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Facility
A number of problems of interest to theoretical researchers lie at the forefront of structure formation and evolution of the universe. The fundamental problems are computationally challenging, intrinsically three dimensional and characterized by a wide range of length scales and time scales. In order to attack such problems requiring extensive memory and/or evolutionary time requirements, TIARA provides access to computational resources using many processors on clusters, visualization servers, and software, as outlined below.
Theoretical Clusters
XL Cluster (89 nodes, 1,456 cores, 6.3TB memory) |
85 nodes |
E5-2640 v3 @ 2.60GHz x 2 |
64GB RAM |
4 nodes |
E5-2680 v3 @ 2.50GHz x 2 |
256GB RAM |
PX Cluster (27 nodes, 432 cores, 1.7TB memory) |
27 nodes |
E5-2690 @ 2.90GHz x 2 |
64GB RAM |
TC Cluster (50 nodes, 600 cores, 2.3TB memory) |
22 nodes |
X5660 @ 2.80GHz x 2 |
48GB RAM |
28 nodes |
X5670 @ 2.93GHz x 2 |
48GB RAM |
OC Cluster (32 nodes, 256 cores, 1.1TB memory) |
32 nodes |
X5560 @ 2.80GHz x 2 |
32GB RAM |
GPU Cluster |
1 nodes |
E5-2620 v4 @ 2.10GHz x 2
NVIDIA Tesla P100-SXM2 (3,584 CUDA Cores, 16GB) x 2 |
256GB RAM |
3 nodes |
E5-2603 v2 x 2
NVIDIA TITAN X (Pascal) (3,584 CUDA Cores, 12GB) x 2 |
32GB RAM |
Visualization Servers |
2 nodes |
X5675 @ 3.07GHz x 2
NVIDIA Quadro 4000 (256 CUDA Cores, 2GB) x 2 |
96GB RAM |
1 nodes |
X5450 @ 3.00GHz x 2
NVIDIA Quadro FX 4600 (128 CUDA Cores, 768MB) |
32GB ram |
Software |
IRAF, LAM-MPI, MPICH, OpenMPI, OpenMP, Intel C/Fortran Compiler, PGI, FFTW, HDF,
SuperMongo, Zeus3D, ZeusMP, pgplot, Visit, MatLab, IDL |
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Cluster Report
A monitoring system has been implemented to allow users to remotely view live or historical statistics for all nodes, such as CPU load averages or network utilization.



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