文档介绍：Issues with Production Grids
Tony Hey
Director of UK e-Science
Core Programme
NGS “Today”
Interfaces
Projects
e-Minerals OGSI::Lite
e-Materials
Orbital Dynamics of Galaxies
Bioinformatics (using BLAST)
GEODISE project
UKQCD Singlet meson project
Census data analysis
MIAKT project
e-HTPX project.
RealityGrid (chemistry)
Users
Leeds
Oxford
UCL
Cardiff
Southampton
Imperial
Liverpool
Sheffield
Cambridge
Edinburgh
QUB
BBSRC
CCLRC.
NGS Hardware
Compute Cluster Data Cluster
•64 dual CPU Intel GHz (1MB cache) nodes •20 dual CPU Intel GHz nodes
•2GB memory per node •4GB memory per node
•2x 120GB IDE disks (1 boot, 1 data) •2x120GB IDE disks (1 boot, 1 data)
•work •work
• M3F-PCIXD-2 • M3F-PCIXD-2
•Front end (as node) •Front end (as node)
•Disk server (as node) with 2x Infortrend •18TB Fibre SAN ( Infortrend F16F Fibre
U16U SCSI Arrays (UltraStar 146Z10 disks) Arrays (UltraStar 146Z10 disks)
•pilers •pilers
•pilers, MKL •pilers, MKL
•PBSPro •PBSPro
•TotalView Debugger •TotalView Debugger
•RedHat ES •Oracle 9i RAC
•Oracle Application server
•RedHat ES
NGS Software
RealityGrid AHM Experiment
• Measuring protein-peptide
∆∆
binding energies – Gbind
is vital for . understanding
fundamental physical
processes at play at the
molecular level, for desig