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XES Path to Close-Out

XES Path to Close-Out. Stefan Moeller – XES Manager May 14, 2009. Recent Developments. Increased scope in XES Added SXR Instrument Michael Rowen and engineers Integration and Installation Aligned XES organization and increased staffing

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XES Path to Close-Out

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  1. XES Path toClose-Out Stefan Moeller – XES Manager May 14, 2009

  2. Recent Developments Increased scope in XES Added SXR Instrument Michael Rowen and engineers Integration and Installation Aligned XES organization and increased staffing Added Jose Chan as CAM for AMO fabrication, procurement and installation Strengthened support from Eng Physics Div. Jean Charles Castagna, Michael Holmes Added Rich Atkinson as Installation Manager Added Zoe van Hoover as Safety Officer Adding Christopher Bostedt as AMO instr. scientist

  3. Updates Design completed for all systems in XES (except SXR) Procurement, fabrication phase is nearing completion Working towards installation target dates Upstream stoppers installed on time in electron beam dump ST0 tank serves as first chamber for FEL beam diagnostics

  4. XES Overview (WBS 1.6/2.6) • 2.6.5 2D X-ray Detector for CXI • Niels van Bakel, Detector Physicist • Sol Gruner Group at Cornell University • PPA Mechanical and Controls Group • 1.6.9 Mechanical Systems • Stoppers, Infrastructure, Shielding • Eric Bong, EPD • Khalid Ahmed, Rich Maggie, LCLS CF • MFD • 1.6.6 Installation • Jose Chan, CAM • Ponce Rodriguez, PCD, Cable contracts • Rich Atkinson, Installation Manager • 2.6.3 Commissioning • Hal Tompkins, XFD • 1.6.1 XES Management • Stefan Moeller • 1.6.2 Controls: • Gunther Haller, Remi Machet, Perry Anthony, PPA • Photon System Controls • Global/Instrument/DAQ • 1.6.4 Laser System in NEH • Bill White, Greg Hayes • LCLS Laser Group • 1.6.7 Atomic Physics Instrument (AMO) • Jose Chan, CAM • Jean Charles Castagna, ME • Michael Holmes, ME • Engineering Physics Div. • MFD-SLAC, LBL, LLNL, OSU • John Bozek, Instrument Scientist • 1.6.10 SXR Instrument • Michael Rowen, Physicist • Integration and Installation

  5. Status AMO AMO Instrument: In house fabrication: Assembly at MFD Goal: June 2nd ready for install in hutch 1 June testing with Controls and alignment Start Commissioning with beam July 16 User Operations starting mid September External components provided by: KB focusing system @LBL due July 16 Energy Detector @LLNL due July 7th Magnetic Bottle Spectrometer @ Ohio State University due Aug 5th

  6. Status Hutch 1 Hutch 1 utility contracts: Overhead crane installation May 15 complete PPS sliding doors approved by BIO, install by May 22th Laser sliding doors- complete by June 8th Hole drilling complete by June 8th Piping for PCW, compressed air, hutch exhaust system exhaust start install May 18 – June 8 Coordinate activities within hutch and with AMO and SXR installation Daily status from LCLS CF, MFD Weekly installation meetings

  7. Safety AMO Hazard Analysis Document finalized Review Process with Safety Oversight Committee (SOC) is nearing completion Approval of all committees planned by end of May NEH Laser SOP for hutch 1 approved Finalize in time for IRR for AMO Upcoming Dates: RSC for AMO design June 16 Radiation Physics Approval ARR for NEH July 1 Instrument Readiness Review for AMO July 14 PPS certification for NEH and recertification of FEE in July

  8. NEH Laser System • LCLS Laser Group • Bill White, Greg Hays, see talk 5/14 9AM • Tables installed in NEH 2/1/09 • Commercial laser system accepted and installed 3/30/09 • Transport to hutch is designed, commissioning 7/1/09 • SOP for hutch 1 approved • LSS near completion, ready to certify • Start commissioning in laser room June 15 • NEH Laser system available for AMO commissioning July 15 • Laser to MBES by August 15

  9. Laser transport through floor Basement Level Laser Hall AMO Hutch Sub-basement Level

  10. Cornell 2D Detector Courtesy: Niels van Bakel

  11. Cornell 2D Detector • 2D pixel array detector for CXI instrument • Collaboration with Sol Gruner Group at Cornell Univ. • LDAC Review #8 in May 7-8, 2009 • Revised plan to allow for detailed testing of prototype detector • Extended contract from May to December 2009 • On time for CXI experiments later in 2010 • Eliminated several prototype fab runs and one full lot submission due to reliable prototype chip • SLAC developed DAQ system and interfaces • SLAC designed mechanical packaging • Delivery of Final Detector at SLAC in December 2009

  12. Mechanical Design Overview Light shroud (cover removed) Cooling coil • Quadrant board • Combines signals from 16 ASIC’s • 1 FPGA/quadrant • Double detector package • 4 ASIC’s • 2 pixel array detectors Martin Nordby, Matt Swift PPA Mech. Eng.

  13. CXI Quadrant Board Interfaces Courtesy: Niels van Bakel

  14. SXR Instrument Lead by Michael Rowen Engineering group SXR is being integrated into LCLS With AMO in hutch 1 Similar designs Controls, Laser, utility contracts Safety Process Funding issues have been resolved Optical Systems are on critical path Steep ramp-up of design Adding SXR Instrument Scientist 1st call for proposals due SXR on path to be ready for beam by end of February 2010.

  15. Level 3 Milestones

  16. Other Close out dates • Installation of X-ray tunnel and FEH cable contracts • PPS, network and timing system 11/09 • Install of Tunnel and FEH stoppers 9/09 • Delivery of LBL timing system in June 09 • Installation early July • Commissioning by LBL and SLAC team • XES complete by end of 2/10

  17. Summary XES is working on schedule to complete: the AMO instrument for first science in 7/09 the SXR instrument for 2/10 the Cornell Detector for CXI 12/09 Supporting systems are on schedule XES is transitioning to LCLS Operations

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