><a href="scaling-amr/results-carpet-1lev.pdf"><img |