international escience infrastructure bill st. arnaud [email protected]
TRANSCRIPT
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
S2 VLBI Space Observatory
GLOBAL RING NETWORK FOR ADVANCED APPLICATIONS
DEVELOPMENT
Russia-China-USA-Korea-Canada-Netherlands Science & Education Network
GLIF links
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.
CRC (CA)
i2CAT (ES)
L1/L2 + GigE
L1/L2 + STM4GigE+L1/L2
GigE + L2
LP 1
LP4
LP3Seattle Ottawa
Chicago
CA*net 4 OC-12
L3
APAN (TH)
NCHC (TW)
KISTI (KR) LP2
Calgary
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
Global Astronomy InitiativeMauna Kea Observatories
UH 0.6 UH 0.6-m telescope 0.6m University of HawaiiUH 2.2m UH 2.2-m telescope 2.2m University of HawaiiIRTF NASA Infrared Telescope Facility 3.0m NASACFHT Canada-France-Hawaii Telescope 3.6m Canada/France/UHUKIRT United Kingdom Infrared Telescope 3.8m United KingdomKeck I W. M. Keck Observatory 10m Caltech/University of CaliforniaKeck II W. M. Keck Observatory 10m Caltech/University of CaliforniaSubaru Subaru Telescope 8.3m JapanGemini Gemini Northern Telescope 8.1m USA/UK/ Canada/Argentina/ Australia/Brazil/Chile SubmillimeterCSO Caltech Submillimeter Observatory 10.4m Caltech/NSFJCMT James Clerk Maxwell Telescope 15m UK/Canada/NetherlandsSMA Submillimeter Array 8x6m Smithsonian Astrophysical Observatory/TaiwanRadioVLBA Very Long Optical/InfraredUH 0.6m UH 0.6-m telescope 0.6m University of Hawaii UH Baseline Array 25m NRAO/AUI/NSF
Source: George McGaughlin AARnet
1. E-gun & 1. E-gun & Linear Linear AcceleratorAccelerator
3. Storage Ring3. Storage Ring4. Beamline End 4. Beamline End
StationStation
VESPERS Beamline at the Canadian Light Source
microanalysis with microanalysis with unprecedented sensitivityunprecedented sensitivity
Courtesy of CLSICourtesy of CLSI
