Supercomputer Breaks the $100/GFLOPS Barrier
Hank Dietz writes "At the University of Kentucky, KASY0,
a Linux cluster of 128+4 AMD Athlon XP 2600+ nodes, achieved 471 GFLOPS on 32-bit HPL. At a cost of less than $39,500, that makes it the first supercomputer to break $100/GFLOPS. It also is the new record holder for POV-Ray 3.5 render speed.
The reason this 'Beowulf' is so cost-effective is a new network architecture that achieves high performance using standard hardware: the asymmetric Sparse Flat Neighborhood Network (SFNN)." Because this was a university project, KASY0 was assembled entirely by unversity students, which while being a source of cheap labor, is also a good way to get a lot of students of involved in a great project.
How much electricity will these super computers use up?
All those wires, it looks like it takes up alot of juice.
If you use Linux, please help development of Autopac
Obviously, I don't get it. This doesn't look any different than redundant backbones or what is frequently done with VLANs. Multiple paths between hosts is what I see. How is this "new"?
I wonder which universities/institutes have larger and maybe cheaper clusters, but just don't bother with running benchmarks. I for one are sitting next next to a tiny cluster with 40 dual-cpu nodes, which is connected (GRID like) to a 340 dual-node cluster in a nearby town. Non of us high ernergy physicists bothers with running any benchmarks on our clusters, other than our own applications. I wonder how many "linux-cluster-supercomputers" are out there which would easyly make it into the top 500, but noone has ever heard of....
Cheers.
KdenLive/PIAVE - non-linear video editing
Nice machine, but this January, CITA and the astro department at the University of Toronto brought a 256 node dual Xenon system on line: "1.2 trillion floating point mathematical operations per second (Tflops) on the standard LINPACK linear algebra benchmark." Total cost: CDN$900K (including tax) (in January prices, that's $600K U.S. or $0.50USD/GFlop.) It's being used for some very cool Astro simulations...
See http://www.cita.utoronto.ca/webpages/mckenzie