Hi Sam, Thanks for the extended report. I am in the middle of the iVDGL annual report, so I will look at this in detail later. Ruth is also free to comment. Thanks, Paul At 07:45 PM 6/19/02, Lee Samuel Finn wrote: >Dear Paul and Ruth: > >As Paul, Albert and I discussed last month, until iVDGL personnel are >on-board at Penn State I will be reporting once a month via e-mail on >progress and status of iVDGL activities at Penn State. This is the first >such report. > >The overall focus of activities at Penn State have been on recruiting >personnel and scoping the LIGO Data Analysis requirements on a Penn State >greenfield tier-2 center. > >On the personnel front, we have two positions we intend to have filled by >Fall 2002: these are a systems analyst level position and a postdoc level >position. The systems analyst will be the principal systems administrator >for the cluster and also support integration and operations of LDAS and >grid/globus tools at Penn State. We seek to fill this position from the >computer science community; however, the scarcity of qualified personnel at >the budgeted salary may require that we turn back to the physics community >for this position. The postdoc level position, which has been filled, will >provide the interface between the systems development work and the LIGO data >analysis community: i.e., support the porting of analysis codes to the PSU >tier 2 site, and the use of grid/globus tools by the physics data analysis >community. The postdoc offer was accepted June 1 with a start date of >October 1. > >The Penn State situation is different then other iVDGL greenfield sites, in >that there is an existing software system - LDAS - that it must support in >order to fulfill its mission of servicing LIGO data analysis. Consequently, >in consultation with the LIGO Lab, we have identified as a high priority >maintaining the same basic configuration as the LIGO Laboratory tier-2 >facilities (LIGO Hanford Observatory, LIGO Livingston Observatory, and LIGO >MIT). This configuration is discussed in the attached aide memoir, which >summarizes the outcome of discussions with Lab personnel responsible for the >design of the Lab tier-2 systems and the LDAS software system. > >Since the LIGO Lab tier-2 centers are part of the iVDGL tier-2 framework >this requirement should not be in conflict with any iVDGL facilities >requirements, which necessarily respect the existing centers at the LIGO >Labs and UWM. Indeed, this choice should minimize the FTE drain that would >be involved in implementing and supporting LDAS on yet another system >architecture. > >In putting PSU forward as a tier 2 site I teamed with Vijay Agarwala, >Director of Computing and Information Systems at Penn State, who has >extensive experience in the development, deployment and operations of >specialized computing clusters for numerically intensive computing work. >Following upon the discussions with the LIGO Lab on the basic architecture >of the LIGO Lab systems Vijay and I have settled on the purchase of a small >number of nodes that will allow us to develop experience in supporting LDAS >for production and make a few basic hardware choices for the full-sized >cluster. With this experience, and consultation with the LIGO Scientific >Collaboration Computing Committee and iVDGL Facilities Committee, we will >proceed to the development of the full cluster, which will mirror in >architecture a LIGO tier-2 center. > >The initial node purchases will include > >Eight 2.4GHz intel/1GB/36GB disk: compute part of LDAS cluster >Two 2x2.4GHz intel/2GB/36GB disk: front-end to compute part of cluster, >data-conditioning unit > >Two 2x2.4GHz intel/4GB/5x73GB disk: for testing intel solution for data >server and database server > >Two Sun 280R (dual proc packed fiber channel disk): for testing sun solution >for data server, database server > >While testing the intel solution for data and database server, we can use a >280R for the front-end to the entire system (runs globus and other external >connectivity services: everything else is behind it on a private net); while >testing the sun solution, we can use one of the intel boxes as the >front-end. > >Sun prices are currently being negotiated; intel hardware described above >has already been negotiated at $46K. > >Best, > >Sam > > >-- >Lee Samuel Finn off: 814-863-9605 >Director, Center for Gravitational Wave Physics fax: 814-863-9608 >Center for Gravitational Physics and Geometry >Professor, Departments of Physics, Astronomy and Astrophysics >The Pennsylvania State University >