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International eScience Infrastructure

International eScience Infrastructure. Bill St. Arnaud bill.st.arnaud@canarie.ca. International eScience. International large instrument facilities are the low hanging fruit for eScience Astronomy, eVLBI, high energy physics, synchrotrons, ocean observatories

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International eScience Infrastructure

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  1. International eScience Infrastructure Bill St. Arnaud bill.st.arnaud@canarie.ca

  2. International eScience • International large instrument facilities are the low hanging fruit for eScience • Astronomy, eVLBI, high energy physics, synchrotrons, ocean observatories • CERN LHC, ITER, Neptune, JIVE, SKA, LOOKING, OPtiPuter, Exoplanet Global Optical Telescope Network • Most data sets are still sent by tape

  3. S2 VLBI Space Observatory

  4. GLOBAL RING NETWORK FOR ADVANCED APPLICATIONS DEVELOPMENT Russia-China-USA-Korea-Canada-Netherlands Science & Education Network

  5. GLIF links

  6. UCLP DemonstrationsOverall Network Architecture • A local end-user will create the LightPaths between each participant to Korea via UCLP and get the HDTV stream sequentially. CA*net 4 OC-12 CRC (CA) KISTI (KR) LP 1 LP2 LP3 GigE+L1/L2 Seattle L1/L2 + STM4 Ottawa LP4 Calgary NCHC (TW) L1/L2 + GigE Chicago GigE + L2 L3 i2CAT (ES) APAN (TH)

  7. Hyugens Cassini Global Collaboration • This data was transferred to AARNet’s International GigaPoP using a dedicated GbE path provided by CeNTIE, one of Australia’s Advanced Network Program (ANP) initiatives • Transit to Pacific Wave (US) was engineered on a path of the northern 10Gbps circuit of SXTransPORT • AARNet’s was connected to a CANARIE (CA) switch and a User Controlled LightPath (UCLP) set up at 1GbE to the Joint Institution for VLBI in Europe (JIVE, NL) • The Physical path for the UCLP involved the use of CAnet4 (CA) from Pacific Wave to the ManLan (US) facility in New York; the Internet Educational Equal Access Foundation’s (IEEAF, US) trans-Atlantic capacity to the SURFnet, NL GigaPoP in Amsterdam; and one of six GbE paths from the SURFnet GigaPoP to the JIVE facility at Dwingeloo

  8. Global Astronomy InitiativeMauna Kea Observatories UH 0.6 UH 0.6-m telescope 0.6m University of Hawaii UH 2.2m UH 2.2-m telescope 2.2m University of Hawaii IRTF NASA Infrared Telescope Facility 3.0m NASA CFHT Canada-France-Hawaii Telescope 3.6m Canada/France/UH UKIRT United Kingdom Infrared Telescope 3.8m United Kingdom Keck I W. M. Keck Observatory 10m Caltech/University of California Keck II W. M. Keck Observatory 10m Caltech/University of California Subaru Subaru Telescope 8.3m Japan Gemini Gemini Northern Telescope 8.1m USA/UK/ Canada/Argentina/ Australia/Brazil/Chile Submillimeter CSO Caltech Submillimeter Observatory 10.4m Caltech/NSF JCMT James Clerk Maxwell Telescope 15m UK/Canada/Netherlands SMA Submillimeter Array 8x6m Smithsonian Astrophysical Observatory/Taiwan Radio VLBA Very Long Optical/Infrared UH 0.6m UH 0.6-m telescope 0.6m University of Hawaii UH Baseline Array 25m NRAO/AUI/NSF Source: George McGaughlin AARnet

  9. VESPERS Beamline at the Canadian Light Source 1. E-gun & Linear Accelerator • microanalysis with unprecedented sensitivity 4. Beamline End Station 3. Storage Ring Courtesy of CLSI

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