Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center.

Slides:



Advertisements
Similar presentations
Electron Beam Control and Alignment LCLS FEL Undulator Commissioning Workshop UCLA Jan , 2004 P. Emma, SLAC Undulator collimation and protection.
Advertisements

Workshop Issues Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center Diagnostics.
E. Schneidmiller and M. Yurkov (SASE & MCP) C. Behrens, W. Decking, H. Delsim, T. Limberg, R. Kammering (rf & LOLA) N. Guerassimova and R. Treusch (PGM.
Beam-Based Alignment with New Parameters Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator.
Workshop Introduction Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center Diagnostics.
Hal Tompkins FEE/FEL June 16, FEE/FEL Commissioning Overview By Hal Tompkins Photon Beam Systems Deputy.
October 12, 2006 Heinz-Dieter Nuhn, SLAC / LCLS Undulator Good Field Region and Tuning Strategy 1 Undulator Good Field Region and.
LCLS undulator diagnostics and commissioning workshop January 19-20, 2004 (UCLA) Zhirong Huang, SLAC 1 Linac Coherent Light Source.
Performance Analysis Using Genesis 1.3 Sven Reiche LCLS Undulator Parameter Workshop Argonne National Laboratory 10/24/03.
October 30, 2007 Heinz-Dieter Nuhn, SLAC / LCLS Undulator Commissioning Plans 1 Undulator Commissioning Plans Heinz-Dieter Nuhn,
James Welch October 30, FEL Commissioning Plans J. Welch, et. al. FEL Commissioning Plans J. Welch, et. al. Accelerator.
1 Daniel Ratner 1 Gain Length and Taper August, 2009 FEL Gain length and Taper Measurements at LCLS D. Ratner A. Brachmann, F.J.
P. Emma, SLACLCLS Commissioning – Sep. 22, 2004 Linac Commissioning P. Emma LCLS Commissioning Workshop, SLAC Sep , 2004 LCLS.
Richard M. Bionta XTOD October 12, 2004 UCRL-PRES-XXXXX X Ray Transport, Optics, and Diagnostics, Overview Facility Advisory Committee.
LCLS Undulators October 14, 2004 Heinz-Dieter Nuhn, SLAC / SSRL MMF Review Introduction to the LCLS Undulators Heinz-Dieter Nuhn,
X-Ray Diagnostics for the LCLS Jan , 2004 UCLA.
John N. Galayda LCLS Commissioning 22 September 2004 Welcome/Charge Welcome to the Workshop LCLS Status Since the January.
Undulator Overview FEL Performance Assessment
Undulator Physics Update October 12, 2004 Heinz-Dieter Nuhn, SLAC / LCLS Facility Advisory Committee Meeting Undulator Physics Update.
Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Alignment.
A U.S. Department of Energy Office of Science Laboratory Operated by The University of Chicago Argonne National Laboratory Office of Science U.S. Department.
BBA Related Issues Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center Undulator.
Undulator Gap Increase Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center.
Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Physics.
Opening Comments and Charge 19 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear.
Overview of Proposed Parameter Changes Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator.
A U.S. Department of Energy Office of Science Laboratory Operated by The University of Chicago Argonne National Laboratory Office of Science U.S. Department.
RF Systems and Stability Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center.
Undulator Specifications Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center.
A U.S. Department of Energy Office of Science Laboratory Operated by The University of Chicago Argonne National Laboratory Office of Science U.S. Department.
LCLS Undulator Systems TDR Charge Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 3, 2004.
A U.S. Department of Energy Office of Science Laboratory Operated by The University of Chicago Argonne National Laboratory Office of Science U.S. Department.
EM vs. PM Quads Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center Undulator.
Gek 16/6/041 ITRP Comments on Question 19 GEK 9/06/04 19) For the X-band (warm) technology, detail the status of the tests of the full rf delivery system.
The impact of undulators in an ERL Jim Clarke ASTeC, STFC Daresbury Laboratory FLS 2012, March 2012.
Summary of WG1 K. Kubo, D. Schulte, P. Tenenbaum.
LCLS Prototype Undulator Design LCLS Prototype Undulator Design Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory.
Linac Coherent Light Source Coherent Synchrotron Radiation Workshop
J. Turner 02/07/05 SLAC PEPII Accelerator Physics LER WIGGLER PLAN J. Turner, M. Donald, M. Sullivan, U. Wienands, J. Yocky Motivation and Concerns Details.
FLASH Operation at DESY From a Test Accelerator to a User Facility Michael Bieler FLASH Operation at DESY WAO2012, SLAC, Aug. 8, 2012.
DESY: From High Energy Physics to Synchrotron Radiation Accelerator Operation in a changing Environment Michael Bieler DESY: From High Energy Physics to.
Energy Spectrometer for the ILC Alexey Lyapin University College London.
Transverse Profiling of an Intense FEL X-Ray Beam Using a Probe Electron Beam Patrick Krejcik SLAC National Accelerator Laboratory.
Undulator parameters choice/wish based on a simplified XFEL cost model Jürgen Pfingstner 29 st of July 2015.
Simulation of Microbunching Instability in LCLS with Laser-Heater Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory.
Option – 5m Undulators What is the optimum length for an LCLS undulator?  XFEL is using 5m undulator segments.  Is this optimum?  What are the advantages.
NLC - The Next Linear Collider Project NLC January Video conference Status of Permanent Quadrupoles James T Volk January 18, 2001.
Proposal to use electromagnetic correction coils for RT trajectory correction.
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:
Harmonic lasing in the LCLS-II (a work in progress…) G. Marcus, et al. 03/11/2014.
State-of-the-art devices for compact light sources Finn O’Shea RadiaBeam Technologies October 15, 2015 Cryogenic Short Period Undulators.
PAC-2001, Chicago, IL Paul Emma SLAC SLAC Issues and R&D Critical to the LCLS UCLA LLNL.
Tuning Techniques And Operator Diagnostics for FACET at SLAC National Accelerator Laboratory Chris Melton SLAC Accelerator Operations.
Optics for VUV and soft x-ray FEL Oscillators Michelle Shinn & Steve Benson Future Light Sources Jefferson Lab March 5, 2012 Work supported by the U.S.
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.
Workshop on Accelerator R&D for Ultimate Storage Rings – Oct Nov.1 – Huairou, Beijing, China A compact low emittance lattice with superbends for.
Experience with Novosibirsk FEL Getmanov Yaroslav Budker INP, Russia Dec. 2012, Berlin, Germany Unwanted Beam Workshop.
What did we learn from TTF1 FEL? P. Castro (DESY).
Beam-based alignment techniques for linacs Masamitsu Aiba, PSI BeMa 2014 workshop Bad Zurzach, Switzerland Thanks to Michael Böge and Hans Braun.
Seeding in the presence of microbunching
J. Alexander + Cornell accelerator group Cornell University
Coupling Correction at the Australian Synchrotron
Beam Optics Set-Up at SLAC End Station A
Yuhui Li How to edit the title slide
Phase Adjustments: K vs
Undulator Line Design Liz Moog, Advanced Photon Source April 24, 2002
Introduction to Free Electron Lasers Zhirong Huang
Linac Design Update P. Emma LCLS DOE Review May 11, 2005 LCLS.
Undulator Physics Issues Heinz-Dieter Nuhn, SLAC / LCLS July 11, 2007
Presentation transcript:

Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Diagnostics Workshop John N. Galayda, SLAC 1 LCLS Undulator Diagnostics and Comissioning Workshop Wrap-up John N. Galayda, Stanford Linear Accelerator Center 20 January 2004 Challenges of Commissioning the FEL Alignment Undulator K Undulator Damage Undulator Diagnostics CommissioningOperationCharge Challenges of Commissioning the FEL Alignment Undulator K Undulator Damage Undulator Diagnostics CommissioningOperationCharge

Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Diagnostics Workshop John N. Galayda, SLAC 2 Beam-Based Alignment, Quad Design Tolerances on Trajectory are Tight for SASE at 1.5Å Beam-based alignment, RFBPMs must deliver a good trajectory Dispersion-free steering delivers a “straight” trajectory But beam is not centered in quads at completion Absolute accuracy is not the crucial requirement- sensitivity is critical Ability to change quad gradient would be a significant advantage Iron/copper quads would be longer than 50mm-long permanent magnet quads New gradient is ~60 T/m, about 11 mm bore: 3,000 gauss on the pole? NLC has struggled with “variable” permanent magnet designs Difficult to vary the gradient without moving the magnetic center Electromagnets still perform best in this regard NLC needs beam centered in quads to 1 micron- we don’t Trim windings may be an acceptable option for LCLS Trim windings still leave a residual uncertainty about actual location of quad center “AC” center is not necessarily the same as the “DC” center Tolerances on Trajectory are Tight for SASE at 1.5Å Beam-based alignment, RFBPMs must deliver a good trajectory Dispersion-free steering delivers a “straight” trajectory But beam is not centered in quads at completion Absolute accuracy is not the crucial requirement- sensitivity is critical Ability to change quad gradient would be a significant advantage Iron/copper quads would be longer than 50mm-long permanent magnet quads New gradient is ~60 T/m, about 11 mm bore: 3,000 gauss on the pole? NLC has struggled with “variable” permanent magnet designs Difficult to vary the gradient without moving the magnetic center Electromagnets still perform best in this regard NLC needs beam centered in quads to 1 micron- we don’t Trim windings may be an acceptable option for LCLS Trim windings still leave a residual uncertainty about actual location of quad center “AC” center is not necessarily the same as the “DC” center

Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Diagnostics Workshop John N. Galayda, SLAC 3 Challenges for Diagnostics in the Undulator Channel Tolerance on K of an undulator is around 1.5 x At this time, canted undulator poles provide preferred solution for K fine-tuning (3 milliradians) K tolerance equivalent to 300 micron horizontal displacement K tolerance equivalent to 50 micron vertical misplacement Piezo tuners may be deleted This displacement does little to the electron optics Dispersion-free steering gets beam to within 20 microns of quad centers If quads and undulators are aligned to within 25 microns, this tolerance is met This is not quite impossible; still pretty difficult This displacement does little to the spontaneous spectrum of 1 und. No one disputed this Tolerance on K of an undulator is around 1.5 x At this time, canted undulator poles provide preferred solution for K fine-tuning (3 milliradians) K tolerance equivalent to 300 micron horizontal displacement K tolerance equivalent to 50 micron vertical misplacement Piezo tuners may be deleted This displacement does little to the electron optics Dispersion-free steering gets beam to within 20 microns of quad centers If quads and undulators are aligned to within 25 microns, this tolerance is met This is not quite impossible; still pretty difficult This displacement does little to the spontaneous spectrum of 1 und. No one disputed this

Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Diagnostics Workshop John N. Galayda, SLAC 4 Challenges for Diagnostics in the Undulator Channel Radiation Damage to Undulators is a Concern Interlocks will be implemented but tolerable losses are low ANL-APS actively studying radiation damage to storage ring undulators Can the diagnostics identify a damaged undulator? No one asserts that the LCLS diagnostics suite can do this Radiation Damage to Undulators is a Concern Interlocks will be implemented but tolerable losses are low ANL-APS actively studying radiation damage to storage ring undulators Can the diagnostics identify a damaged undulator? No one asserts that the LCLS diagnostics suite can do this

Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Diagnostics Workshop John N. Galayda, SLAC 5 Will the Undulator Diagnostics Serve Commissioning and Operations Needs for the LCLS? Charge – Will the Undulator Diagnostics Serve Commissioning and Operations Needs for the LCLS? Commissioning Can diagnostics be used to troubleshoot the new hardware? Can diagnostics be used to guide path to saturation? Draft commissioning document emphasizes easier tolerances at long wavelength Implication is that achievement of saturation at 1.5 nm will lead to easier path to 0.15 nm saturation Implication of implication is reliance on FEE diagnostics Does the commissioning plan bear this out? Do simulations show convergence of K-tweaking and steering to optimum output? Commissioning Can diagnostics be used to troubleshoot the new hardware? Can diagnostics be used to guide path to saturation? Draft commissioning document emphasizes easier tolerances at long wavelength Implication is that achievement of saturation at 1.5 nm will lead to easier path to 0.15 nm saturation Implication of implication is reliance on FEE diagnostics Does the commissioning plan bear this out? Do simulations show convergence of K-tweaking and steering to optimum output?

Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Diagnostics Workshop John N. Galayda, SLAC 6 Will the Undulator Diagnostics Serve Commissioning and Operations Needs for the LCLS? Charge – Will the Undulator Diagnostics Serve Commissioning and Operations Needs for the LCLS? Operations Will the diagnostics permit simple and speedy troubleshooting? Reliability/Availability goals of the LCLS will be those of a light source Progressive installation of undulators may work for commissioning, but In operation, this would require automated “removal” of undulators Routine replacement/measurement of undulators must be part of plan Operations troubleshooting needs attention Operations Will the diagnostics permit simple and speedy troubleshooting? Reliability/Availability goals of the LCLS will be those of a light source Progressive installation of undulators may work for commissioning, but In operation, this would require automated “removal” of undulators Routine replacement/measurement of undulators must be part of plan Operations troubleshooting needs attention

Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Diagnostics Workshop John N. Galayda, SLAC 7 Will the Undulator Diagnostics Serve Commissioning and Operations Needs for the LCLS? Charge – Will the Undulator Diagnostics Serve Commissioning and Operations Needs for the LCLS? Light diagnostics are crucial Can the Inter-undulator diagnostics survive at high power? No good solution for 800 eV If not, are we placing too heavy a reliance on data taken with low charge? Will optimization at low charge allow us to reach optimum at higher charge 40 cm looks very tight A lot of work required to develop inter-undulator diagnostics Inter-undulaor diagnostics that work at all wavelengths are challenging Even at shorter wavelength, variable geometry of diagnostics is a mechanical challenge Rollaway undulators? How far must they move to be useful? Variable Gap would require a lot of R&D Light diagnostics are crucial Can the Inter-undulator diagnostics survive at high power? No good solution for 800 eV If not, are we placing too heavy a reliance on data taken with low charge? Will optimization at low charge allow us to reach optimum at higher charge 40 cm looks very tight A lot of work required to develop inter-undulator diagnostics Inter-undulaor diagnostics that work at all wavelengths are challenging Even at shorter wavelength, variable geometry of diagnostics is a mechanical challenge Rollaway undulators? How far must they move to be useful? Variable Gap would require a lot of R&D

Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Diagnostics Workshop John N. Galayda, SLAC 8 Will the Undulator Diagnostics Serve Commissioning and Operations Needs for the LCLS? Charge – Will the Undulator Diagnostics Serve Commissioning and Operations Needs for the LCLS? Do we have redundant diagnostics capability where appropriate? Diagnostics that check the diagnostics We are heavily dependent on FEE diagnostics I don’t see much redundancy yet FEL/Spont is very bad for the 0.15nm case Nothing to tune on in the first 40 meters What is the smallest PROJECTED energy spread we can produce at any (lower) charge? Can spontaneous radiation serve as our diagnostic? Do we need a hi-res monochromator on day 1? Do we have redundant diagnostics capability where appropriate? Diagnostics that check the diagnostics We are heavily dependent on FEE diagnostics I don’t see much redundancy yet FEL/Spont is very bad for the 0.15nm case Nothing to tune on in the first 40 meters What is the smallest PROJECTED energy spread we can produce at any (lower) charge? Can spontaneous radiation serve as our diagnostic? Do we need a hi-res monochromator on day 1?

Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Diagnostics Workshop John N. Galayda, SLAC 9 Conclusions Gain versus z can be measured by turning off gain with an orbit kink In early commissioning there may be no measurable gain signal for meters when attempting to lase at 0.15 nm energy resolution is a must, to get rid of spontaneous Gain versus z can be measured by turning off gain with an orbit kink In early commissioning there may be no measurable gain signal for meters when attempting to lase at 0.15 nm energy resolution is a must, to get rid of spontaneous

Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Diagnostics Workshop John N. Galayda, SLAC 10 Issues to be Addressed It is important to estimate how many gain lengths needed to produce a gain signal above spontaneous background ~10 -3 energy resolution is a must, to get rid of spontaneous investigate whether spontaneous radiation become a diagnostic for undulator alignment and quality Investigate whether roll-away undulators provide a useful degree of freedom for diagnosing problems in commissioning or operations It is important to estimate how many gain lengths needed to produce a gain signal above spontaneous background ~10 -3 energy resolution is a must, to get rid of spontaneous investigate whether spontaneous radiation become a diagnostic for undulator alignment and quality Investigate whether roll-away undulators provide a useful degree of freedom for diagnosing problems in commissioning or operations

Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Diagnostics Workshop John N. Galayda, SLAC 11 Point of No Return

Wrap-up 20 January 2004 Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center LCLS Undulator Diagnostics Workshop John N. Galayda, SLAC 12 End of Presentation