LCLS-II: Accelerator Systems LCLS SAC Meeting P. Emma et al. April 23, 2010.

Slides:



Advertisements
Similar presentations
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.
Advertisements

Soft X-ray Self-Seeding
Approaches for the generation of femtosecond x-ray pulses Zhirong Huang (SLAC)
SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE.
Hard X-ray FELs (Overview) Zhirong Huang March 6, 2012 FLS2012 Workshop, Jefferson Lab.
1 Enhancements to the Linac Coherent Light Source.
P. Emma LCLS FAC 12 Oct Comments from LCLS FAC Meeting (April 2004): J. Roßbach:“How do you detect weak FEL power when the.
P. Emma FAC Meeting 7 Apr Low-Charge LCLS Operating Point Including FEL Simulations P. Emma 1, W. Fawley 2, Z. Huang 1, C.
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.
LCLS Transition to Science DOE Status Review of the LUSI MIE Project Near term opportunities for LCLS 'upgrades' J. Hastings for the LCLS Experimental.
Status of LCLS A. Brachmann, SLAC National Accelerator Laboratory.
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
S. Spampinati, J.Wu, T.Raubenhaimer Future light source March, 2012 Simulations for the HXRSS experiment with the 40 pC beam.
Soft X-ray Self-Seeding in LCLS-II J. Wu Jan. 13, 2010.
Paul Emma, et. al. Sep. 18, 2013 Paul Emma, et. al. Sep. 18, 2013 Design Considerations for the NGLS (Next Generation Light Source) NGLS.
Transverse Profiling of an Intense FEL X-Ray Beam Using a Probe Electron Beam Patrick Krejcik SLAC National Accelerator Laboratory.
Two Longitudinal Space Charge Amplifiers and a Poisson Solver for Periodic Micro Structures Longitudinal Space Charge Amplifier 1: Longitudinal Space Charge.
The Future of Photon Science and Free-Electron Lasers Ingolf Lindau Lund University and Stanford University MAX-Lab and Synchrotron Light Research KTH,
FLASH II. The results from FLASH II tests Sven Ackermann FEL seminar Hamburg, April 23 th, 2013.
Beam Dynamics and FEL Simulations for FLASH Igor Zagorodnov and Martin Dohlus Beam Dynamics Meeting, DESY.
A bunch compressor design and several X-band FELs Yipeng Sun, ARD/SLAC , LCLS-II meeting.
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.
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,
LCLS-II Capabilities & Overview LCLS-II Science Opportunities Workshop Tor Raubenheimer February 10 th, 2015.
Max Cornacchia, SLAC LCLS Project Overview BESAC, Feb , 2001 LCLS Project Overview What is the LCLS ? Transition from 3 rd generation light sources.
External Seeding Approaches: S2E studies for LCLS-II Gregg Penn, LBNL CBP Erik Hemsing, SLAC August 7, 2014.
Basic Energy Sciences Advisory Committee MeetingLCLS February 26, 2001 J. Hastings Brookhaven National Laboratory LCLS Scientific Program X-Ray Laser Physics:
FEL R&D Zhirong Huang May4, 2011 Pre-SPC Meeting for Accelerator R&D.
Harmonic lasing in the LCLS-II (a work in progress…) G. Marcus, et al. 03/11/2014.
Harmonic Lasing for LCLS-II? Z. Huang 11/10/
P. Krejcik LINAC 2004 – Lübeck, August 16-20, 2004 LCLS - Accelerator System Overview Patrick Krejcik on behalf of the LCLS.
Singel pass FELs for ERL. X-RAY FELS BASED ON ERL FACILITIES A. Meseck, C. Mayes F. Löhl G. Hoffstätter.
LCLS-II Design and FEL R&D
The Next Generation Light Source Test Facility at Daresbury Jim Clarke ASTeC, STFC Daresbury Laboratory Ultra Bright Electron Sources Workshop, Daresbury,
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/
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),
Twin bunches at FACET-II Zhen Zhang, Zhirong Huang, Ago Marinelli … FACET-II accelerator physics workshop Oct. 12, 2015.
Lessons Learned From the First Operation of the LCLS for Users Presented by Josef Frisch For the LCLS March 14, 2010.
Preliminary Tracking Results through LCLS-II P. Emma et al., Oct. 23, 2013 Thanks to Mark Woodley and Yuri Nosochkov for MAD design work Use Christos Papadopoulos.
FEL Spectral Measurements at LCLS J. Welch FEL2011, Shanghai China, Aug. 25 THOB5.
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.
LCLS-II Project Overview David Schultz LCLS-II Deputy Project Director March 19, 2012.
E. Schneidmiller and M. Yurkov FEL Seminar, DESY April 26, 2016 Reverse undulator tapering for polarization control at X-ray FELs.
Harmonic lasing in the LCLSII SXR beamline G. Marcus, Y. Ding, Z. Huang 11/21/2013.
1 0.1-nm Hard X-ray XFEL  Project Period: 2011 ~ 2015  Total Budget: 400 M$  10-GeV Electron Linac (Normal Conducting S-band, 60 Hz)  Total Length:
A single-shot method for measuring fs bunches in linac-based FELs Z. Huang, K. Bane, Y. Ding, P. Emma.
Applications of transverse deflecting cavities in x-ray free-electron lasers Yuantao Ding SLAC National Accelerator Laboratory7/18/2012.
LCLS-II options: CuRF → SXR, VPU, HXR harmonics G. Marcus 5/13/2015.
Some Simulations for the Proposed Hard X-Ray Self- Seeding on LCLS J. Wu J. Wu et al. Feb. 25, 2011.
Harmonic Generation in a Self-Seeded Soft X-Ray LCLS-II J. Wu Feb. 24, 2010.
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.
Eduard Prat / Sven Reiche :: Paul Scherrer Institute
LCLS-II: An upgrade for the LINAC Coherent Light Source
Beam dynamics for an X-band LINAC driving a 1 keV FEL
Sara Thorin, MAX IV Laboratory
Status and Interest of the X-ray FEL SINAP
Short pulse, low charge LCLS operation
Gu Qiang For the project team
LCLS Instrument Development
LCLS-II-HE FEL Facility Overview
Review of Application to SASE-FELs
LCLS-II-HE FEL Facility Overview
Self-seeding for the soft x-ray line in LCLS upgrade
WBS 5.0 LCLS Strategic Projects Division
Z. Huang LCLS Lehman Review May 14, 2009
Two-bunch self-seeding for narrow-bandwidth hard x-ray FELs
LCLS FEL Parameters Heinz-Dieter Nuhn, SLAC / SSRL April 23, 2002
Introduction to Free Electron Lasers Zhirong Huang
Presentation transcript:

LCLS-II: Accelerator Systems LCLS SAC Meeting P. Emma et al. April 23, 2010

LCLS-II: Accelerator Systems Page Å FEL Saturation at 65 m (of 112 m) This success motivates an extension of the capacity, capabilities, and quality of this revolutionary new light source. April 26, 2009

LCLS Beam Supports 25-keV (0.5 Å) FEL at 14 GeV increase undulator gap further  x,y = 0.4  m (slice) I pk = 3.0 kA  E /E = 0.01% (slice) 0.5 Å Same beam quality and energy as now 1.5 Å K = 1.65

Ultra-Short Pulses in Operation at LCLS BC2 4.3 GeV BC2 4.3 GeV BC1 250 MeV BC1 250 MeV L1S L2-linac L3-linac DL1 135 MeV DL1 135 MeV gun  wall undulator 4-14 GeV undulator 4-14 GeV 1.5 Å Et under- compressed  =  0.6º E tfullycompressed peak current monitor (CSR) gas detector (FEL power) Measurements at 20 pCEt over-compressed  =  0.5º 

Ultra-Short X-ray Pulse Simulations Suggest <10 fs FWHM 20 pC bunch charge 3 keV initial rms slice energy spread 0.23-mm initial rms bunch length X-ray pulse duration should be <10 fs (FWHM), but no measurement possible yet …now delivered to users fully compressed

LCLS-II Requirements Build new soft x-ray line from 200 to eV Extend hard x-rays out to ~20 keV Include seeding options for narrow BW Incorporate 2-pulse, 2-color schemes Provide polarization control Take advantage of 3-km SLAC linac to provide separate sources for independent FELs Explore multi-bunch operations Find ways to increase capacity (user access)! Build new soft x-ray line from 200 to eV Extend hard x-rays out to ~20 keV Include seeding options for narrow BW Incorporate 2-pulse, 2-color schemes Provide polarization control Take advantage of 3-km SLAC linac to provide separate sources for independent FELs Explore multi-bunch operations Find ways to increase capacity (user access)! LCLS-II: Accelerator Systems Page 6

X undulator L1 L2L3BC1BC2 RFgun-1 L GeV sector-10sector-20sector-24sector-14 existing LCLS enclosure exists at sector 10 und-hall sector-30 L3 XRFgun-2L1 L2BC1BC2 L0 Sector-20 wall 3-7 GeV e  bypass line 3-7 GeV new undulators LCLS-II: New Injector & Accelerator Use 2 nd km of SLAC linac (sector-10 to 20) – greater flexibility 3-7 GeV energy (no SLED) allows possible 360-Hz beam rate 2 nd injector, linac, & bypass line allows 2+ independent FELs serving 2 experiments simultaneously with flexible parameters Combining beams allows x-ray pump/probe with decoupled wavelengths, pulse width, energy, and timing Preserves possibility of GeV (and still 1 more km left!)

Phase-1 (2010) Å GW 3-15 GeV FEE-1 Existing 112-m Undulator ( Å) SHAB 30 m Å Shortened 80-m ( Å) FEE-2 SXR2 (36 m) 5 m full polarization control self-seeding option 6-60 Å adjust. gap 6-60 Å adjust. gap SXR1 (36 m) 3-7-GeV bypass 3-7-GeV SXR and 3-15-GeV HXR simultaneous op’s with bypass line 2-pulse 2-color No civil construction. Uses existing beam energy and quailty. ExistingPhase-2Phase-3EEHG*? 240 nm  6 nm Phased Enhancement Plan for LCLS-II FELs * G. Stupakov, Phys. Rev. Lett. 102, (2009) 5 m full polarization control Å Increased fixed-gap: 112 m ( Å) Å Å (54 m) Å (54 m Å (54 m) self-seeding HXR option (2 bunches) Å 1-2 GW H.-D. Nuhn

1.5 Å (and 0.5 Å), K = Å, K = 2.26 /2 /2 Fast Path to Producing FEL 2 nd Harmonic 16 keV = 0.75 Å (up to 20 keV at 15 GeV) Smaller  function in afterburner helps 2 nd harmonic after-burner 9 undulators LCLS undulator cross- section Replace shims for last 8-10 undulators (of 33) Z. Huang, S. Reiche existing LCLS undulator 2 nd harm. bunching 2 nd harm. bunching

10-m chicane 1 st undulator 2 nd undulator SASE FEL grating Seeded FEL grazing mirrors slit e  dump Self-Seeded SXR FEL in LCLS-II FWHM 3.1  10  4 FEL spectrum at ~26 m in 2 nd undulator for seed of 0.1 MW () and 0.01 MW (red). FEL spectrum at ~26 m in 2 nd undulator for seed of 0.1 MW (black) and 0.01 MW (red) MW 0.1 MW 10 MW 2 nd undulator Power on monochromator is amplified 1 st undulator 6 nm Power over 1 st undulator eeee J. Wu et al. (10% transmission)

LCLS-II: Accelerator Systems Page 11 The next 6 slides will graphically outline 6 LCLS-II operating modes… (thanks to H.-D. Nuhn) 1.Hard X-ray SASE 2.Soft X-ray SASE 3.Soft X-ray Self Seeding 4.Two-pulse, two-color soft x-rays (one e  bunch) 5.Two-pulse, two-color soft x-rays (two e  bunches) 6.Seeded soft x-ray FEL (‘Echo’) 7.Self Seeding of hard x-rays (two e  bunches)

FEE-1 FEE-2 SX2 (36 m) APU polarization control self-seeding option 6-60 Å adjust. gap 6-60 Å adjust. gap Sector-10 Gun 3-7-GeV Beam SX1 (36 m) 2-pulse 2-color 1. LCLS-II: Hard X-Ray SASE APU polarization control Sector-20 Gun GeV Beam APU SHAB ( Å) LCLS-I Undulator ( Å) 2 nd harmonic after-burner in 2010 ( Å, 1-2 GW) Open all 33 undulator gaps for LCLS-II ( Å, GW) Or (?) replace all with variable gap ( Å, >20 GW) Z. Huang, S. Reiche, FEL’04, 201, (2004). Larger Gap Undulator (112 m) ( Å)

FEE-1 polarization control Sector-20 Gun GeV Beam Larger Gap Undulator ( Å) APU SHAB ( Å) LCLS-I Undulator ( Å) FEE-2 SX2 (36 m) APU polarization control self-seeding option 6-60 Å adjust. gap 6-60 Å adjust. gap Sector-10 Gun 3-7-GeV Beam SX1 (36 m) 2-pulse 2-color 2. LCLS-II: SX2 (or SX1) SASE APU polarization control APU Simple use of new soft x-ray line: SASE from SX2 (or SX1) Full polarization control (fast at 80% or slow at ~100%) Y. Ding, Z. Huang, Phys. Rev. ST-AB 11, (2008).

FEE-2 SX2 (36 m) polarization control self-seeding option 6-60 Å adjust. gap 6-60 Å adjust. gap Sector-10 Gun 3-7-GeV Beam SX1 (36 m) 2-pulse 2-color 3. LCLS-II: Soft X-Ray Self-Seeding APU polarization control APU FEE-1 polarization control Sector-20 Gun GeV Beam Larger Gap Undulator ( Å) APU SHAB ( Å) LCLS-I Undulator ( Å) SX1 pulse passes monochromator and seeds SX2 pulse Narrow bandwidth pulse to <10  4 FWHM (6-60 Å) Can also use chirped bunch to generate short pulse (<50 fs) J. Feldhaus et al., Opt. Commun. 140, 341 (1997).

FEE-1 FEE-2 polarization control self-seeding option 6-? Å adjust. gap ?-60 Å adjust. gap Sector-10 Gun 3-7-GeV Beam SX1 (36 m)delay polarization control 4. LCLS-II: SX1 & 2 SASE, One-Bunch, Two-Color APU polarization control Sector-20 Gun GeV Beam Larger Gap Undulator ( Å) APU SX2 (36 m) One e  bunch produces 2 SXR pulses (0-15 ps separation) for pump probe Deliver both pulses to one experiment or split them to two SX2 pulse color (  ) must be longer wavelength than SX1 (  ) Angled SX2 suggested by J. Hastings and P. Heimann  

FEE Å adjust. gap 6-60 Å adjust. gap Sector-10 Gun 3-7-GeV Beam SX1 (36 m) 5. LCLS-II: SX1 & 2 SASE, Two-Bunch, Two-Color Sector-20 Gun GeV Beam Larger Gap Undulator ( Å) APU DC Dipole Magnet FEE-2 SX2 (36 m) Fast Kicker Magnet e  Dump color-1 color-2 Two e  bunches ns apart (no pump probe here) One fast kicker & one DC – each bunch lases in just one FEL Allows 2 SXR experiments simultaneously (user doubler) Two colors can be any value (6-60 Å) Suggested by J. Frisch and independently by R. Brinkmann et al.

FEE-1 polarization control Sector-20 Gun GeV Beam Larger Gap Undulator ( Å) APU SHAB ( Å) LCLS-I Undulator ( Å) FEE-2 SX2 (36 m) APU polarization control self-seeding option 6-60 Å adjust. gap 6-60 Å adjust. gap 2-pulse 2-color 6. LCLS-II: Echo Seeding of SX1 or SX2 polarization control APU External seeding (~30-60 Å) using Echo-Enhanced Harmonic Generation (EEHG*) – not in LCLS-II baseline at present Allows narrow BW and longitudinal coherence Under study now at NLCTA (SLAC) EEHG 240 nm  6 nm Sector-10 Gun 3-7-GeV Beam APU * G. Stupakov, Phys. Rev. Lett. 102, (2009) SX1 (36 m)

Planar + Helical Stable >90% polarization Slow switching Planar + Helical Stable >90% polarization Slow switching Planar + Crossed Planar May have fluctuations ~80% polarization Fast switching Planar + Crossed Planar May have fluctuations ~80% polarization Fast switching Planar + Crossed Pair at Stable ~90% Fast switching ~1% of fundamental power Planar + Crossed Pair at Stable ~90% Fast switching ~1% of fundamental power EPUEPU ~4L G helical operate near saturation EPUEPU APPLE planar mode ( y ) fast polarization control with pulsed phase shifter EPUEPU EPUEPU 2 crossed planar APPLEs at operate in saturation PlanarPlanar PlanarPlanar PlanarPlanar ~1.3L G for P x = P y Z. Huang

Peak Brightness of LCLS H.-D. Nuhn

LCLS-II Timeline, Compatible with Operations Annual 3 month summer downtime FY12 FY12 FY13 FY13 FY15 FY15 FY14 FY14 FY16 FY16 FY17 FY17 Phase-1 Installation Phase-2 Installation ED&IED&I FabricationFabrication FY11 FY11 R&DR&D CD 1 CD 2, 3a CD 3 CD 4 CDR InstallationInstallation FY10 FY10 CD 0 Facilities Installation FY18 FY18 LCLS-II: Accelerator Systems Page 20

LCLS-II Accelerator Summary Soft X-Rays: 2-pulse, 2-color, variable delay (6-60 Å) using 1 e  bunch or 2 Self-seeding for narrow bandwidth (~10  4 at 6-60 Å) Full polarization control in SASE and self-seeded modes (fast & slow) 3-7 GeV bypass line allows simultaneous soft and hard x-ray operations in two separate beamlines with completely independent parameters Single femtosecond near-transform limited spike in low-charge mode LCLS-II: Accelerator Systems Page 21 Hard X-Rays: Harder x-rays (0.62 Å) by modifying all undulators Few femtosecond pulses possible in low-charge mode Full polarization control Self-seeding with 2 electron bunches and short chicane (4 m) And… GeV still possible using both 1-km linacs (+ 3 rd km still open)