Comments from LCLS FAC Meeting (April 2004): J. Rößbach:“How do you detect weak FEL power when the gain is very low (few hundred)?” K. Robinson:“Can you.

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

BC System – Review Options ● BC2 working point (energy-charge-compr.) ● 2BC (rf-rf-bc-rf-bc-rf) ● table: 2BC (rf-rf-bc-rf-bc-rf) dogleg + 2BC (rf-dog-rf-rf-bc-rf-bc-rf)
1 Bates XFEL Linac and Bunch Compressor Dynamics 1. Linac Layout and General Beam Parameter 2. Bunch Compressor –System Details (RF, Magnet Chicane) –Linear.
CALCULATIONS OF THE LCLS INJECTOR USING ASTRA Jean-Paul Carneiro DESY Hamburg ICFA Future Light Sources Sub-Panel Mini Workshop on Start-to-End Simulations.
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.
Juhao Wu Feedback & Oct. 12 – 13, 2004 Juhao Wu Stanford Linear Accelerator Center LCLS Longitudinal Feedback with CSR as Diagnostic.
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 FAC Meeting - April 29, 2004 Linac Physics, Diagnostics, and Commissioning Strategy P. Emma LCLS FAC Meeting April 29, 2004 LCLS.
Feedback and CSR Miniworkshop on XFEL Short Bunch, SLAC, July 26 – 30, 2004 Juhao Wu, SLAC 1 Juhao Wu Stanford Linear Accelerator.
Z. Huang LCLS FAC April Effect of AC RW Wake on SASE - Analytical Treatment Z. Huang, G. Stupakov see SLAC-PUB-10863, to.
Paul Emma LCLS Commissioning Status Nov. 11, 2008 SLAC National Accelerator Laboratory 1 LCLS Commissioning Status P. Emma for The.
C.Limborg-Deprey Beam Dynamics Justifying L01 November 3 rd 2004 Beam Dynamics Justifications of modification of.
Feedback and CSR Miniworkshop on XFEL Short Bunch, SLAC, July 26 – 30, 2004 Juhao Wu, SLAC 1 Juhao Wu Stanford Linear Accelerator.
E. Bong, SLACLCLS FAC Meeting - April 29, 2004 Linac Overview E. Bong LCLS FAC Meeting April 29, 2004 LCLS.
LCLS Transition to Science DOE Status Review of the LUSI MIE Project Near term opportunities for LCLS 'upgrades' J. Hastings for the LCLS Experimental.
P. Emma, SLACICFA XFEL July 29, 2004 Electron Bunch Measurements with a Transverse RF Deflector P. Emma ICFA XFEL 2004 Workshop July 29, 2004 ICFA.
David H. Dowell Injector Physics/Diagnostics/Gun&L0 RF April 29-30, 2004 Injector Physics / Diagnostics / Gun & L0 Linac.
LCLS-II Transverse Tolerances Tor Raubenheimer May 29, 2013.
Longitudinal Space Charge in LCLS S2E Z. Huang, M. Borland, P. Emma, J.H. Wu SLAC and Argonne Berlin S2E Workshop 8/21/2003.
TTF2 Start-to-End Simulations Jean-Paul Carneiro DESY Hamburg TESLA COLLABORATION MEETING DESY Zeuthen, 22 Jan 2004.
S2E in LCLS Linac M. Borland, Lyncean Technologies, P. Emma, C. Limborg, SLAC.
SPPS, Beam stability and pulse-to-pulse jitter Patrick Krejcik For the SPPS collaboration Zeuthen Workshop on Start-to-End Simulations of X-ray FEL’s August.
LCLS Accelerator SLAC linac tunnel research yard Linac-0 L =6 m Linac-1 L  9 m  rf   25° Linac-2 L  330 m  rf   41° Linac-3 L  550 m  rf  0°
Two Longitudinal Space Charge Amplifiers and a Poisson Solver for Periodic Micro Structures Longitudinal Space Charge Amplifier 1: Longitudinal Space Charge.
Simulation of Microbunching Instability in LCLS with Laser-Heater Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory.
FLASH II. The results from FLASH II tests Sven Ackermann FEL seminar Hamburg, April 23 th, 2013.
SFLASH  SASE interference setup & optics rough estimation 1d estimation 3d estimation summary.
A bunch compressor design and several X-band FELs Yipeng Sun, ARD/SLAC , LCLS-II meeting.
J. Wu J. Wu working with T.O. Raubenheimer, J. Qiang (LBL), LCLS-II Accelerator Physics meeting April 11, 2012 Study on the BC1 Energy Set Point LCLS-II.
P. Krejcik LINAC 2004 – Lübeck, August 16-20, 2004 LCLS - Accelerator System Overview Patrick Krejcik on behalf of the LCLS.
‘S2E’ Study of Linac for TESLA XFEL P. Emma SLAC  Tracking  Comparison to LCLS  Re-optimization  Tolerances  Jitter  CSR Effects.
Design Considerations of table-top FELs laser-plasma accelerators principal possibility of table-top FELs possible VUV and X-ray scenarios new experimental.
LCLS Energy Jitter Status in 2012 Franz-Josef Decker 24-Oct-2012 thanks to: J. Turner, R. Akre, J. Craft, A. Krasnykh, M. Nguyen, W. Colocho, … for helping.
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.
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.
Injector Requirements Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile.
Microbunching Instability and Slice Energy Spread
PAL-XFEL Commissioning Plan ver. 1.1, August 2015 PAL-XFEL Beam Dynamics Group.
Applications of transverse deflecting cavities in x-ray free-electron lasers Yuantao Ding SLAC National Accelerator Laboratory7/18/2012.
LSC/CSR Instability Introduction (origin of the instability) CSR/LSC
A 6 GeV Compact X-ray FEL (CXFEL) Driven by an X-Band Linac
Beam dynamics for an X-band LINAC driving a 1 keV FEL
Cutting Beam Horns in BC1
Short pulse, low charge LCLS operation
Timing and synchronization at SPARC
XFEL Beam Physics 10/30/2015 Tor Raubenheimer.
Revised Commissioning Strategy
BC2 Commissioning Parameters
Review of Application to SASE-FELs
LCLS Commissioning Parameters
LCLS Commissioning Parameters
LCLS Longitudinal Feedback and Stability Requirements
Simulation Calculations
LCLS Commissioning Parameters
Z. Huang LCLS Lehman Review May 14, 2009
Two-bunch self-seeding for narrow-bandwidth hard x-ray FELs
Linac/BC1 Commissioning P
Design of Compression and Acceleration Systems Technical Challenges
Modified Beam Parameter Range
Gain Computation Sven Reiche, UCLA April 24, 2002
Linac Physics, Diagnostics, and Commissioning Strategy P
LCLS FEL Parameters Heinz-Dieter Nuhn, SLAC / SSRL April 23, 2002
LCLS Commissioning Parameters
Introduction to Free Electron Lasers Zhirong Huang
Linac Design Update P. Emma LCLS DOE Review May 11, 2005 LCLS.
setups 7 (low E1) 4 modules 3rd h. L = 8m 12 modules rf = 20 deg
Electron Optics & Bunch Compression
Presentation transcript:

Comments from LCLS FAC Meeting (April 2004): J. Rößbach:“How do you detect weak FEL power when the gain is very low (few hundred)?” K. Robinson:“Can you modulate the laser heater in some way to help FEL signal detection?” Comments from LCLS FAC Meeting (April 2004): J. Rößbach:“How do you detect weak FEL power when the gain is very low (few hundred)?” K. Robinson:“Can you modulate the laser heater in some way to help FEL signal detection?” Laser-Heater Modulation P. Emma, Z. Huang, J. Wu

modulate laser power (1.2 to 19 7 Hz) Kem Robinson idea… modulated slice energy spread (0.01% to 0.04% rms at 14 GeV) laser heater Laser Heater at 135 MeV

Simulate LCLS (Linac + M. Xie) with linac jitter, large emittance (3  m), spontaneous radiation background, and laser-heater modulated at 7 Hz (or other unique frequency << 120 Hz) 1.5-Å LCLS, except  x,y = 3  m 2% rms charge jitter 0.5 ps rms gun-timing jitter 0.1-deg rms RF phase jitter (each of 4 linacs) 0.1% rms RF amplitude jitter (each of 4 linacs) 2% rms emittance jitter includes small emittance growth in laser-heater 100-MW spontaneous power (1% BW cut)* 10% rms radiation energy measurement noise fast, accurate 2 nd -order linac model in Matlab, with jitter * Sven Reiche says 10-MW at 1% BW cut (allows a 3.5-  m emittance)

Effects of Linac Jitter bunch length energy spread peak current e  relative energy bunch arrival time

P < P sat : P > P sat : 1-D startup power: Use ‘Ming Xie’ model to calculate gain length, L g, then calculate power as: Assume 1% BW cut to get 100-MW spontaneous power (none)

Red:Total power + meas. noise Magenta:Spontaneous power Green:FEL power  Gain   230

14.7 ± 4.1 m ± %  x,y = 3.0  m 4.2 ± 0.6 kA 0 ± % 1.0 ± 0.02 nC 21 ± 3.0  m

7 Hz FFT of total power + noise  Gain   230 Get similar result if P spont = 10 MW and  x,y = 3.5  m