James B. Murphy, Director BES Scientific User Facilities Division

Slides:



Advertisements
Similar presentations
Ultimate Storage Rings PEP-X and SPring-8 II R. Hettel for the PEP-X design team and T. Watanabe et al., SPring-8 FLS 2012 JNAL March 7, 2012.
Advertisements

Ultrafast Experiments Hao Hu The University of Tennessee Department of Physics and Astronomy, Knoxville Course: Advanced Solid State Physics II (Spring.
Superconducting Particle Accelerator Forum of the Americas December 11, 2013 Dr. Patricia M. Dehmer Acting Director, Office of Science, U.S. Department.
SPEAR3 short pulse development J. Safranek for the SSRL accelerator physics group* Outline: Timing mode fill patterns Short bunches –Low alpha Bunch length.
Soft X-ray light sources Light Sources Ulrike Frühling Bad Honnef 2014.
Briefing for SEAB 20 June 2014 Patricia M. Dehmer Acting Director, Office of Science U.S. Department of Energy.
Research Opportunities at LCLS September 2011 Joachim Stöhr.
1 Enhancements to the Linac Coherent Light Source.
Does the short pulse mode need energy recovery? Rep. rateBeam 5GeV 100MHz 500MWAbsolutely 10MHz 50MW Maybe 1MHz 5MW 100kHz.
Sept. 18, 2008SLUO 2008 Annual Meeting Vision for SLAC Science Persis S. Drell Director SLAC.
The BESSY Soft X-Ray SASE FEL (Free Electron Laser)
Synchrotron Radiation Science at SLAC Joachim Stohr, SSRL Deputy Director July 6, 2004.
February 19, 2008 FACET Review 1 Lab Overview and Future Onsite Facilities Persis S. Drell DirectorSLAC.
Office of Science U.S. Department of Energy U.S. Department of Energy’s Office of Science Dr. Raymond L. Orbach Under Secretary for Science U.S. Department.
UCLA The X-ray Free-electron Laser: Exploring Matter at the angstrom- femtosecond Space and Time Scales C. Pellegrini UCLA/SLAC 2C. Pellegrini, August.
Slide 1 George R. Neil Associate Director Jefferson Lab Jefferson Avenue Newport News, Virginia VUV Program Directors Review Plans for a VUV.
Birth of the X-Ray Laser and a New Era of Science Joachim Stohr
Status of LCLS A. Brachmann, SLAC National Accelerator Laboratory.
Thomas Jefferson National Accelerator Facility J. Michael Klopf Jefferson Lab - Free Electron Laser Division Outline of the proposed JLAMP VUV/soft X-ray.
Electromagnetic radiation sources based on relativistic electron and ion beams E.G.Bessonov 1.Introduction 2.Spontaneous and stimulated emission of electromagnetic.
Diamond and the UK new light source Chris Christou, X-band workshop, Cockcroft Institute, 1 st December 2008.
1 Energy recovery linacs Sverker Werin MAX-lab 8 July 2003.
Kwang-Je Kim ANL & U of C& POSTECH Workshop on Sciences Outlook and R&D Issues of X-ray FEL Oscillator February 14-15, 2013 POSCO International Center.
Progress at the XFELs in Europe and Japan Hans-H. Braun, PSI 48 th ICFA Advanced Beam Dynamics Workshop on Future Light Sources March 1-5, 2010 SLAC National.
Photon Diagnostic Station For TAC IR-FEL Test Facility ILHAN TAPAN* *on behalf of the TAC collaboration Uludag Universitesi, Bursa,16059, TURKEY References.
Low Emittance RF Gun Developments for PAL-XFEL
Alvaro Sanchez Gonzalez Prof. Jon Marangos Prof. Jim Clarke
A. Doyuran, L. DiMauro, W. Graves, R. Heese, E. D. Johnson, S. Krinsky, H. Loos, J.B. Murphy, G. Rakowsky, J. Rose, T. Shaftan, B. Sheehy, Y. Shen, J.
FLASH Operation at DESY From a Test Accelerator to a User Facility Michael Bieler FLASH Operation at DESY WAO2012, SLAC, Aug. 8, 2012.
Transverse Profiling of an Intense FEL X-Ray Beam Using a Probe Electron Beam Patrick Krejcik SLAC National Accelerator Laboratory.
The Future of Photon Science and Free-Electron Lasers Ingolf Lindau Lund University and Stanford University MAX-Lab and Synchrotron Light Research KTH,
W.S. Graves ASAC Review Sept 18-19, 2003 R&D at Bates William S. Graves MIT-Bates Laboratory Presentation to MIT X-ray laser Accelerator Science Advisory.
Optimization of Compact X-ray Free-electron Lasers Sven Reiche May 27 th 2011.
Brief Introduction to (VUV/)Soft X-ray FELs R. P. Walker Diamond Light Source, UK ICFA Workshop on Future Light Sources March 5 th -9 th, 2012 Thomas Jefferson.
1 BROOKHAVEN SCIENCE ASSOCIATES NSLS-II Overview Satoshi Ozaki Director, Accelerator Systems Division NSLS-II Project March 27, 2007.
Compact X-ray & Emittance Measurement by Laser Compton Scattering Zhi Zhao Jan. 31, 2014.
Max Cornacchia, SLAC LCLS Project Overview BESAC, Feb , 2001 LCLS Project Overview What is the LCLS ? Transition from 3 rd generation light sources.
Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory LCLS Scientific Program X-Ray Laser Physics:
Workshop Overview, Charge and Deliverables Joachim Stöhr.
James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys.
Electron Sources for ERLs – Requirements and First Ideas Andrew Burrill FLS 2012 “The workshop is intended to discuss technologies appropriate for a next.
DESY Deutsches Electron Synchrotron Shima Bayesteh.
The Next Generation Light Source Test Facility at Daresbury Jim Clarke ASTeC, STFC Daresbury Laboratory Ultra Bright Electron Sources Workshop, Daresbury,
ERL Status and Plans at Jefferson Lab Stephen V. Benson, On behalf of the Jefferson Lab FEL team Current status Next Generation Soft X-ray Sources JLab.
UCLA Claudio Pellegrini UCLA Department of Physics and Astronomy X-ray Free-electron Lasers Ultra-fast Dynamic Imaging of Matter II Ischia, Italy, 4/30-5/3/
김 귀년 CHEP, KNU Accelerator Activities in Korea for ILC.
J. Corlett. June 16, 2006 A Future Light Source for LBNL Facility Vision and R&D plan John Corlett ALS Scientific Advisory Committee Meeting June 16, 2006.
T. Atkinson*, A. Matveenko, A. Bondarenko, Y. Petenev Helmholtz-Zentrum Berlin für Materialien und Energie The Femto-Science Factory: A Multi-turn ERL.
Highlights of science of USR Yuhui Dong BSRF, IHEP, CAS 2012/10/29.
, Summary of Working Group 1 Linear Colliders and Light Sources C. Christou, M. Dehler.
G. Penn SLAC 25 September 2013 Comments on LCLS-IISC Design.
Temporal overlapping for HHG- seeded EUV-FEL operation by using EOS-based timing-drift controlling system H. Tomizawa 1,4 *, S. Matsubara 1, T. Togashi.
LCLS 2009 NSLS-II 2015 APS 1995 BES Light & Neutron Sources SPEAR ALS 1993 HFIR 2008 SNS
X-Ray Free-Electron Laser Amplifiers and Oscillators for Materials and Fundamental Research Kwang-Je Kim ANL and U. of Chicago ICABU Meeting November 12,
1 NGLS Outline and Needs in Superconducting RF Materials Development John Corlett SRFMW, July 16, 2012 Office of Science.
Paper: Acoustic Injectors for Drop-On-Demand Serial
MSc-Student Activities at the European XFEL
Beam dynamics for an X-band LINAC driving a 1 keV FEL
Status and Interest of the X-ray FEL SINAP
Introduction to Synchrotron Radiation
Biology at Advanced Laser Light Sources
Two color FEL experiment
ERL working modes Georg Hoffstaetter, Professor Cornell University / CLASSE / SRF group & ERL effort High Current mode High Coherence mode High Buch charge.
ERL accelerator review. Parameters for a Compton source
TW FEL “Death-Ray“ Studies
WBS 5.0 LCLS Strategic Projects Division
Jim Clarke ASTeC Daresbury Laboratory March 2006
LCLS History and Science Overview Keith Hodgson, SSRL Director April 23, 2002 LCLS DOE Review, April 23, 2002 Keith Hodgson, SSRL.
Brief Introduction to (VUV/)Soft X-ray FELs
Introduction to Free Electron Lasers Zhirong Huang
Presentation transcript:

James B. Murphy, Director BES Scientific User Facilities Division Status of International Light Sources: Today and in the Near Future presented to the BESAC Meeting 25 July 2013 Persis S. Drell SLAC/Stanford James B. Murphy, Director BES Scientific User Facilities Division

Light Sources: ERL, FEL & Storage Ring approx. 500m Spontaneous Emission FEL Stimulated Emission

What Do We Care Most About in Light* Sources? Wavelength Range Determines the kind science you can access—atomic or electronic structure and dynamics Brightness: Average and Peak Determines sensitivity of measurements Pulse Width fs pulses opens the window on ultrafast dynamics and ‘probe before destroy’ technology Coherence Allows new techniques (e.g. coherent imaging) Leads to high brightness of the beams; transform limited pulses are possible Stability Source stability in energy, position, time, intensity Number of Undulators/Beamlines/Endstations Determines the number of users in parallel that can be accommodated and ultimately how much science gets delivered * For this presentation focus on 100 eV – 100 keV sources

Light Source Pulse Structures Burst Mode Pulsed CW

X-Ray Light Source Comparison Parameter Storage Rings FEL ERL Wavelength Range + Peak Brightness ~ Pulse Structure CW Pulsed/Burst CW in future fs Pulse Width Coherence Stability Number of Beamlines

What is the Science? Science Goals will drive technology decisions. What is the science we want to target? Electron dynamics? Atomic scale imaging? Structure vs Dynamics? To achieve science goals, more than x-ray sources will be needed Pumps: Lasers, THz, etc…. Technology: Optics, Detectors, …. Other infrastructure for science Bottom line focus must be on science delivery! But the focus of this talk is status of the light source tools we have to do the science

BES Light Sources & Key Worldwide Competitors Circa 2013 NSLS-I,II SSRL MAX IV SIRIUS APS,U PETRA III SPRING8,U ESRF,U PSI SLS LCLS-I,II XFEL PAL XFEL SACLA XFEL SWISSFEL FLASH-I,II ALS Storage Rings in Blue FELs in Red There are many more UV/X-ray rings, IR/UV FELs & a few ERLs

How do Storage Rings and FELs Compare Today? Parameter Storage Rings X-ray FEL Wavelength Range 2-3+ decades typically 1+ decades (multiple undulators) Peak Brightness (ph/s/mr2/mm2/0.1%BW) 1022 – 1024 1031 – 1033 (109 times higher than SR) Average Brightness (ph/s/mr2/mm2/0.1%BW) 1019– 1021 1020– 1022 Minimum Pulse Width (fs) ~10,000 ~5 Coherence Limited transverse spatial coherence Transverse spatial coherence, limited temporal coherence without seeding Energy Position Time <.01% (with ~0.1% energy spread) < 0.1 s (~10 mm H, ~0.3 mm V) < 0.1 s (~1 ps, ~0.2 ps low a) 0.01-0.03% wo / self seeding ~0.1 s ~100 fs Number of Beamlines Large (~30-60) Limited (6 endstations per undulator) Stability

Frontiers of FEL and Storage Ring Development Storage Rings ‘Ultimate Storage Ring’ technology Diffraction limited emittance resulting in: higher peak brightness higher average brightness enhanced coherence Free Electron Lasers Seeding  Higher brightness (peak and average), better energy stability, reduction of temporal and intensity fluctuations More undulators per injector Higher rep rate  Higher average brightness Shorter pulses Multiple colors

How will Storage Rings and FELs Compare in the Future? Parameter Storage Rings FEL Wavelength Range 2-3 decades typically 1-2 decades (multiple undulators) Peak Brightness (ph/s/mr2/mm2/0.1%BW) 1024 – 1026 (x 100 increase but still modest compared to FEL) 1031 – 1033 Average Brightness (ph/s/mr2/mm2/0.1%BW) 1021– 1023 (x 100 increase) 1023– 1025 (x 1000 increase) Minimum Pulse Width (fs) ~1000 Below ~1 fs Coherence High spatial coherence Full coherence Energy Position Time <.01% (with ~0.1% energy spread) < 0.1 s (~0.3 mm H, V) < 0.1 s (~0.5 ps ) < 0.1 eV (seeded) ~0.1 s ~10 fs Number of Beamlines Large (~30-60) Limited (~3-6 endstations per undulator), multiple undulators per facility Stability

Path to the Future… Europe, Asia and the US are taking different approaches to deliver capability and capacity Hard x-ray facilities vs. soft x-ray facilities Storage Ring vs FEL vs ERL Balance investments in ~1B$ class tools and ~100M$ class infrastructure to exploit the tools What’s the best (affordable) idea?

Ring Horizontal Emittance vs Ring Energy Ring Name (Circumference in km) Achieved Construction Design Diffraction Limit @1Å ε ~ λ/4π ~ 8 pm

Hard X-Ray FELs in Operation & Under Construction LCLS-I, II 2009, 2018 14.5 GeV, 120 Hz NC SACLA 2011 8.5 GeV, 60 Hz NC XFEL 2015 17.5 GeV, 3000 x 10 Hz SC PAL XFEL 2015 10 GeV, 100 Hz NC SWISS FEL 2017 5.8 GeV, 100 Hz NC Four normal conducting (NC) linacs One pulsed superconducting (SC) linac How low can Ee & $ go without dashing performance?

Asian Strategy SACLA 2011 8.5 GeV, 60 Hz NC PAL XFEL 2015 Current Status: SPring-8: High performing 3rd generation SR Many other ‘regional’ storage rings SACLA: 60 Hz, one beam line hard x-ray FEL Near Future: Upgrade SPring-8 to ‘USR’ at 6 GeV Upgrade SACLA SACLA with additional injector and additional undulators New FEL in Korea: PAL XFEL One beam line, 100Hz Far Future: 3 GeV ERL @ KEK SACLA 2011 8.5 GeV, 60 Hz NC PAL XFEL 2015 10 GeV, 100 Hz NC

European Strategy XFEL 2015 17.5 GeV, 3000 x 10 Hz SC Current Status: Several high performance hard-x-ray SR ESRF, PETRA-3 Several high performance soft/medium x-ray SR BESSY-II, SLS, Diamond, SOLEIL Two soft x-ray FEL’s FLASH I & FERMI with1 undulator each Near Future Upgrade ESRF to ‘USR’, build new high performance ring (MAX-4), expand PETRA-3 Expand FLASH I  FLASH II Two new hard x-ray FELs: XFEL: rep rate 3000 x 10; 6 undulators SwissFEL: rep rate 100 Hz and 1 undulator XFEL 2015 17.5 GeV, 3000 x 10 Hz SC SWISS FEL 2017 5.8 GeV, 100 Hz NC

European Strategy Continued By 2020, Europe will have the most advanced suite of light source tools in the world Enormous concentration of tools in Hamburg FLASH I, II PETRA-3 XFEL (managed by XFEL corporation) German strategy includes tremendous investments in infrastructure to exploit the light sources and deliver science CFEL CSSB Nanocenter Nano-Bio-Femto

DESY Science Platforms Center for Free Electron Laser Science Site Prep: Center for Structural Systems Biology Conceptual Design: NanoLab

Investments at DESY Over 5 Years 1 Euro = $1.30

BES USA Strategy Current State Near Future Longer Future (past 2020) 4 storage rings 3 hard x-ray, 1 soft x-ray 1 hard x-ray FEL: 120 Hz, one undulator, 6 endstations Near Future NSLS II: 104 boost in brightness, goal of 1 nm spatial & 0.1 meV energy resolution APS will be upgraded to APS-U, brightness boost and high rep rate 2 ps pulse capability LCLS II will extend capacity and capability with a new injector + 1km of linac, 2 undulators and 5-6 endstations. Longer Future (past 2020) NGLS Proposal: MHz rep rates and ultimately10 undulators in soft x-ray FEL 2015 2018 2018 BES Strategy will be guided and informed by the BESAC Report we are about to discuss >2020

Conclusions Our charge: ‘The Charge to BESAC that we have been asked to address is to determine what is the most challenging and important science yet to be done that will require light sources and to determine the best sources, we can afford, that will allow us to explore those scientific frontiers’ The goal of this talk was to help set the stage: By 2020 Europe will have the most advanced suite of light source tools in the world There will be an extraordinarily high concentration of those tools in Hamburg, along with excellent supporting infrastructure to deliver science In addition to new FEL sources, both Europe and Japan propose to upgrade their hard x-ray rings to near diffraction limited Existing US sources will still be very competitive into the 2020’s but the quality of the science performed at the US user facilities rather than the facilities specs alone will have to set the US apart from the pack The work of this subcommittee is extremely important to ensure the US is well positioned past 2020