Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory LCLS Scientific Program X-Ray Laser Physics:

Slides:



Advertisements
Similar presentations
X-ray Free Electron lasers Zhirong Huang. Lecture Outline XFEL basics XFEL basics XFEL projects and R&D areas XFEL projects and R&D areas Questions and.
Advertisements

Schemes for generation of attosecond pulses in X-ray FELs E.L. Saldin, E.A. Schneidmiller, M.V. Yurkov The potential for the development of XFEL beyond.
Soft X-ray Self-Seeding
Workshop Issues Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center Diagnostics.
1 Optimal focusing lattice for XFEL undulators: Numerical simulations Vitali Khachatryan, Artur Tarloyan CANDLE, DESY/MPY
1 Bates XFEL Linac and Bunch Compressor Dynamics 1. Linac Layout and General Beam Parameter 2. Bunch Compressor –System Details (RF, Magnet Chicane) –Linear.
LCLS Linac Coherent Light Source Update John N. Galayda LCLS Project Manager Basic Energy Sciences Advisory Committee Meeting 2-3 August 2001.
Sub-femtosecond bunch length diagnostic ATF Users Meeting April 26, 2012 Gerard Andonian, A. Murokh, J. Rosenzweig, P. Musumeci, E. Hemsing, D. Xiang,
Professor David Attwood / UC Berkeley / ICTP-IAEA School, Trieste, November 2014 ICTP_Trieste_Lec1_Nov2014.pptx Introduction to Synchrotron Radiation and.
Approaches for the generation of femtosecond x-ray pulses Zhirong Huang (SLAC)
P. Emma LCLS FAC 12 Oct Comments from LCLS FAC Meeting (April 2004): J. Roßbach:“How do you detect weak FEL power when the.
The BESSY Soft X-Ray SASE FEL (Free Electron Laser)
Undulator Physics April 29, 2004 Heinz-Dieter Nuhn, SLAC / SSRL Facility Advisory Committee Meeting Undulator Physics Diagnostics.
Performance Analysis Using Genesis 1.3 Sven Reiche LCLS Undulator Parameter Workshop Argonne National Laboratory 10/24/03.
A. Zholents, July 28, 2004 Timing Controls Using Enhanced SASE Technique *) A. Zholents or *) towards absolute synchronization between “visible” pump and.
Undulator Gap Increase Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center.
Overview of Proposed Parameter Changes Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator.
E. Bong, SLACLCLS FAC Meeting - April 29, 2004 Linac Overview E. Bong LCLS FAC Meeting April 29, 2004 LCLS.
UCLA The X-ray Free-electron Laser: Exploring Matter at the angstrom- femtosecond Space and Time Scales C. Pellegrini UCLA/SLAC 2C. Pellegrini, August.
John Arthur LCLS Diagnostics and Commissioning September 22, 2004 Summary of Related Topics from the Miniworkshop on.
New Electron Beam Test Facility EBTF at Daresbury Laboratory B.L. Militsyn on behalf of the ASTeC team Accelerator Science and Technology Centre Science.
PAC2001 J. Rossbach, DESY 1 New Developments on Free Electron Lasers Based on Self-amplified Spontaneous Emission J. Rossbach, DESY Why SASE FELs? How.
Steve LidiaICFA Workshop, Chia LagunaJuly, 2002 Flat Beam Photoinjectors for Ultrafast Synchrotron Radiation Sources Steve Lidia Lawrence Berkeley National.
W.S. Graves1 Seeding for Fully Coherent Beams William S. Graves MIT-Bates Presented at MIT x-ray laser user program review July 1, 2003.
Low Emittance RF Gun Developments for PAL-XFEL
+ SwissFEL Introduction to Free Electron Lasers Bolko Beutner, Sven Reiche
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.
R&D Towards X-ray Free Electron Laser Li Hua Yu Brookhaven National Laboratory 1/23/2004.
S2E in LCLS Linac M. Borland, Lyncean Technologies, P. Emma, C. Limborg, SLAC.
Free Electron Lasers (I)
Soft X-ray Self-Seeding in LCLS-II J. Wu Jan. 13, 2010.
Linac Coherent Light Source Coherent Synchrotron Radiation Workshop
Two Longitudinal Space Charge Amplifiers and a Poisson Solver for Periodic Micro Structures Longitudinal Space Charge Amplifier 1: Longitudinal Space Charge.
Beam Dynamics and FEL Simulations for FLASH Igor Zagorodnov and Martin Dohlus Beam Dynamics Meeting, DESY.
Optimization of Compact X-ray Free-electron Lasers Sven Reiche May 27 th 2011.
A bunch compressor design and several X-band FELs Yipeng Sun, ARD/SLAC , LCLS-II meeting.
J. Wu In collaboration with Y. Jiao, W.M. Fawley, J. Frisch, Z. Huang, H.-D. Nuhn, C. Pellegrini, S. Reiche (PSI), Y. Cai, A.W. Chao, Y. Ding, X. Huang,
Max Cornacchia, SLAC LCLS Project Overview BESAC, Feb , 2001 LCLS Project Overview What is the LCLS ? Transition from 3 rd generation light sources.
Vladimir Bushuev Effect of the Thermal Heating of a Crystal
P. Krejcik LINAC 2004 – Lübeck, August 16-20, 2004 LCLS - Accelerator System Overview Patrick Krejcik on behalf of the LCLS.
The Next Generation Light Source Test Facility at Daresbury Jim Clarke ASTeC, STFC Daresbury Laboratory Ultra Bright Electron Sources Workshop, Daresbury,
Design Considerations of table-top FELs laser-plasma accelerators principal possibility of table-top FELs possible VUV and X-ray scenarios new experimental.
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/
PAC-2001, Chicago, IL Paul Emma SLAC SLAC Issues and R&D Critical to the LCLS UCLA LLNL.
LCLS-II: Accelerator Systems LCLS SAC Meeting P. Emma et al. April 23, 2010.
J. Wu March 06, 2012 ICFA-FLS 2012 Workshop Jefferson Lab, Newport News, VA Tolerances for Seeded Free Electron Lasers FEL and Beam Phys. Dept. (ARD/SLAC),
Lessons Learned From the First Operation of the LCLS for Users Presented by Josef Frisch For the LCLS March 14, 2010.
김 귀년 CHEP, KNU Accelerator Activities in Korea for ILC.
Awake electron beam requirements ParameterBaseline Phase 2Range to check Beam Energy16 MeV MeV Energy spread (  ) 0.5 %< 0.5 % ? Bunch Length (
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.
Injector Requirements Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile.
X-band Based FEL proposal
E. Schneidmiller and M. Yurkov FEL Seminar, DESY April 26, 2016 Reverse undulator tapering for polarization control at X-ray FELs.
Operation and Upgrades of the LCLS J. Frisch 1,R. Akre 1, J. Arthur 1, R. Bionta 2, C. Bostedt 1, J. Bozek 1, A. Brachmann 1, P. Bucksbaum 1, R. Coffee.
Free Electron Laser Studies
Beam dynamics for an X-band LINAC driving a 1 keV FEL
Paul Scherrer Institut
Review of Application to SASE-FELs
F. Villa Laboratori Nazionali di Frascati - LNF On behalf of Sparc_lab
Self-seeding for the soft x-ray line in LCLS upgrade
Z. Huang LCLS Lehman Review May 14, 2009
Two-bunch self-seeding for narrow-bandwidth hard x-ray FELs
Design of an ECHO-seeded FEL at nm wavelength
Status of FEL Physics Research Worldwide  Claudio Pellegrini, UCLA April 23, 2002 Review of Basic FEL physical properties and definition of important.
Gain Computation Sven Reiche, UCLA April 24, 2002
Optics John Arthur, SLAC & William W. Craig, LLNL April 24, 2002
LCLS FEL Parameters Heinz-Dieter Nuhn, SLAC / SSRL April 23, 2002
Introduction to Free Electron Lasers Zhirong Huang
Enhanced Self-Amplified Spontaneous Emission
Electron Optics & Bunch Compression
Presentation transcript:

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory LCLS Scientific Program X-Ray Laser Physics: Advanced R&D J. B. Hastings Brookhaven National Laboratory February 26, 2001 Focusing of X-Ray Pulses Generation Shorter X-Ray Pulses Increase of Longitudinal Coherence Focusing of X-Ray Pulses Generation Shorter X-Ray Pulses Increase of Longitudinal Coherence

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Working Group Members J. B. Hastings, Brookhaven National Laboratory, Upton, NY, USA J. Arthur, Stanford Linear Accelerator Center, Stanford, CA, USA P. Emma, Stanford Linear Accelerator Center, Stanford, CA, USA A. Freund, European Synchrotron Radiation Facility, Grenoble, France D. Mills, Argonne National Laboratory, Argonne, IL, USA C. Pellegrini, University of California, Los Angeles, CA, USA D. Peter Siddons, Brookhaven National Laboratory, Upton, NY, USA R. Tatchyn, Stanford Linear Accelerator Center, Stanford, CA, USA A. Toor, Lawrence Livermore National Laboratory, Livermore, CA, USA L.-H. Yu, Brookhaven National Laboratory, Upton, NY, USA J. B. Hastings, Brookhaven National Laboratory, Upton, NY, USA J. Arthur, Stanford Linear Accelerator Center, Stanford, CA, USA P. Emma, Stanford Linear Accelerator Center, Stanford, CA, USA A. Freund, European Synchrotron Radiation Facility, Grenoble, France D. Mills, Argonne National Laboratory, Argonne, IL, USA C. Pellegrini, University of California, Los Angeles, CA, USA D. Peter Siddons, Brookhaven National Laboratory, Upton, NY, USA R. Tatchyn, Stanford Linear Accelerator Center, Stanford, CA, USA A. Toor, Lawrence Livermore National Laboratory, Livermore, CA, USA L.-H. Yu, Brookhaven National Laboratory, Upton, NY, USA

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Photons/pulse/100 nm spot Landscape of damage tolerance Ionisation and subsequent sample explosion cause diffraction intensities to change Agreement factor: Time (fs) Crystallographic R-factor for proteins in the PDB

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Calculated limits of resolution with R electronic = 15 % Limit with 1 photon/pixel Limit with 9 photons/pixel

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Temporal and Spatial Scales Time in femtoseconds, distance in Å H 2 O  OH + H CH 2 I 2  CH 2 I + I

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Shortest Fundamental FEL Radiation Wavelength1.5Å Electron Beam Energy14.3GeV Normalized RMS Slice Emittance 1.2mm-mrad Peak Current3.4kA FEL Mode Source Size (FWHM)78  m FEL Mode Source Divergence (FWHM)1  rad Peak Brightness * X-Ray Pulse Length (FWHM)230fs Average Time Between Micro-Pulses0.9fs Average Full width of Micro-Pulses0.2fs Average Number of Micro-Pulses in Pulse250 Transverse CoherenceFull Slice Bandwidth Projected Bandwidth * photons/sec/mm 2 /mrad 2 /0.1%-BW LCLS Baseline Design Parameters

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Focusing of LCLS Pulses Focusing is singularly important phase space transformation of the LCLS pulse Available Field Strengths ~10 10 V/m  V/m Proposed R&D in six areas critical to Reflective, Diffractive and Refractive focusing Focusing is singularly important phase space transformation of the LCLS pulse Available Field Strengths ~10 10 V/m  V/m Proposed R&D in six areas critical to Reflective, Diffractive and Refractive focusing Beam Diameter ~100  m -> ~100 nm X-ray field 5x10 17 W/cm 2 exceeds atomic unit: 3.5x10 16 W/cm 2

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory SLAC linac tunnel FFTB tunnel Linac-0 Linac-1Linac-2Linac-3 BC-1 BC-2 DL-2 DL-1 undulator L  120 m 7 MeV  z  0.84 mm 150 MeV  z  0.84 mm 250 MeV  z  0.20 mm 4.54 GeV  z  mm GeV  z  mm...existing linac (8/29/00) new RF gun Linac-X Short-Pulse Generation (Electron Bunch): LCLS Accelerator and Compressor Schematic Courtesy of P. Emma, SLAC X

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Short-Pulse Generation (Electron Bunch): Magnetic Electron Bunch Compression  z z z RF Accelerating Voltage Path Length-Energy Dependent Beamline V = V 0 sin(  ) z0z0 zz  z = R 56  Under- compression Over- compression Courtesy of P. Emma, SLAC

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory nominal LCLS compression Q = 1 nC chirped compression Q = 0.6 nC 230 fs 240 fs 1% 0.01%  E/E Current Z (  m)

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Short-Pulse Generation (X-Ray Pulse): Based on Chirping Chirped X-Ray Pulse Generated from Chirped Electron Pulse in FEL Undulator 1% Chirp Amplitudes Obtainable Optical techniques using the chirped pulse Optical Pulse Compression Optical Pulse Slicing with Zone Plates, Multi-Layers, Crystals Chirped X-Ray Pulse Generated from Chirped Electron Pulse in FEL Undulator 1% Chirp Amplitudes Obtainable Optical techniques using the chirped pulse Optical Pulse Compression Optical Pulse Slicing with Zone Plates, Multi-Layers, Crystals

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Optical Compression and Pulse Slicing  Z (t)  Pulse Slicing Pulse Compression  

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Optical Pulse Compression Optical pulse compression by energy chirping the photon beam and compressing it with 2 gratings. Example of minimum pulse length: Minimum pulse length:~ 10 fs Wavelength spread:2 % Grating line separations:5.5  m Gratings vert. separation:75 cm Gratings hor. separation:107 m Incident angle at grating:0.2 mrad Grating length:1 m Courtesy of C. Pellegrini, SLAC No Practical Solution has yet been worked out

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Optical Pulse Slicing with Crystals Minimum sliced bunch length ~ 10 fs

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory SASE FEL theory well developed and verified by simulations FEL radiation starts from noise in spontaneous radiation Transverse radiation electric field modulates the energy and bunches the electrons within an optical wavelength Exponential build-up of radiation along undulator length SASE FELs Undulator Regime Exponential Gain Regime Saturation 0.2 fs 0.9 fs 1 % of X-Ray Pulse Electron Bunch Micro-Bunching

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Longitudinal coherence SASE FEL starts up from noise No longitudinal coherence Seeding Impose microbunching of the electron beam Output is the amplified input Preserves the longitudinal coherence of the seed An example: self seeding SASE FEL starts up from noise No longitudinal coherence Seeding Impose microbunching of the electron beam Output is the amplified input Preserves the longitudinal coherence of the seed An example: self seeding

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Increase of Longitudinal Coherence : Two Stage FEL Undulator 1 Linac Undulator 2 Monochromator Electrons Electron Beam Dump X-Rays LCLS Spectral Properties Control

Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory Summary The LCLS design opens the possibility for adjusting X-Ray beam parameters according to the needs of the experiments. Improvement are with high user interest include –Increased Electrical Field Strength (Focusing) –Shorter Bunch Length (Electron Bunch / X-Ray Pulse Compression,slicing) –Increased Longitudinal Coherence (Seeding / Monochromatization) All areas need extensive R&D Efforts 230 fs -> fs V/m -> V/m Coherence Length: 1 fs -> >100 fs Beam Diameter: ~100  m ->below 100nm  E/E: > 10 -6