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LCLS Project Transition to Operations 14 May 2008
Handover, Endgame Operations Organization Staffing Budget Schedule Experiment Program Science Advisory Committee User access policy User Outreach User Organization, Executive Committee User Proposal Preparation Workshops Joint SSRL-LCLS User Meeting Proposal support/processing
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Transition to Operations: Commissioning
Ground rules for transfer of accelerator systems from LCLS to ASD were defined in Lab Director’s memo, 12/2006 ASD SOP for control of accelerator configuration implemented from start of commissioning Staged handover of accelerator systems to Accelerator Systems Division at start of commissioning Injector + BC-1 Commissioning: April 2007 start, November 2007 finish + Linac through Sector 30 Commissioning: January 2008 start, April 2008 finish + Beam Transport through Undulator and Beam Dump January 2009 start, July 2009 finish Safety Assessment and Readiness planning underway
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Transition to Operation: X-Rays
Near Hall start of experiment program July 2009 Far Hall detection of x-rays (CD-4) July 2010
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Transition to Operations: Civil Construction
Beneficial Occupancy through Near Hall May 2008 Beneficial Occupancy through Far Hall August 2008 Weekly planning meetings underway
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Operations Organization
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Operations Work Breakdown Structure
Project approach to planning/scoping budgeting staffing conduct of operations improvements definition and coordination of matrixed resources
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Accelerator operations budget and staffing
Presented for BES review in September 2006 $96.7M proposed for FY2009 Experiment operations budget request FY2009: $ 2M FY2010: $ 9M
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LCLS Linac Operations Budget
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Photon Operations Staffing
Details in John Arthur’s talk FY09 FY10 Long term Instrument scientists 1 4.5 24 Engineering (laser, mech, elec) 2 6 30 Development scientists 1.5 3 10 Detectors 0.5 Computer applications 5 12 Technicians 4 34 Admin 11 Totals 9 29.5 124
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Target Running Schedule – Operation Hours
2009: AMO, SXR 2010: AMO, SXR, XPP 2011: AMO, SXR, XPP, CXI 2012: AMO, SXR, XPP, CXI, XCS HED?
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Future - Beam Sharing LCLS LUSI Described in John Bozek’s talk
Described in J. Hastings’ Talk Split proportion 10% to XPP 50% xmital to far hall Same split between PCS & CXI Soft x-ray experiments will require exclusive use of beam Ability to split/share the “hard” x-ray beam with thin crystals
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LCLS Science Program LCLS Science Advisory Committee
LCLS Scientific Advisory Committee (SAC) Roger Falcone UC Berkeley, USA - Chair Massimo Altarelli European XFEL Project Phil Bucksbaum Stanford University Robert L. Byer Stanford University Hans Frauenfelder LANL Wayne Hendrickson Columbia University Tetsuya Ishikawa RIKEN Spring-8 Center Margaret Murnane University of Colorado-Boulder Francesco Sette ESRF, France Sunil Sinha UCSD Dietrich von der Linde University of Essen Justin Wark Oxford University C. Lewis Cocke Kansas State University Robert Schoenlein LBNL Philip Anfinrud NIH Geraldine Richmond University of Oregon, USA
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LCLS/LUSI Instrument Teams
SAC recommended scientific thrust areas, based on letters of intent to do LCLS science (250 signatories) Thrust areas: AMO, XPP, CXI, HED, XCS, SXR Interested scientists chose team leaders for each area, to interface with SLAC and provide input to instrument design process AMO & LUSI instrument scientists are in regular contact with AMO, XPP, CXI, and XCS team leaders Team leaders review and accept instrument physics requirement documents Workshops have brought many team members to SLAC LCLS encourages instrument team presence from “Day One” of instrument operation
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Instrument Team Leaders (LUSI)
XPP (Instrument scientist: David Fritz) K. Gaffney (SLAC, leader) D. Reis (U. of MI) T. Tschentscher (DESY) J. Larsson (Lund Inst Tech) CXI (Instrument scientist: Sebastien Boutet) J. Hajdu (SLAC + Uppsala U, leader) H. Chapman (DESY) J. Miao (UCLA) XCS (Instrument scientist: Aymeric Robert) B. Stephenson (ANL, leader) K. Ludwig (Boston U) G. Grübel, DESY
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Instrument Team Leaders (non-LUSI)
AMO (Instrument scientist: John Bozek) L. Di Mauro (Ohio State, leader) N. Berrah (Western Michigan U) SXR (Instrument scientist TBD) A. Nilsson (Stanford) W. Wurth (U Hamburg) HED (Instrument scientist TBD) R. Lee (LLNL, leader) P. Heimann (LBNL)
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LCLS User Organization Executive Committee
Elected at 2007 LCLS Users Meeting A. Barty (LLNL) R. Lee (LLNL) L. Young (ANL) First task: create charter Draft in circulation
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2008 LCLS-SSRL User Meeting
15 October – LCLS agenda 16 October – Joint SSRL-LCLS agenda 17 October – SSRL agenda Associated workshops AMO CXI SXR
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Access to LCLS Information
LCLS Web Page Proposal Submission Through LCLS web page Will go live at end of May 2008 AMO Workshop 2-3 June 2008 XPP Workshop June 2008
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Guidance for First Round of Proposals
Early ops Mature Electron energy 4.3 GeV Repetition rate 30 Hz 120 Hz Bunch length 200 fs FWHM FEL peak power 500 MW 5 GW FEL bandwidth 0.25% 0.2% Energy per pulse 0.1 mJ 2 mJ Photons/0.1%BW 3 1011 1 1013 Peak brightness 3 1030 3 1031 Average brightness 2 1019 2 1021
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Startup - LCLS User Program
Pre-Proposal Workshops /2008 Initial Call (AMO): /2008 Proposals due, 1st round: /2008 Notification to users: ~12/2008 Schedule setting: /2009
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User Access Policy Description in Jochen Schneider’s talk
DOE-BES Perspective Demonstrate science potential early in operation Rapid transit to general user access Early Productivity: Select the best science consistent with early operations Founding instrument teams General users Emphasis on efficient use of beam time
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Science Program Formulation
LCLS Science Advisory Committee Review/approve science case for instrument Review instruments’ scientific productivity LCLS Proposal Review Panel Score proposals Recommend time allocations for proposals
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Challenges for the Future
Maximum efficiency of beam time use setup in one hutch while another operates best use of split beam Staffing for instruments Early and sustained productivity
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Summary LCLS operations organization taking shape
User outreach progressing well User policy encourages and supports widespread accessibility LCLS is open for business
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End of Presentation
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