Results from measurement and simulation methods (LW, PIC, Astra) and setup About LW & Astra Simulations of The Pitz Gun comparison LW  Astra more analysis.

Slides:



Advertisements
Similar presentations
Contour plots of electron density 2D PIC in units of  [n |e|] cr wake wave breaking accelerating field laser pulse Blue:electron density green: laser.
Advertisements

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.
First operation of the TTF2 injector with beam Jean-Paul Carneiro DESY Hamburg TESLA COLLABORATION MEETING DESY Hamburg, 16 Sept 2003.
Particle-Driven Plasma Wakefield Acceleration James Holloway University College London, London, UK PhD Supervisors: Professor Matthew wing University College.
Synchrotron Radiation What is it ? Rate of energy loss Longitudinal damping Transverse damping Quantum fluctuations Wigglers Rende Steerenberg (BE/OP)
Reduced Gun Simulations 1. Comparison 60MV/m Gun vs 50MV/m Gun, Flat Top Laser Pulse 2. Comparison for the worst case: Gun50+Gauss Laser Pulse 3. Summary.
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.
SPACE CHARGE EFFECTS IN PHOTO-INJECTORS Massimo Ferrario INFN-LNF Madison, June 28 - July 2.
Cecile Limborg-Deprey Injector Commissioning September Injector Commissioning Plans C.Limborg-Deprey Gun exit measurements.
Simulation studies of the e-beams for Renkai Li and Juhao Wu 5/20/2014 ALD Review.
2 Lasers: Centimeters instead of Kilometers ? If we take a Petawatt laser pulse, I=10 21 W/cm 2 then the electric field is as high as E=10 14 eV/m=100.
Magnetic Compression of High Brightness Beams: Survey of Experimental Results Scott G. Anderson ICFA Sardinia July 2002.
Carbon Injector for FFAG
Modelling of the ALICE Injector Julian McKenzie ASTeC STFC Daresbury Laboratory IOP Particle Accelerators and Beams Group Status and Challenges of Simulation.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, N.Kazarinov.
FEL simulation code FAST Free-Electron Laser at the TESLA Test Facility Generic name FAST stands for a set of codes for ``full physics'' analysis of FEL.
Photocathode 1.5 (1, 3.5) cell superconducting RF gun with electric and magnetic RF focusing Transversal normalized rms emittance (no thermal emittance)
I.V. Bazarov, Multivariate Optimization of High Brightness DC Gun Photoinjector, UCLA Workshop, 8-10 November CHESS / LEPP ERL DC Gun Injector.
Astra A Space Charge Tracking Algorithm
1nC 10ps square pulse, 1 mm uniform transverse laser pulse No Thermal emittance 110MV/m Solenoid kG 1nC 10ps square pulse, 1 mm uniform transverse.
TTF2 Start-to-End Simulations Jean-Paul Carneiro DESY Hamburg TESLA COLLABORATION MEETING DESY Zeuthen, 22 Jan 2004.
IRPSS: A Green’s Function Approach to Modeling Photoinjectors Mark Hess Indiana University Cyclotron Facility & Physics Department *Supported by NSF and.
ASTRA Injector Setup 2012 Julian McKenzie 17/02/2012.
Yauhen Kot Current Status of XFEL Simulations.
Recent Experiments at PITZ ICFA Future Light Sources Sub-Panel Mini Workshop on Start-to-End Simulations of X-RAY FELs August 18-22, 2003 at DESY-Zeuthen,
Two Longitudinal Space Charge Amplifiers and a Poisson Solver for Periodic Micro Structures Longitudinal Space Charge Amplifier 1: Longitudinal Space Charge.
Simulation of Beam Instabilities in SPring-8 T. Nakamura JASRI / SPring-8
Simulation of Microbunching Instability in LCLS with Laser-Heater Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory.
FCC electron cloud study plan K. Ohmi (KEK) Mar FCC electron cloud study meeting CERN.
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.
K. Floettmann30 th Nov XFEL Injector matching The present XFEL injector foresees operation of the first four cavities of the first module to operate.
Optics considerations for ERL test facilities Bruno Muratori ASTeC Daresbury Laboratory (M. Bowler, C. Gerth, F. Hannon, H. Owen, B. Shepherd, S. Smith,
IMPACT-T - A 3D Parallel Beam Dynamics Code for Modeling High Brightness Beams in Photo-Injectors Ji Qiang Lawrence Berkeley National Laboratory Work performed.
1D-FEL Without Approximations motivation, capabilities 1D theory  1D-solver for waves implementation (without and with Lorentz transformation) excitation.
Midwest Accelerator Physics Meeting. Indiana University, March 15-19, ORBIT Electron Cloud Model Andrei Shishlo, Yoichi Sato, Slava Danilov, Jeff.
GWENAEL FUBIANI L’OASIS GROUP, LBNL 6D Space charge estimates for dense electron bunches in vacuum W.P. LEEMANS, E. ESAREY, B.A. SHADWICK, J. QIANG, G.
3D codes: TraFiC4 and CSRtrack Torsten Limberg DESY Zeuthen 2003.
Change in Program Tuesday Morning Review of 2002 CSR Workshop (T. Limberg, 20 min) CSR calculation Models (M. Dohlus, 40 min) The 3D Codes TraFiC4 and.
D. Lipka, V. Vogel, DESY Hamburg, Germany, Oct Optimization cathode design with gun5 D. Lipka, V. Vogel, DESY Hamburg, Germany.
P I T Z Photo Injector Test Facility Zeuthen Design consideration of the RF deflector to optimize the photo injector at PITZ S.Korepanov.
S2E (start-to-end) Simulations at DESY T. Limberg TESLA Collaboration Meeting in Frascati, May 2003.
S. Bettoni, R. Corsini, A. Vivoli (CERN) CLIC drive beam injector design.
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 (
Warm linac simulations (DTL) and errors analysis M. Comunian F. Grespan.
LCLS-II Injector layout design and study Feng Zhou 8/19/2015.
ELI PHOTOINJECTOR PARAMETERS: PRELIMINARY ANALYSIS AND SIMULATIONS C. RONSIVALLE.
LSC/CSR Instability Introduction (origin of the instability) CSR/LSC
Seeding in the presence of microbunching
S.M. Polozov & Ko., NRNU MEPhI
Gun Calculations by Poisson Model for Non-Uniform Distributions
Beam dynamics for an X-band LINAC driving a 1 keV FEL
Calculation of Beam Equilibrium and Luminosities for
Jeffrey Eldred, Sasha Valishev
F. Villa Laboratori Nazionali di Frascati - LNF On behalf of Sparc_lab
Injector: What is needed to improve the beam quality?
calculation with 107 particles
Simulation Calculations
Selected simulations for XFEL photo injector
Modified Beam Parameter Range
Gain Computation Sven Reiche, UCLA April 24, 2002
Injector Experimental Results John Schmerge, SSRL/SLAC April 24, 2002
Simulations for the LCLS Photo-Injector C
Thermal Emittance Measurement at PITZ
New VUV-FEL Simulation results
Injector for the Electron Cooler
Update on ERL Cooler Design Studies
Presentation transcript:

results from measurement and simulation methods (LW, PIC, Astra) and setup About LW & Astra Simulations of The Pitz Gun comparison LW  Astra more analysis of LW results about Astra results: sensitivity to numerical parameters about approaches: some analytical calculations second inspection summary

results from measurement and simulation see: DESY/TEMF Meeting - Status

methods (LW, PIC, Astra) and setup LW = Lienard Wichert exact solution of Maxwell problem (based on retarded trajectory) no spatial mesh numeric integration of EoM; fixed time step higher order PIC ; PIC = particle in cell exact numerical approach for Maxwell problem spatial mesh & time step numeric integration of EoM; fixed time step extensive convergence test in 2010 carefull comparison in 2011  simulation of PITZ injector for z <= 5 cm Astra approximation based on uniform motion rz - Poisson approach; spatial mesh numeric integration of EoM; variable time step

methods (LW, PIC, Astra) and setup setup bunch charge = 1 nC bunch length = 21.5 psec (Lt= rt=0.002) rms-radius = (radius/2) = 0.2 … 0.6 mm MaxE = MV/m phi = deg (or auto phase = deg)  E0 = 41.6 MV/m estimated SC limitation (DC field and planar diode) R rms /mm = Q SC-limit /nC =

comparison LW  Astra

rms laser spot size = 0.6 mm, slice properties LW Astra see also: s2e-seminar 2011-Feb-07 (z-mean(z))/m norm. (hor;vert) emittance / m c 0 p z / eVrms{c 0 p z }/ eV (z-mean(z))/m

comparison LW  Astra rms laser spot size = 0.6 mm

comparison LW  Astra rms laser spot size = 0.6 mm

comparison LW  Astra rms laser spot size = 0.4 mm

comparison LW  Astra rms laser spot size = 0.3 mm

comparison LW  Astra rms laser spot size = 0.2 mm

more analysis of LW results

rms laser spot size = 0.6 mm r/m z/m

more analysis of LW results rms laser spot size = 0.5 mm r/m z/m

more analysis of LW results rms laser spot size = 0.4 mm r/m z/m

more analysis of LW results rms laser spot size = 0.3 mm (0.5MP; dt=0.1psec) r/m z/m aliasing

more analysis of LW results rms laser spot size = 0.2 mm r/m z/m

more analysis of LW results micro modulation 0.2mm; 0.3mm; 0.4mm; 0.5mm; 0.6mm; r/m z/m

more analysis of LW results rms laser spot size = 0.3 mm simulation with more particles 0.5M 1M r/m z/m

more analysis of LW results rms laser spot size = 0.3 mm; calc. with different time step 0.2mm/9 =22.2um; pz 1mm/24=42um; dt = 0.10 psec dt = 0.05 psec r/m z/m

 this bunch needs more compression ! r/m z/m 0.6 mm 0.5 mm 0.4 mm 0.3 mm 0.2 mm “micro bunching” vs. injection time color frequency = 2x 0.1psec 0.3 mm, half time step  dt = 0.10 psec  dt = 0.05 psec more analysis of LW results

0.2 mm, = 10 mm r/m z/m 0.3 mm, = 10 mm0.6 mm, = 10 mm = 20 mm = 30 mm = 40 mm = 50 mm 50 mm more analysis of LW results different longitudinal position

more analysis of LW results rms laser spot size = 0.3 mm; slice properties 500k, 0.1psec (z-mean(z))/m norm. (hor;vert) emittance / m c 0 p z / eVrms{c 0 p z }/ eV (z-mean(z))/m

more analysis of LW results rms laser spot size = 0.3 mm; slice properties 1M, 0.1psec (z-mean(z))/m norm. (hor;vert) emittance / m c 0 p z / eVrms{c 0 p z }/ eV (z-mean(z))/m

more analysis of LW results rms laser spot size = 0.3 mm; slice properties 500k, 0.05psec (z-mean(z))/m norm. (hor;vert) emittance / m c 0 p z / eVrms{c 0 p z }/ eV (z-mean(z))/m

about Astra results

rms laser spot size = 0.6 mm no SC limitation is it possible to provoke numerical microbunching? (fine mesh, big time step) about Astra results: sensitivity to numerical parameters Hammersley  random mesh lines time step rms laser spot size = 0.2 mm strong SC limitation: late emission is pulsing no: Astra is too clever; during emission it does not use the user defined time step

rms laser spot size = 0.2 mm strong SC limitation: late emission is pulsing emitted particles 40.5% pitzTT 100x40 pitzTT 100x40 r/m z/m about Astra results: sensitivity to numerical parameters N z  N r

Hammersley emitted particles 40.5% pitzTT 100x40 pitzN 100x40 random emitted particles 40.5% pulsing (multiple fronts) is no artifact of pseudo random gen. r/m z/m about Astra results: sensitivity to numerical parameters rms laser spot size = 0.2 mm strong SC limitation: late emission is pulsing

Hammersley emitted particles 41.9% pitzTF 200x40 pitzTFF 1000x40 Hammersley emitted particles 45.4% r/m z/m about Astra results: sensitivity to numerical parameters rms laser spot size = 0.2 mm strong SC limitation: late emission is pulsing N z  N r

pitzTTfixed 100x40 Hammersley emitted particles 39.1% Hammersley emitted particles 40.5% pitzTT 100x40 not quite the same time r/m z/m about Astra results: sensitivity to numerical parameters rms laser spot size = 0.2 mm strong SC limitation: late emission is pulsing N z  N r

still running: pitzTFFF, 10000x40 pitzTFFR, 1000x200 pitzTFFF pitzTFFR 1000x200 r/m z/m about Astra results: sensitivity to numerical parameters rms laser spot size = 0.2 mm strong SC limitation: late emission is pulsing pitzTFF 1000x %  45.4% 43.2%

about Astra results: sensitivity to numerical parameters pitzTFFF 10000x40 r/m z/m q/Q z/m 10 mesh lines q/Q = 0.05

about Astra results: sensitivity to numerical parameters result is extremely sensitive on initial conditions and both mesh settings no initial energy spread caused by r-mesh 0.55eV initial energy spread

about approaches

about approaches: some analytical calculations the planar diode a three dimensional driven problem exact solution of Maxwell problem no explicit appearance of retarded time exact solution of EoM with = slice index, t = ejection time of slice, in the following: three different approaches to calculate comparison for external field,

about approaches: some analytical calculations three approaches “M” exact Maxwell solution “BUM” solution: bunch in uniform motion “SUM” solution: slices in individual uniform motion with and “com” = center of mass with and z(v,t) the slice velocity

about approaches: some analytical calculations injection ( z = 0 ) bunch charge accelerating field time of injection (rectangular) (rms = 0.5 mm) … planar diode __ SUM __ BUM x_ M (rms = 0.3 mm) space charge limitation

space charge limitation … planar diode __ SUM __ BUM x_ M about approaches: some analytical calculations injection ( z = 0 ) (rms = 0.2 mm) M calculates stronger field reduction than UM & BUM !

… planar diode __ SUM __ BUM __ M about approaches: some analytical calculations after injection ( t > T i ) bunch charge accelerating field time of injection (rectangular) (rms = 0.5 mm)

… planar diode __ SUM __ BUM __ M about approaches: some analytical calculations after injection ( t > T i )

second inspection

injection time / sec   injection radius / m lost particles vs. accelerated particles injection) integrated charge accelerated particles lost particles integrated charge accelerated particles lost particles injection time / sec  0.2mm: ASTRA, lost particles = blue injection time / sec   injection radius / m pitzTT 100x40

second inspection lost particles vs. accelerated particles injection) integrated charge accelerated particles lost particles injection time / sec  0.2mm: ASTRA, lost particles = blue injection time / sec   injection radius / m pitzTT 100x40 pitzTT 10000x40 not calc.

second inspection injection time / sec   injection radius / m lost particles vs. accelerated particles injection) integrated charge accelerated particles lost particles injection time / sec  pitzTT 100x40

second inspection 0.2mm: ASTRA, lost particles = blue  injection radius / m pitzTT 100x40 injection time / sec   injection radius / m … planar diode __ SUM __ BUM x_ M (rms = 0.2 mm) correct numbers: q = 1nC Ti = 21.5 psec Eacc=41.61 MV/m M-shielding should be stronger than BUM-shielding!

summary SC limited emission: differences between measurement and ASTRA ASTRA incomplete model predicts strong SC limited emission SC limited emissions needs extreme mesh resolution (usually not fulfilled at end of emission) very sensitive to initial conditions (is it real physics?) SC shielding seems to agree with analytical model LW should include all effects has been benchmarked with PIC or vice versa (but: same tracker) less SC shielding: seems to agree with measurement problems with boundary condition at injection (mirror-point-charge) micro modulation: related to time step and time of injection analytical model (Maxwell  Poisson) predicts stronger shielding measurement …?!