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Networks for HENP and ICFA SCIC Networks for HENP and ICFA SCIC Harvey B. Newman Harvey B. Newman California Institute of Technology APAN High Energy Physics.

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Presentation on theme: "Networks for HENP and ICFA SCIC Networks for HENP and ICFA SCIC Harvey B. Newman Harvey B. Newman California Institute of Technology APAN High Energy Physics."— Presentation transcript:

1 Networks for HENP and ICFA SCIC Networks for HENP and ICFA SCIC Harvey B. Newman Harvey B. Newman California Institute of Technology APAN High Energy Physics Workshop January 21, 2003 California Institute of Technology APAN High Energy Physics Workshop January 21, 2003

2 Next Generation Networks for Experiments: Goals and Needs u Providing rapid access to event samples, subsets and analyzed physics results from massive data stores è From Petabytes by 2002, ~100 Petabytes by 2007, to ~1 Exabyte by ~2012. u Providing analyzed results with rapid turnaround, by coordinating and managing the large but LIMITED computing, data handling and NETWORK resources effectively u Enabling rapid access to the data and the collaboration è Across an ensemble of networks of varying capability u Advanced integrated applications, such as Data Grids, rely on seamless operation of our LANs and WANs è With reliable, monitored, quantifiable high performance Large data samples explored and analyzed by thousands of globally dispersed scientists, in hundreds of teams

3 Four LHC Experiments: The Petabyte to Exabyte Challenge ATLAS, CMS, ALICE, LHCB Higgs + New particles; Quark-Gluon Plasma; CP Violation Data stored ~40 Petabytes/Year and UP; CPU 0.30 Petaflops and UP Data stored ~40 Petabytes/Year and UP; CPU 0.30 Petaflops and UP 0.1 to 1 Exabyte (1 EB = 10 18 Bytes) (2007) (~2012 ?) for the LHC Experiments 0.1 to 1 Exabyte (1 EB = 10 18 Bytes) (2007) (~2012 ?) for the LHC Experiments

4 LHC Data Grid Hierarchy Tier 1 Tier2 Center Online System CERN 700k SI95 ~1 PB Disk; Tape Robot FNAL IN2P3 Center INFN Center RAL Center Institute Institute ~0.25TIPS Workstations ~100-400 MBytes/sec 2.5 Gbps 0.1 to 10 Gbps Tens of Petabytes by 2007-8. An Exabyte within ~5 Years later. Physics data cache ~PByte/sec ~2.5 Gbps Tier2 Center ~2.5 Gbps Tier 0 +1 Tier 3 Tier 4 Tier2 Center Tier 2 Experiment CERN/Outside Resource Ratio ~1:2 Tier0/(  Tier1)/(  Tier2) ~1:1:1

5 ICFA and Global Networks for HENP uNational and International Networks, with sufficient (rapidly increasing) capacity and capability, are essential for èThe daily conduct of collaborative work in both experiment and theory èDetector development & construction on a global scale; Data analysis involving physicists from all world regions èThe formation of worldwide collaborations èThe conception, design and implementation of next generation facilities as “global networks” u“Collaborations on this scale would never have been attempted, if they could not rely on excellent networks”

6 ICFA and International Networking uICFA Statement on Communications in Int’l HEP Collaborations of October 17, 1996 See “ICFA urges that all countries and institutions wishing to participate even more effectively and fully in international HEP Collaborations should:  Review their operating methods to ensure they are fully adapted to remote participation  Strive to provide the necessary communications facilities and adequate international bandwidth”

7 ICFA Network Task Force: 1998 Bandwidth Requirements Projection (Mbps) 100–1000 X Bandwidth Increase Foreseen for 1998-2005 See the ICFA-NTF Requirements Report: NTF

8 ICFA Standing Committee on Interregional Connectivity (SCIC) uCreated by ICFA in July 1998 in Vancouver ; Following ICFA-NTF uCHARGE: Make recommendations to ICFA concerning the connectivity between the Americas, Asia and Europe (and network requirements of HENP) èAs part of the process of developing these recommendations, the committee should  Monitor traffic  Keep track of technology developments  Periodically review forecasts of future bandwidth needs, and  Provide early warning of potential problems uCreate subcommittees when necessary to meet the charge uThe chair of the committee should report to ICFA once per year, at its joint meeting with laboratory directors (Feb. 2003) uRepresentatives: Major labs, ECFA, ACFA, NA Users, S. America

9 ICFA-SCIC Core Membership u Representatives from major HEP laboratories: W. Von Reuden(CERN) Volker Guelzow (DESY) Vicky White(FNAL) Yukio Karita (KEK) Richard Mount (SLAC) u User Representatives Richard Hughes-Jones (UK) Harvey Newman(USA) Dean Karlen (Canada) u For Russia: Slava Ilyin (MSU) u ECFA representatives: Denis Linglin (IN2P3, Lyon) Frederico Ruggieri (INFN Frascati) u ACFA representatives: Rongsheng Xu (IHEP Beijing) H. Park, D. Son (Kyungpook Nat’l University) u For South America: Sergio F. Novaes (University of Sao Paulo)

10 SCIC Sub-Committees Web Page u Monitoring: Les Cottrell ( With Richard Hughes-Jones (Manchester), Sergio Novaes (Sao Paolo); Sergei Berezhnev (RUHEP), Fukuko Yuasa (KEK), Daniel Davids (CERN), Sylvain Ravot (Caltech), Shawn McKee (Michigan) u Advanced Technologies: Richard Hughes-Jones, With Vladimir Korenkov (JINR, Dubna), Olivier Martin(CERN), Harvey Newman u The Digital Divide: Alberto Santoro (Rio, Brazil) è With Slava Ilyin, Yukio Karita, David O. Williams è Also Dongchul Son (Korea), Hafeez Hoorani (Pakistan), Sunanda Banerjee (India), Vicky White (FNAL) u Key Requirements: Harvey Newman è Also Charlie Young (SLAC)

11 Transatlantic Net WG (HN, L. Price) Bandwidth Requirements [*] u [*] BW Requirements Increasing Faster Than Moore’s Law See

12 History – One large Research Site Current Traffic ~400 Mbps; ESNet Limitation Projections: 0.5 to 24 Tbps by ~2012 Much of the Traffic: SLAC IN2P3/RAL/INFN; via ESnet+France; Abilene+CERN

13 Tier0-Tier1 Link Requirements Estimate: for Hoffmann Report 2001 1)Tier1  Tier0 Data Flow for Analysis0.5 - 1.0 Gbps 2)Tier2  Tier0 Data Flow for Analysis0.2 - 0.5 Gbps 3)Interactive Collaborative Sessions (30 Peak) 0.1 - 0.3 Gbps 4)Remote Interactive Sessions (30 Flows Peak) 0.1 - 0.2 Gbps 5)Individual (Tier3 or Tier4) data transfers 0.8 Gbps Limit to 10 Flows of 5 Mbytes/sec each uTOTAL Per Tier0 - Tier1 Link1.7 - 2.8 Gbps NOTE: è Adopted by the LHC Experiments; given in the upcoming Hoffmann Steering Committee Report: “1.5 - 3 Gbps per experiment” è Corresponds to ~10 Gbps Baseline BW Installed on US-CERN Link è Hoffmann Panel also discussed the effects of higher bandwidths ­ For example all-optical 10 Gbps Ethernet across WANs

14 Tier0-Tier1 BW Requirements Estimate: for Hoffmann Report 2001 u Does Not Include the more recent ATLAS Data Estimates è 270 Hz at 10 33 Instead of 100Hz è 400 Hz at 10 34 Instead of 100Hz è 2 MB/Event Instead of 1 MB/Event u Does Not Allow Fast Download to Tier3+4 of “Small” Object Collections è Example: Download 10 7 Events of AODs (10 4 Bytes)  100 Gbytes; At 5 Mbytes/sec per person (above) that’s 6 Hours ! u This is a still a rough, bottoms-up, static, and hence Conservative Model. è A Dynamic distributed DB or “Grid” system with Caching, Co-scheduling, and Pre-Emptive data movement may well require greater bandwidth è Does Not Include “Virtual Data” operations: Derived Data Copies; Data-description overheads è Further MONARC Computing Model Studies are Needed

15 ICFA SCIC Meetings[*] and Topics u Focus on the Digital Divide This Year è Identification of problem areas; work on ways to improve u Network Status and Upgrade Plans in Each Country è Performance (Throughput) Evolution in Each Country, and Transatlantic u Performance Monitoring World-Overview (Les Cottrell, IEPM Project) u Specific Technical Topics (Examples): è Bulk transfer, New Protocols; Collaborative Systems, VOIP u Preparation of Reports to ICFA (Lab Directors’ Meetings) è Last Report: World Network Status and Outlook - Feb. 2002 è Next Report: Digital Divide, + Monitoring, Advanced Technologies; Requirements Evolution – Feb. 2003 [*] Seven Meetings in 2002; at KEK In December 13.

16 Network Progress in 2002 and Issues for Major Experiments u Backbones & major links advancing rapidly to 10 Gbps range è “Gbps” end-to-end throughput data flows have been tested; will be in production soon (in 12 to 18 Months) è Transition to Multi-wavelengths 1-3 yrs. in the “most favored” regions u Network advances are changing the view of the net’s roles è Likely to have a profound impact on the experiments’ Computing Models, and bandwidth requirements è More dynamic view: GByte to TByte data transactions; dynamic path provisioning u Net R&D Driven by Advanced integrated applications, such as Data Grids, that rely on seamless LAN and WAN operation è With reliable, quantifiable (monitored), high performance Ü All of the above will further open the Digital Divide chasm. We need to take action

17 ICFA SCIC: R&E Backbone and International Link Progress uGEANT Pan-European Backbone ( èNow interconnects >31 countries; many trunks 2.5 and 10 Gbps uUK: SuperJANET Core at 10 Gbps è2.5 Gbps NY-London, with 622 Mbps to ESnet and Abilene uFrance (IN2P3): 2.5 Gbps RENATER backbone from October 2002 èLyon-CERN Link Upgraded to 1 Gbps Ethernet èProposal for dark fiber to CERN by end 2003 uSuperSINET (Japan): 10 Gbps IP and 10 Gbps Wavelength Core èTokyo to NY Links: 2 X 2.5 Gbps started; Peer with ESNet by Feb. uCA*net4 (Canada): Interconnect customer-owned dark fiber nets across Canada at 10 Gbps, started July 2002 è“Lambda-Grids” by ~2004-5 uGWIN (Germany): 2.5 Gbps Core; Connect to US at 2 X 2.5 Gbps; Support for SILK Project: Satellite links to FSU Republics uRussia: 155 Mbps Links to Moscow (Typ. 30-45 Mbps for Science) è Moscow-Starlight Link to 155 Mbps (US NSF + Russia Support) è Moscow-GEANT and Moscow-Stockholm Links 155 Mbps

18 R&E Backbone and Int’l Link Progress uAbilene (Internet2) Upgrade from 2.5 to 10 Gbps in 2002 èEncourage high throughput use for targeted applications; FAST uESNET: Upgrade: to 10 Gbps “As Soon as Possible” uUS-CERN èto 622 Mbps in August; Move to STARLIGHT è2.5G Research Triangle from 8/02; STARLIGHT-CERN-NL; to 10G in 2003. [10Gbps SNV-Starlight Link Loan from Level(3) uSLAC + IN2P3 (BaBar) èTypically ~400 Mbps throughput on US-CERN, Renater links è600 Mbps Throughput is BaBar Target for Early 2003 (with ESnet and Upgrade) uFNAL: ESnet Link Upgraded to 622 Mbps èPlans for dark fiber to STARLIGHT, proceeding uNY-Amsterdam Donation from Tyco, September 2002: Arranged by IEEAF: 622 Gbps+10 Gbps Research Wavelength uUS National Light Rail Proceeding; Startup Expected this Year


20 > 200 Primary Participants All 50 States, D.C. and Puerto Rico 75 Partner Corporations and Non-Profits 23 State Research and Education Nets 15 “GigaPoPs” Support 70% of Members 2.5  10 Gbps Backbone

21 2003: OC192 and OC48 Links Coming Into Service; Need to Consider Links to US HENP Labs

22 National R&E Network Example Germany: DFN Transatlantic Connectivity 2002 STM 4 STM 16 Virtual SILK Highway Project (from 11/01): NATO ($ 2.5 M) and Partners ($ 1.1M) è Satellite Links to South Caucasus and Central Asia (8 Countries) èIn 2001-2 (pre-SILK) BW 64-512 kbps èProposed VSAT to get 10-50 X BW for same cost èSee [*] Partners: CISCO, DESY. GEANT, UNDP, US State Dept., Worldbank, UC London, Univ. Groenigen u 2 X OC48: NY-Hamburg and NY-Frankfurt u Direct Peering to Abilene (US) and Canarie (Canada) uUCAID said to be adding another 2 OC48’s; in a Proposed Global Terabit Research Network (GTRN)

23 National Research Networks in Japan SuperSINET è Started operation January 4, 2002 è Support for 5 important areas: HEP, Genetics, Nano-Technology, Space/Astronomy, GRIDs è Provides 10 ’s:  10 Gbps IP connection  Direct intersite GbE links  9 Universities Connected January 2003: Two TransPacific 2.5 Gbps Wavelengths (to NY); Japan-US-CERN Grid Testbed Soon Tokyo Osaka Nagoya Internet Osaka U Kyoto U ICR Kyoto-U Nagoya U NIFS NIG KEK Tohoku U IMS U-Tokyo NAO U Tokyo NII Hitot. NII Chiba IP WDM path IP router OXC ISAS

24 SuperSINET Updated Map: October 2002

25 APAN Links in Southeast Asia January 15, 2003

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