Linac optimisation for the New Light Source

Similar documents
Linac Driven Free Electron Lasers (III)

LCLS-II SCRF start-to-end simulations and global optimization as of September Abstract

Generation and characterization of ultra-short electron and x-ray x pulses

PAL LINAC UPGRADE FOR A 1-3 Å XFEL

X-band RF driven hard X-ray FELs. Yipeng Sun ICFA Workshop on Future Light Sources March 5-9, 2012

4GLS Status. Susan L Smith ASTeC Daresbury Laboratory

LOLA: Past, present and future operation

Short Pulse, Low charge Operation of the LCLS. Josef Frisch for the LCLS Commissioning Team

S2E (Start-to-End) Simulations for PAL-FEL. Eun-San Kim

Expected properties of the radiation from VUV-FEL / femtosecond mode of operation / E.L. Saldin, E.A. Schneidmiller, M.V. Yurkov

4 FEL Physics. Technical Synopsis

Coherence Requirements for Various Seeding Schemes

FURTHER UNDERSTANDING THE LCLS INJECTOR EMITTANCE*

Linac Based Photon Sources: XFELS. Coherence Properties. J. B. Hastings. Stanford Linear Accelerator Center

Progress in Soft X-rays FELs

Femto-second FEL Generation with Very Low Charge at LCLS

X-ray Free-electron Lasers

Two-Stage Chirped-Beam SASE-FEL for High Power Femtosecond X-Ray Pulse Generation

Beam Dynamics and SASE Simulations for XFEL. Igor Zagorodnov DESY

Simulations of the IR/THz Options at PITZ (High-gain FEL and CTR)

ATTOSECOND X-RAY PULSES IN THE LCLS USING THE SLOTTED FOIL METHOD

Excitements and Challenges for Future Light Sources Based on X-Ray FELs

Excitements and Challenges for Future Light Sources Based on X-Ray FELs

Low slice emittance preservation during bunch compression

ASTRA simulations of the slice longitudinal momentum spread along the beamline for PITZ

FACET-II Design Update

CSR Benchmark Test-Case Results

Simulations of the IR/THz source at PITZ (SASE FEL and CTR)

Towards a Low Emittance X-ray FEL at PSI

X-band Experience at FEL

SwissFEL INJECTOR DESIGN: AN AUTOMATIC PROCEDURE

Length of beam system = 910m. S. Reiche X var = ~50m ~ 650m / Y. Kim FEL-KY ~150m. ~60m. LaserHutch2 (access during operation)

X-Band RF Harmonic Compensation for Linear Bunch Compression in the LCLS

Echo-Enabled Harmonic Generation

Parameter selection and longitudinal phase space simulation for a single stage X-band FEL driver at 250 MeV

Velocity Bunching Studies at FLASH. Bolko Beutner, DESY XFEL Beam Dynamics Meeting

Diagnostic Systems for Characterizing Electron Sources at the Photo Injector Test Facility at DESY, Zeuthen site

Beam Echo Effect for Generation of Short Wavelength Radiation

Microbunching Workshop 2010 March 24, 2010, Frascati, Italy. Zhirong Huang

Ultra-Short Low Charge Operation at FLASH and the European XFEL

R&D experiments at BNL to address the associated issues in the Cascading HGHG scheme

Free-electron laser SACLA and its basic. Yuji Otake, on behalf of the members of XFEL R&D division RIKEN SPring-8 Center

Update on and the Issue of Circularly-Polarized On-Axis Harmonics

A 6 GeV Compact X-ray FEL (CXFEL) Driven by an X-Band Linac

FEL SIMULATION AND PERFORMANCE STUDIES FOR LCLS-II

OPTIMIZATION OF COMPENSATION CHICANES IN THE LCLS-II BEAM DELIVERY SYSTEM

Simple limits on achieving a quasi-linear magnetic compression for an FEL driver

LCLS Commissioning Status

VARIABLE GAP UNDULATOR FOR KEV FREE ELECTRON LASER AT LINAC COHERENT LIGHT SOURCE

Femtosecond and sub-femtosecond x-ray pulses from a SASE-based free-electron laser. Abstract

CONCEPTUAL STUDY OF A SELF-SEEDING SCHEME AT FLASH2

Undulator radiation from electrons randomly distributed in a bunch

FACET-II Design, Parameters and Capabilities

Laser acceleration of electrons at Femilab/Nicadd photoinjector

Introduction. Thermoionic gun vs RF photo gun Magnetic compression vs Velocity bunching. Probe beam design options

Experimental Optimization of Electron Beams for Generating THz CTR and CDR with PITZ

LCLS Accelerator Parameters and Tolerances for Low Charge Operations

Layout of the HHG seeding experiment at FLASH

Simulations of the Microbunching Instability in FEL Beam Delivery Systems

SPARCLAB. Source For Plasma Accelerators and Radiation Compton. On behalf of SPARCLAB collaboration

OPERATING OF SXFEL IN A SINGLE STAGE HIGH GAIN HARMONIC GENERATION SCHEME

WG2 on ERL light sources CHESS & LEPP

Dark Current at Injector. Jang-Hui Han 27 November 2006 XFEL Beam Dynamics Meeting

Observation of Coherent Optical Transition Radiation in the LCLS Linac

High-Brightness Electron Beam Challenges for the Los Alamos MaRIE XFEL

Femto second X ray Pulse Generation by Electron Beam Slicing. F. Willeke, L.H. Yu, NSLSII, BNL, Upton, NY 11973, USA

MaRIE. MaRIE X-Ray Free-Electron Laser Pre-Conceptual Design

VELA/CLARA as Advanced Accelerator Studies Test-bed at Daresbury Lab.

THE LASER HEATER SYSTEM OF SWISSFEL

Modeling of Space Charge Effects and Coherent Synchrotron Radiation in Bunch Compression Systems. Martin Dohlus DESY, Hamburg

START-TO-END SIMULATIONS FOR IR/THZ UNDULATOR RADIATION AT PITZ

SRF GUN CHARACTERIZATION - PHASE SPACE AND DARK CURRENT MEASUREMENTS AT ELBE*

FLASH/DESY, Hamburg. Jörg Rossbach University of Hamburg & DESY, Germany - For the FLASH Team -

6 Bunch Compressor and Transfer to Main Linac

Accelerator Physics Issues of ERL Prototype

Harmonic Lasing Self-Seeded FEL

Introduction to Free Electron Lasers and Fourth-Generation Light Sources. 黄志戎 (Zhirong Huang, SLAC)

SPPS: The SLAC Linac Bunch Compressor and Its Relevance to LCLS

SCSS Prototype Accelerator -- Its outline and achieved beam performance --

UV laser pulse temporal profile requirements for the LCLS injector - Part I - Fourier Transform limit for a temporal zero slope flattop

Potential use of erhic s ERL for FELs and light sources ERL: Main-stream GeV e - Up-gradable to 20 + GeV e -

Femtosecond X-ray Pulse Temporal Characterization in Free-Electron Lasers Using a Transverse Deflector. Abstract

Introduction to single-pass FELs for UV X-ray production

Alignment requirement for the SRF cavities of the LCLS-II injector LCLSII-TN /16/2014

Simulations for photoinjectors C.Limborg

Opportunities and Challenges for X

First operation of a Harmonic Lasing Self-Seeded FEL

FLASH II Seeding History and Future. Kirsten Hacker April 2014

An Adventure in Marrying Laser Arts and Accelerator Technologies

Using IMPACT T to perform an optimization of a DC gun system Including merger

MOGA Optimization of LCLS2 Linac

Fast Simulation of FEL Linacs with Collective Effects. M. Dohlus FLS 2018

LCLS-II Capabilities & Overview LCLS-II Science Opportunities Workshop. Tor Raubenheimer (P. Emma) February 9 th, 2015

Greenfield FELs. John Galayda, SLAC Kwang-Je Kim, ANL (Presenter) James Murphy, BNL

Cavity Field Maps (TESLA & 3 rd Harmonic Cavity) Undulator Wakes. Estimation of CSR Effects for FLASH2HGHG

Start-to-End Simulations

High Energy Gain Helical Inverse Free Electron Laser Accelerator at Brookhaven National Laboratory

modeling of space charge effects and CSR in bunch compression systems

FIRST LASING OF THE LCLS X-RAY FEL AT 1.5 Å

Longitudinal Impedance Budget and Simulations for XFEL. Igor Zagorodnov DESY

Transcription:

Linac optimisation for the New Light Source NLS source requirements Electron beam requirements for seeded cascade harmonic generation LINAC optimisation (2BC vs 3 BC) CSR issues energy chirp issues jitter (preliminary studies at 200 pc and 500 pc) FEL simulations (time dependent SASE cascade harmonic) R. Bartolini Diamond Light Source and John Adams Institute, Oxford University FEL Beam Dynamics Meeting DESY, 13 July 2009

NLS Source requirements (Dec 08) 1. Photon energy range and tunability: Three FELs: FEL1 @ 50-300 ev; FEL2 @ 250-850 ev; FEL3 @ 430-1000 ev 2. Polarisation: FEL1&FEL2: complete polarisation control (arbitrary elliptical and rotatable linear). FEL3: at least horizontal and circular (R/L) polarisation over the full range 430-1000 ev. 3. Pulse length & pulse energy: 20 fs FWHM photon pulse length at all photon energies with 10 11 photons/pulse at 1 kev (upgrade path to sub-fs pulses) 4. Repetition rate: 1 khz with an upgrade path to 100 khz (or more) 5. Transverse and longitudinal coherence

Electron beam requirements Operation of an X-ray FEL requires extremely high quality electron beams; Energy 1-few GeV Emittance (normalised) 10 6 m relative energy spread 10 4 Peak current few ka for seeded cascade harmonic generation constant slice parameters on a length of 100 fs and more? to accommodate the seed pulse and the jitters without accidental good slices that would spoil the contrast ratio no jagged current distribution no slice offset and angle not too sensitive to jitters no residual energy chirp (or very limited) Carefully optimised RF photocathode gun and LINAC with magnetic bunch compressors can provide high brightness electron beam, but satisfying all the requirements is non trivial

Layout and parameters of a 2.2 GeV Linac based FEL 2.2 GeV; 200-500 pc optimised L-band gun: 20 ps FW, 0.33 µm (proj. nor. emit.) see J-H. Han s talk LINAC L-band gradient 20 MV/m and 3HC @ 3.9 GHz 15 MV/m Magnetic bunch compressors Beam spreader see D. Angal-Kalinin s talk Undulator train see also N. Thompson s talk on FEL harmonic schemes Gun A01 A02 A03 A39 BC1 A04 A05 A06 A07 A08 BC2 A09 A10 A11 A12 A13 A14 DL undulators Gun A01 A39 BC0 A02 A03 BC1 A04 A05 A06 A07 A08 BC2 A09 A10 A11 A12 A13 A14 DL undulators Gun A01 A39 BC0 A02 A03 A39 BC1 A04 A05 A06 A07 A08 BC2 A09 A10 A11 A12 A13 A14 DL undulators Gun A01 A02 A39 BC1 A03 A04 A05 A06 A07 A08 A09 A10 A11 A12 A13 A14 DL undulators

Working point defined by: FEL working point minimum allowable undulator gap at 430 ev (8 mm) saturation length at 1 kev requirements on K (K > 0.7) and beam quality Using Xie parameterisation with I peak = 1 ka, ε n = 1µm, σ ε = 5 10 4 430 ev 1 kev λ u = 32 mm; g = 8 mm K = 1.56; < β > = 5 m λ u = 32 mm; g = 14.4 mm K = 0.67; < β > = 10 m

Numerical optimisation of a 2.2 GeV LINAC (I) Gun A01 A02 A03 A39 BC1 A04 A05 A06 BC2 A09 A10 A11 A12 DL undulators A07 A08 A13 Layout 1 (2BCs) Astra elegant GENESIS Gun A01 A39 BC0 A02 A03 BC1 A04 A05 A06 A07 A08 BC2 A09 A10 A11 A12 A13 A14 DL undulators Layout 2 (3BCs) Tracking studies to optimise the beam quality at the beginning of the undulators peak current, slice emittance, slice energy spread, etc elegant simulations include CSR, longitudinal space charge, wake-fields in TESLA modules Parameters used in the optimisation Accelerating section and 3HC amplitude and phase, Bunch compressors strengths Validation with full start-to-end simulation Gun to FEL (time dependent)

Numerical optimisation of a 2.2 GeV LINAC (II) Main issues and guidelines for the optimisation compression should not introduce space charge and CSR issues avoid strong compression at lower energy linear optics tailored to reduce CSR (e.g. minimum horizontal beta at 4 th dipole) compression aided by linearisation of longitudinal phase space with a 3HC analytical formulae for 3HC setting, microbunching gain curves, beam quality optimisation driven directly by the required FEL performance We have devised a multi-parameters multi-objectives optimisation of the LINAC working point based on the Xie parameterisation (semi-analytical expressions) for the gain length and the FEL saturation power. We target gain length, FEL saturation power as in a SASE FEL and due to the additional complication with seeding simultaneous optimisation of many slices to achieve a flat portion of the bunch (length 100 fs) with constant slice parameters

Numerical Optimisation of a 2.2 GeV LINAC (III) We have adopted a multi-objectives multi-parameters optimisation of the LINAC based on a fast numerical computation of the Xie gain length vs LINAC parameters Xie gain length L = L ( ε, σ, σ,...) 3D 3D x ε x Compute the slice properties ε x,σ ε, σ x, from elegant L = ( V1,..., Vn, V3HC, φ1,..., φn, φ3hc, θ1, 2,...) 3D L3 D θ Objectives: L 3D, P sat AND length of the good slice region (compression strength, ) Parameters: amplitudes and phases of RF accelerating sections, compressors, Parallel Search Algorithms (Genetic Algorithm SPEA)

Multi-objective multi-parameter optimisation 18000 runs with 100K particle each 2 objectives: minimise Xie Length and maximise and P sat 4 parameters: phase of ACC02; ACC4-7, BC1, BC2 Manual optimisation (red dot) xie length 1.24 (m) avg sat power 2030 (MW) (θ 2, θ 3, ϕ 2, ϕ 4 ) = (17.5, 6.1, 7.75, 25) Multi-objective optimisation xie length 1.15 (m) ( 8%) avg sat power 2220 (MW) (+11%) (θ 2, θ 3, ϕ 2, ϕ 4 ) = (17.54, 4.92, 8.96, 29.91) The Xie length is averaged over the slices covering a portion of 100 fs of the bunch

Optimised beam from the L-band L injector L-band NC gun optimisation ongoing Longitudinal phase space ASTRA to deal with space charge issues 200 pc 20 ps FW 130 MeV Normalised slice emittance below 4 10-7 m Slice relative energy spread below 2 10-5 I peak 15 A Slice normalised emittance Longitudinal current distribution

Beam properties along the LINAC: layout 1 (2BCs) Gun A01 A02 A03 A39 BC1 A04 A05 A06 A07 A08 BC2 A09 A10 A11 A12 A13 DL undulators before 3HC after BC1 before undulators 50 fs (rms) 200 fs BC2 6.95 deg; best slices I peak 1.7 ka, ε n 0.4 µm, σ ε 10 4 ; 50 fs (rms)

CSR issues and compression optimisation (BC2) 180 8000 160 7000 bunch length rms (fs) 140 120 100 80 60 40 peak current (A) 6000 5000 4000 3000 2000 20 1000 0 6.4 6.6 6.8 7 7.2 7.4 7.6 7.8 0 6.4 6.6 6.8 7 7.2 7.4 7.6 7.8 BC2 compressor angle (deg) BC2 compressor angle (deg) 120 normalised H emittance (um) 100 80 60 40 20 working point 0 6.4 6.6 6.8 7 7.2 7.4 7.6 7.8 BC2 compressor angle (deg) over compressed under compressed 10 e - bunches superimposed

FEL Time dependent S2E simulations λ u = 31.9 mm; g = 14.4 mm; K = 0.67 These offsets in position and angle kill the gain 70 µm and 30 µrad Trajectory of centre of charge corrected Lsat 50 m Trajectory of each slice corrected Lsat 36 m

Issues and alternative layouts The main issue with the 2BC layout is the need to reduce 3HC gradient ( 40 MV/m): Several attempts were made generating a shorter (15 ps FW) and more linear bunch from the gun and/or add on more 3HC module (FLASH Type with 4 cavities per modules) Gun A01 A02 A03 A39 A39 BC1 A04 A05 A06 A07 A08 BC2 A09 A10 A11 A12 A13 A14 DL undulators or add on more (weak) bunch compressor Gun A01 A39 BC0 A02 A03 BC1 A04 A05 A06 A07 A08 BC2 A09 A10 A11 A12 A13 A14 DL undulators or other locations of BCs

Beam properties along the LINAC: layout 2 (3BCs) Gun A01 A39 BC0 A02 A03 BC1 A04 A05 A06 A07 A08 BC2 A09 A10 A11 A12 A13 A14 DL undulators 135 MeV 110 MeV 440 MeV 1.2 GeV 18 ps 10 ps 2 ps 300 fs 3HC at 3.9 GHz can work at 15 MV/m; No need of a second 3HC before second BC; ε nx 4.3 10 7

Numerical issues with CSR Significant Modulation with period 7 fs 2 um Compression factor 70 500 fs at the cathode 100k; 500 bins 1M; 500 bins 100k; 100 bins 1M; 100 bins 200 pc optimised case; 100k particles; NBINS = 500; jagged longitudinal phase space Still OK for SASE but too spiky(?) for HGHG

Numerical issues with CSR Sources of density fluctuations shot noise; external causes (e.g. laser flat top, )

Energy chirp issues (I) Energy chirp should be smaller than the SASE intrinsic BW ( ρ = 10-3 ) γ γ / γ = 3.2 10-3 3 times larger than the SASE BW 200 100 0 100 200 Time (fs) Comparing to numerical simulations at LCLS-FERMI wakefields were crucial in flattening the residual chirp. Larger energy helps (large γ and longer linacs)

Energy chirp issues (II) use wakefields in L band structures wakefields are weaker than in S-band 200 pc too small use the main RF to reduce chirp accelerating beyond crest bunch too short after 3BC (RF slope sampled is too small) L-band has a smoother curvature than S-band use less chirp from the beginning γ / γ = 1.6 10-3 reduced but larger compression! 200 100 0 100 200 Time (fs)

C-type chicanes

3D gain length with beam offset and angle Using genesis SS simulations adding H offset, V offset, H angle, V angle Trying to parameterise as per Xie formalism (normalis. emitt. ε x = 0.4 um, relative energy spread 2e-4, I peak = 2 ka) Angle dependence is very critical! (tbc)

S-type chicanes

200 pc best optimisation 100 fs

Cascade Harmonic Scheme output Power @19.3m Spectrum @19.3m z 3.2μm λ/λ 4e-4 Power @19.3m Time-bandwidth product 1 Contrast ratio 15

Jitter studies The FEL performance can be severely spoiled by jitter in the electron beam characteristics To understand this issue we have started a numerical investigation of the sensitivity of the beam quality to various jitter sources: phase and amplitude of RF sections bunch compressor power supplies Adding the jitter sources one-by-one and all together as random noise Jitter in the GUN was also included gun phase and voltage solenoid field charge laser spot position jitter

FEL time dependent simulations with 3BC layout (multi-parameter optimisation) overcompressed Best slice: ε x = 4 10 7 m ; σ γ = 8 10 5 ; I peak = 1.6 ka; along 100 fs or more with a flat plateau (typical for overcompressed bunches) Lsat 45 m

200 pc jitter Gun Jitter Parameters (standard deviations) Solenoid Field 0.02e-3 T Gun Phase 0.15 degrees Gun Voltage 0.05 MV/m Charge 1% X Offset 0.025 mm Arrival Time Jitter at end of LINAC (standard deviation, fs) Phase (P) 0.01 degrees 9 Bunch Compressor (B) 5e-5 fractional 11 Voltage (V) 1-e4 fractional 14 Gun (G) 23 P + V + B 18 P + V + B + G 28

200pC Beam profiles with jitter

Beam jitter causes from the LINAC RF Applying jitter errors in the amplitude and phase of the RF station one by one we can determine the impact of each accelerating section on the beam parameters 100 The plots refer to the extreme case of 0.1 degrees phase jitter and 0.1% voltage jitter to Jitter 10 1 0.1 RMS energy [MeV] RMS projected emittance [mm.mrad] RMS time of flight [fs] 0.01 RF stations near the start of the linac contribute a large amount to jitter Concentrate on minimising jitter in RF stations between first two bunch compressors but cannot neglect contribution from structures between bunch compressors 2 and 3 Cavities after 3BC play little role Jitter 0.001 100 10 1 0.1 0.01 0.001 BC1 BC1 2 2 3 3 BC2 BC2 4 4 5 5 6 7 8 RF station 6 7 8 RF station BC3 BC3 9 9 10 10 11 11 12 12 13 13 14 RMS energy [MeV] RMS projected emittance [mm.mrad] RMS time of flight [fs] 14

Conclusions and future work (I) We have produced a promising layout of a single-pass LINAC which can deliver an electron beam with the required properties with modest improvements on the present technology requirement on 3HC and RF jitter to be further analysed SASE FEL performance achieved exceeds the 10 11 ppp @ 1 kev Alternative FEL operating mode under consideration (Single Spike; different charge) Wakefield effects and jitter issues under consideration along with a thorough tolerance analysis; Finalise layout choice: continue the evaluation of the 3BC vs 2BC layouts collaboration with LBNL (revisiting our 1BC design) Acknowledgments: C. Christou, J.H. Han, I. Martin, J. Rowland (DLS) D. Angal-Kalinin, F. Jackson, B. Muratori, P. Williams (ASTeC) and the NLS Physics and Parameters Working Group

Optimisation for the operation at 500 pc We consider also a longer electron pulses with constant slice parameters with at least 200 fs flat top (in view of jitter results)

Exit of spreader section (500 pc) > 200 fs

Effect of the laser heater (500 pc) The jagged longitudinal current profile is smoothed by the laser heater Laser heater on Still < 2 10 4 Emittance is unaffected

500 pc jitter Gun Jitter Parameters (standard deviations) Solenoid Field 0.02e-3 T Gun Phase 0.075 degrees Gun Voltage 0.025 MV/m Charge 1% X Offset 0.025 mm Arrival Time Jitter (standard deviation, fs) Phase (P) 0.01 degrees 8 Bunch Compressor (B) 5e-5 fractional 17 Voltage (V) 1-e4 fractional 27 Gun (G) 56 P + V + B 32 P + V + B + G 61 Requirements on the gun is even more stringent than in the 200 pc case

500pC Beam profiles with jitter

FEL Scheme (N. Thompson) HHG 75-100eV Modulator 1 λ w = 44 mm Modulator 2 λ w = 44 mm APPLE-II Radiator λ w = 32.2 mm FEL3 e - @ 2.25 GeV Modulator 1 HHG 75-100eV λ w = 44 mm Modulator 2 λ w = 44 mm APPLE-II Radiator λ w = 38.6 mm FEL2 430-1000eV e - @ 2.25 GeV HHG 50-100eV Modulator λ w = 49 mm APPLE-II Radiator λ w = 56.2 mm FEL1 250-850eV e - @ 2.25 GeV 50-300eV - common electron energy for all 3 FELs, allows simultaneous operation - seeded operation for longitudinally coherent output - HHG seeding with realistic laser parameters, up to 100 ev (100kW at 100 ev is realistic) (100 kw at 200 ev seeding level proved insufficient) - harmonic cascade FEL scheme to reach up to 1 kev in the fundamental