676882 SzGeCERN 20160212160325.0 IT-3106/AB/CLIC SUPPLY AND INSTALLATION OF HEATING, COOLING, VENTILATION AND SANITARY SERVICES FOR THE GLOBE OF INNOVATION INFRASTRUCTURE. archived E-tendering_Archives_Purchase_Egroups [CERN] SzGeCERN Supplies IT rachel.bray@cern.ch 519421 95788 http://cds.cern.ch/record/676882/files/IT3106Coverletter.pdf 519422 3160 http://cds.cern.ch/record/676882/files/IT3106Listfirmsfr.pdf 519423 3255 http://cds.cern.ch/record/676882/files/IT3106Listfirmsgb.pdf 519424 175355 http://cds.cern.ch/record/676882/files/IT3106Tender.pdf 519425 300035 http://cds.cern.ch/record/676882/files/IT3106Specification.pdf n 200342 2003-10-16 2003-11-14 65 20031203 0911 MAN01 20031016 PUBLIC 000028840MAN IT 704559 SzGeCERN 20160323123023.0 nlin.CD/0401003 eng nlin/0401003 Burghelea, T Mixing by polymers: experimental test of decay regime of mixing 2004 6 Jan 2004 mult. p By using high molecular weight fluorescent passive tracers with different diffusion coefficients and by changing the fluid velocity we study dependence of a characteristic mixing length on the Peclet number, $Pe$, which controls the mixing efficiency. The mixing length is found to be related to $Pe$ by a power law, $L_{mix}\propto Pe^{0.26\pm 0.01}$, and increases faster than expected for an unbounded chaotic flow. Role of the boundaries in the mixing length abnormal growth is clarified. The experimental findings are in a good quantitative agreement with the recent theoretical predictions. LANL EDS SzGeCERN Nonlinear Systems PREPRINT LANL EDS Chaotic Dynamics LANL EDS nlin.CD Segrè, E Steinberg, V http://documents.cern.ch/cgi-bin/setlink?base=preprint&categ=nlin.CD&id=0401003 Access to fulltext document victor.steinberg@weizmann.ac.il n 200402 10 20060128 0005 CER01 20040107 PUBLIC 002420091CER PREPRINT Hidden 865672 SzGeCERN 20251218230313.0 DOI 10.5170/CERN-2005-002.651 oai:cds.cern.ch:865672 cerncds:FULLTEXT DOI cerncds:CERN:FULLTEXT INIS cerncds:CERN eng Gallas, M CERN Quality Assurance and Testing in LCG 2005 CERN SIS CHEP04-2005 SzGeCERN Computing and Computers ARTICLE CERN YELLOWREPCONTRIB Moscicki, J CERN Aimar, A CERN Lamanna, M CERN Mancera, L CERN IT http://documents.cern.ch/cgi-bin/setlink?base=yellowarticle&categ=2005-002&id=p651 Published version from CERN http://cds.cern.ch/record/865672/files/p651.pdf Published version from CERN n 200531 a2005 13 20071117 0013 CER01 20050804 688747 651 interlaken20040927 PUBLIC 002544489CER https://repository.cern/legacy/record/865672 ARTICLE ConferencePaper MIGRATED 865715 SzGeCERN 20251218230317.0 DOI 10.5170/CERN-2005-002.826 oai:cds.cern.ch:865715 cerncds:FULLTEXT DOI cerncds:CERN:FULLTEXT INIS cerncds:CERN EGEE-PUB-2004-002 eng Laure, E CERN Middleware for the next generation Grid infrastructure 2005 CERN 2004 4 p The aim of the EGEE (Enabling Grids for E-Science in Europe) project is to create a reliable and dependable European Grid infrastructure for e-Science. The objective of the EGEE Middleware Re-engineering and Integration Research Activity is to provide robust middleware components, deployable on several platforms and operating systems, corresponding to the core Grid services for resource access, data management, information collection, authentication & authorization, resource matchmaking and brokering, and monitoring and accounting. For achieving this objective, we developed an architecture and design of the next generation Grid middleware leveraging experiences and existing components essentially from AliEn, EDG, and VDT. The architecture follows the service breakdown developed by the LCG ARDA group. Our strategy is to do as little original development as possible but rather re-engineer and harden existing Grid services. The evolution of these middleware components towards a Service Oriented Architecture (SOA) adopting existing standards (and following emerging ones) as much as possible is another major goal of our activity. CERN EDS SzGeCERN Computing and Computers CERN SOA CERN Middleware CERN Grid CERN gLite CERN EGEE EGEEPUB ARTICLE CERN YELLOWREPCONTRIB Hemmer, F CERN Prelz, F INFN, Italy Beco, S Datamat SpA, Italy Fisher, S RAL, UK Livny, M University of Wisconsin, USA Guy, L CERN Barroso, M CERN Buncic, P CERN AUTHOR|(CDS)2067003 #BEARD# Kunszt, Peter Z CERN Di Meglio, A CERN Aimar, A CERN Edlund, A KTH, Sweden Groep, D NIKHEF, The Netherlands Pacini, F Datamat SpA, Italy Sgaravatto, M INFN, Italy Mulmo, O KTH, Sweden IT http://documents.cern.ch/cgi-bin/setlink?base=egee&categ=pub&id=egee-pub-2004-002 Fulltext http://documents.cern.ch/cgi-bin/setlink?base=yellowarticle&categ=2005-002&id=p826 Published version from CERN http://cds.cern.ch/record/865715/files/p826.pdf Published version from CERN Erwin.Laure@cern.ch n 200531 a2005 13 20091126 1452 CER01 20050804 688747 826 interlaken20040927 PUBLIC 002544532CER https://repository.cern/legacy/record/865715 ARTICLE ConferencePaper MIGRATED 002606026CER01 938515 20060420 1135 CER01 20060328 002606026CER UNKNOWN DELETED 1110531 20251120203403.0 BUL-BN-2008-010 CERN Neutrinos search for sunshine in Italy! Les neutrinos du CERN vont chercher le soleil en Italie ! 18/06/2008 Wednesday, 18th June 2008. The CNGS (CERN Neutrinos to Gran Sasso) beam has re-started, shooting muon neutrinos towards Italy. The neutrino beam should run this year until mid November.The aim of CNGS is to understand the oscillation of neutrinos, for example their transformation from muon into tau neutrinos over long distances.Edda Gschwendtner, the liaison physicist of the CNGS beam, describes the progress of the project, “We did a lot of modifications this year to CNGS, which was a huge amount of work, with many groups and services involved. In parallel the OPERA detector in Italy made an enormous progress in completing their detector and we are looking forward to seeing tau neutrinos soon.” Mercredi 18 juin 2008. Le faisceau du CNGS (Neutrinos du CERN vers le Gran Sasso) a repris du service, propulsant des neutrinos du muon vers l’Italie. Cette année, le faisceau de neutrinos devrait fonctionner jusqu’à mi-novembre.Le but de CNGS est de comprendre l’oscillation des neutrinos, par exemple leur transformation de neutrinos du muon en neutrinos du tau sur de longues distances.Edda Gschwendtner, physicienne pour le faisceau du CNGS, décrit l’avancement du projet : « Cette année, nous avons apporté de nombreuses modifications à l'installation CNGS. Cela a représenté une énorme quantité de travail et a impliqué de nombreux groupes et services. Parallèlement, l’équipe du détecteur OPERA, en Italie, a réalisé d’énormes progrès et a terminé son détecteur. Nous nous réjouissons de voir bientôt des neutrinos du tau ». SzGeCERN Breaking News Breaking News: CNGS Neutrinos 06/18/2008 06/25/2008 https://repository.cern/legacy/record/1110531 BULLETINBREAKING MIGRATED