calculation with 107 particles

Slides:



Advertisements
Similar presentations
Two-dimensional Effects on the CSR Interaction Forces for an Energy-Chirped Bunch Rui Li, J. Bisognano, R. Legg, and R. Bosch.
Advertisements

Paul Emma SLAC January 14, 2002 BERLIN CSR Benchmark Test-Case Results CSR Workshop.
J. Rudolph, Helmholtz-Zentrum Berlin EuCARD 2nd ANNUAL MEETING Slice emittance measurements at the ELBE superconducting RF photoinjector.
Cavity Field Maps (TESLA & 3 rd Harmonic Cavity) Undulator Wakes Estimation of CSR Effects for FLASH2HGHG.
1 Bates XFEL Linac and Bunch Compressor Dynamics 1. Linac Layout and General Beam Parameter 2. Bunch Compressor –System Details (RF, Magnet Chicane) –Linear.
05/03/2004 Measurement of Bunch Length Using Spectral Analysis of Incoherent Fluctuations Vadim Sajaev Advanced Photon Source Argonne National Laboratory.
First operation of the TTF2 injector with beam Jean-Paul Carneiro DESY Hamburg TESLA COLLABORATION MEETING DESY Hamburg, 16 Sept 2003.
SPACE CHARGE EFFECTS IN PHOTO-INJECTORS Massimo Ferrario INFN-LNF Madison, June 28 - July 2.
Chris Rogers, MICE CM16 Wednesday Plenary Progress in Cooling Channel Simulation.
SIMULATION PROGRESS AND PLANS AT ROSTOCK/DESY Aleksandar Markovic ECL2, CERN, March 1, 2007 Gisela Pöplau.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, N.Kazarinov.
07/27/2004XFEL 2004 Measurement of Incoherent Radiation Fluctuations and Bunch Profile Recovery Vadim Sajaev Advanced Photon Source Argonne National Laboratory.
Astra A Space Charge Tracking Algorithm
TTF2 Start-to-End Simulations Jean-Paul Carneiro DESY Hamburg TESLA COLLABORATION MEETING DESY Zeuthen, 22 Jan 2004.
ASTRA Injector Setup 2012 Julian McKenzie 17/02/2012.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, A.Drozhdin, N.Kazarinov.
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.
Beam Modulation due to Longitudinal Space Charge Zhirong Huang, SLAC Berlin S2E Workshop 8/18/2003.
Beam Dynamics and FEL Simulations for FLASH Igor Zagorodnov and Martin Dohlus Beam Dynamics Meeting, DESY.
SFLASH  SASE interference setup & optics rough estimation 1d estimation 3d estimation summary.
Optics with SC horizontal vertical BC0BC1BC2 XFEL, design optics.
A bunch compressor design and several X-band FELs Yipeng Sun, ARD/SLAC , LCLS-II meeting.
Optics considerations for ERL test facilities Bruno Muratori ASTeC Daresbury Laboratory (M. Bowler, C. Gerth, F. Hannon, H. Owen, B. Shepherd, S. Smith,
Beam Dynamics Meeting Bolko Beutner, DESY Summary of new FLASH CSR studies Bolko Beutner, DESY Beam Dynamics Meeting
XFEL Beam Dynamics Meeting Bolko Beutner, DESY Velocity Bunching Studies at FLASH Bolko Beutner, DESY XFEL Beam Dynamics 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.
‘S2E’ Study of Linac for TESLA XFEL P. Emma SLAC  Tracking  Comparison to LCLS  Re-optimization  Tolerances  Jitter  CSR Effects.
The Microbunching Instability in the LCLS-II Linac LCLS-II Planning Meeting October 23, 2013 A. Marinelli and Z. Huang.
Status of the Simulations on Photo Injector Optimization for Low Charges Yauhen Kot BD Meeting,
Awake electron beam requirements ParameterBaseline Phase 2Range to check Beam Energy16 MeV MeV Energy spread (  ) 0.5 %< 0.5 % ? Bunch Length (
Injector Requirements Linac Coherent Light Source Stanford Linear Accelerator Center Technical Review, March 1st, 2004 Cécile.
Microbunching Instability and Slice Energy Spread
B. Marchetti R. Assmann, U. Dorda, J. Grebenyuk, Y. Nie, J. Zhu Acknowledgements: C. Behrens, R. Brinkmann, K. Flöttmann, M. Hüning,
Operated by JSA for the U.S. Department of Energy Thomas Jefferson National Accelerator Facility Alex Bogacz NuFact’08, Valencia, Spain, July 4, 2008 Acceleration.
DEC  x / m  y / m quads undulators vertical correctors chicane 1chicane 2chicane 3.
LSC/CSR Instability Introduction (origin of the instability) CSR/LSC
S.M. Polozov & Ko., NRNU MEPhI
Multi-bunch Operation for LCLS, LCLS_II, LCLS_2025
Gun Calculations by Poisson Model for Non-Uniform Distributions
Electron Cooling Simulation For JLEIC
Beam-beam effects in eRHIC and MeRHIC
Tunable Electron Bunch Train Generation at Tsinghua University
UCLA/ATF chicane compression experiments
Review of Application to SASE-FELs
F. Villa Laboratori Nazionali di Frascati - LNF On behalf of Sparc_lab
CSR Benchmark Test-Case Results
Capture and Transmission of polarized positrons from a Compton Scheme
LCLS Longitudinal Feedback and Stability Requirements
G. Marcus, Y. Ding, J. Qiang 02/06/2017
Soft X-Ray pulse length measurement
Simulation Calculations
Superconducting High Brightness RF Photoinjector Design
UCLA/ATF chicane compression experiments
Two-bunch self-seeding for narrow-bandwidth hard x-ray FELs
Selected simulations for XFEL photo injector
SASE FEL PULSE DURATION ANALYSIS FROM SPECTRAL CORRELATION FUNCTION
Simulating transition crossing in the PS with HeadTail
LCLS Tracking Studies CSR micro-bunching in compressors
Modified Beam Parameter Range
Laser Heater Integration into XFEL. Update.
Gain Computation Sven Reiche, UCLA April 24, 2002
Injector Experimental Results John Schmerge, SSRL/SLAC April 24, 2002
Longitudinal Space Charge Instability C. Limborg-Déprey, Z. Huang, J
Coupler Effects in High Energy Part of XFEL Linac
Bunch Compression Experiment in VUV-FEL BC3
some tools for longitudinal phase space
Electron Optics & Bunch Compression
New VUV-FEL Simulation results
Injector for the Electron Cooler
Presentation transcript:

calculation with 107 particles Astra bunch 0.4 nC, at z=1.45 m bunch current calculation with 107 particles “slice 1” (~1keV energy spread, I=17.6 A) slice energy “slice 2” (small energy spread, I=13.1 A) slice energy spread

compression: 17.6A --> 110A --> 1200A “slice 2” ~1keV energy spread, I=17.6 A 0.3mm, about 110E6 particles compression: 17.6A --> 110A --> 1200A “slice 2” ~250eV energy spread, I=13.1 A 0.3mm, about 82E6 particles compression: 13.1A --> 85.5A --> 944A

 1D model starting after gun (z=0.5m) slicing and densification: criticism: this introduces new noise as it ignores relaxation effects (due to plasma oscillations)  1D model starting after gun (z=0.5m) Astra distribution with 10E6 particles, but 0.4 nC /e = 2.5E9 we need 250 particles per Astra-particles procedure: select all particles in the given slice, extract correlations with z (to 3rd order) keep information about linear z-energy correlation throw away z-information multiply (replicate x 250) and mix the 5D-distribution use random generator for z-coordinates regenerate linear z-energy correlation full shot noise simulation with Xtrack starts after solenoid field (z=1.45 m)

Xtrack simulations “slice 1” (~1keV energy spread, 110E6 particles) compression: 17.6A --> 110A --> 1200A “slice 2” (~250eV energy spread, 82E6 particles) compression: 13.1A --> 85.5A --> 944A

long. position and energy “slice 1” (~1keV energy spread, 110E6 particles) compression: 17.6A --> 110A --> 1200A long. position and energy after BC2 after ACC2 before BC3 energy /eV long. phase space (full period) bunch coordinate / m E,tot  13.5 kEV E  9.6 kEV long. p.s. without z-correlation plasma oscillation long. density

“slice 1” (~1keV energy spread, 110E6 particles) compression: 17 “slice 1” (~1keV energy spread, 110E6 particles) compression: 17.6A --> 110A --> 1200A after BC3 before F2kicker after F2seed chicane E  127 kEV Flash2 E  1.3 MeV I  70 A I  600 A

1d-models 1d-particles (non-linear, real noise) effective impedance (long. impedance transversely averaged) tracking from 0.4m (direct after gun) to 150m (before Flash1/Flash2) 1d-particles (non-linear, real noise) longer sample (~ 1.1mm) distribution from random generator very high bandwidth LGM (linear gain model) frequency domain integral equation

random generator: uniform in z, gaussian in energy 1d particles random generator: uniform in z, gaussian in energy “slice 1” ~1keV energy spread, I=17.6 A 400E6 particles, about 1.1 mm compression: 17.6A --> 110A --> 1200A “slice 2” ~250eV energy spread, I=13.1 A 398E6 particles, about 1.1 mm compression: 13.1A --> 85.5A --> 944A distribution at z =150 m 7 m  500 m/Ctot 3 m  200 m/Ctot bunch coordinate / m bunch coordinate / m slice rms  250 keV total rms  1.2 MeV slice rms  120 keV total rms  0.6 MeV

“slice 1”, compression: 17.6A --> 110A --> 1200A BC2 BC3 127 keV beamline coordinate / m beamline coordinate / m log scale log scale “slice 2”, compression: 13.1A --> 85.5A --> 944A 3D particle tracking 253 keV log scale log scale

spectra: comparison 1d particles, LGM “slice 1” start direct before BC2 “slice 2”  = 30 m  = 30 m /mm  1.5 /mm  0.15 effect of plasma oscillations these oscillations are frozen in ACC1 yes: original white noise is reduced (in some spectral ranges)

? spectra: comparison 1d particles, LGM “slice 1” direct after BC2 direct before BC3 “slice 2”  = 30 m  = 30 m ? unexpected growth of energy spread  needs further investigations

spectra: comparison 1d particles, LGM “slice 1” direct after BC3 at 150m “slice 2”  = 30 m  = 30 m huge disagreement due to strong non-linear effects even for “slice 1”, but this is not very obvious from the plot

energy spread versus initial energy spread “slice 1” “slice 2” but with slightly different optic but for 1.2 GeV log scale log scale C3 “heating” C2 conservation of phase space

rms current fluctuations spread versus initial energy spread “slice 1” “slice 2” but with slightly different optic but for 1.2 GeV log scale log scale

ACC1, slice E-spread q = 1nC, Xtrack cavity amplitudes = [1.00,1.00,1.00,1.00, 1.00,1.00,1.00,1.00] case 100,100 [0.75,0.75,0.75,0.75, 1.25,1.25,1.25,1.25] case 75,125

optics with matching: horizontal/vertical solid: case 100,100 dashed: case 75,125

at 19.8m (after ACC39), with matching slice energy spread after ACC1 at 19.8m (after ACC39), with matching

“slice 2” (~250eV energy spread, 82E6 particles) compression: 13 “slice 2” (~250eV energy spread, 82E6 particles) compression: 13.1A --> 85.5A --> 944A after BC2 after ACC2 before BC3 E,tot  23 kEV E  16.1 kEV plasma oscillation

“slice 2” (~250eV energy spread, 82E6 particles) compression: 13 “slice 2” (~250eV energy spread, 82E6 particles) compression: 13.1A --> 85.5A --> 944A after BC3 before F2kicker after F2seed chicane E  253 kEV Flash2 E  407 keV I  15 A I  139 A

plasma oscillations Sp  bunch coordinate LINAC coordinate  L / m charge density