PDF-SLAC Scientific Computing Services
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Yemi AdesanyaOctober 2016v 302About Yemi AdesanyaIn my previous life CERN fellow and technical student18years at SLACBaBar computingObjectOriented frameworks for
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SLAC Scientific Computing Services: Transcript
Yemi AdesanyaOctober 2016v 302About Yemi AdesanyaIn my previous life CERN fellow and technical student18years at SLACBaBar computingObjectOriented frameworks for data analysis C JavaMonitoring and vi. Uni processor computing can be called centralized computing brPage 3br mainframe computer workstation network host network link terminal centralized computing distributed computing A distributed system is a collection of independent computers interc Les Cottrell . – SLAC. University of . Helwan. / Egypt, Sept 18 – Oct 3, 2010. www.slac.stanford.edu/grp/scs/net/talk10/internet-measure.pptx. 2. Overview. Why is measurement important?. LAN . vs. WP1: . microwave-based accelerators. Progress towards a new standard X-band high-power flange. G. Riddone. , 08.07.2009 . (contribution . from C. . Garion). Outline. General requirements. Recall of existing design from SLAC. accelerators beyond 100 MV/m. Eric R. Colby*. Acting Head of Accelerator Research Division. December 14, 2011. * ecolby@slac.stanford.edu. Outline. Advances in RF concepts. Novel Acceleration Concepts. Building Manager . . Mark Wise (408) 981-7114. . mdwise@slac.stanford.edu. Project Manager Chandler Eason (650-455-4410). . ceason@slac.stanford.edu. Construction Manager Shane Wells (650-922-6932). The beginning. In 1975/6 . Sharon . Traweek. . and Henry . Abarbanel. encouraged me to be in contact with several Japanese groups who might be interested in collaborating on strong interaction spectroscopy studies. This led to a meeting with . Heinz-Dieter Nuhn – . LCLS Undulator Group Leader. Presented at. Monday, March 5, 2012. Project Motivation. Flexible polarization control. Support for large taper ranges required for TW FELs and high SXR output. Name and date: Arial 16 regular. Subheadline. : 42 pt. Arial. 2. SLAC National Accelerator Laboratory. Our mission:. Grow into a premier photon science laboratory. Maintain our position as the premier accelerator laboratory. Outline. Introduction. Key progress. Initial cooling. 6D cooling (VCC and HCC). Final cooling. Current and future activities. Bright . muon. sources. MICE data integration. Session agenda. December 4, 2014. Kathleen R. Geyer. August 12, 2010. Mentor: Dennis . Nordlund. SULI Presentation. August 12, 2010. Kathleen Geyer. geyer@slac.stanford.edu. UHV End Station. Soft X-rays: 0.12 to . . 12 . KeV. PES, XAS, and XES. luminosity . 2 x10. 33 . . t. < 20 . ps. (<2 year ) . Stage II: 10. 34 . . t. < 10 . ps. (<4 years). Compare z-vertex position measured with silicon tracking (. z=50. m. Yemi Adesanya. October 2016. v. 3.0. 2. About Yemi Adesanya…... In my previous life: CERN fellow and technical . student. 1. 8. . years at SLAC. BaBar computing. Object-Oriented frameworks for data analysis (C++, Java). Mauro Pivi, SLAC National Accelerator Laboratory. on behalf of ESTB/ESA team. ARD Status Meeting, SLAC. April 14, 2011. SLAC End Station A Test Beam (ESTB). ESTB will be a unique HEP resource. - . World’s only high-energy primary electron beam for large scale Linear Collider MDI and beam instrumentation studies. JuI2(1)whereCq=3:8310 13m,\rdenotesrelativisticfactor,I2andI5radiationintegralslistedbelow.I2[m 1]=1 21 2yds(2)I5[m 1]=Hu 3ds(3)whereHuuD02u+2uDuD0u\ruD2udependsonthebendingandfocusingstructu
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