Influence of the Third Harmonic Module on the Beam Size Maria Kuhn University of Hamburg Bachelor Thesis Presentation.

Slides:



Advertisements
Similar presentations
Nominal and no CSR (R 56-1 = 55 mm, R 56-2 = 59 mm, R 56-3 = 0) L1 phase = 21 deg, V 3.9 = 55 MV CSR OFF BC3 OFF Elegant Tracking  z1 = mm (post.
Advertisements

ILC Accelerator School Kyungpook National University
Christopher Gerth, Michael Röhrs, Holger Schlarb DESY Hamburg Optics for Diagnostic Section BC1 in the European XFEL.
J. Rudolph, Helmholtz-Zentrum Berlin EuCARD 2nd ANNUAL MEETING Slice emittance measurements at the ELBE superconducting RF photoinjector.
1 Bates XFEL Linac and Bunch Compressor Dynamics 1. Linac Layout and General Beam Parameter 2. Bunch Compressor –System Details (RF, Magnet Chicane) –Linear.
Bunch compressors ILC Accelerator School May Eun-San Kim Kyungpook National University.
1 ILC Bunch compressor Damping ring ILC Summer School August Eun-San Kim KNU.
Low energy electron beam as a nondestructive diagnostic tool for high power beams. P. Logachev, D. Malutin, A. Starostenko, BINP, RUPAC’2006, Novosibirsk.
1 Preliminary Analysis of GTF Longitudinal Emittance Experiment D. Dowell SLAC July 18, 2001.
Bunch compressor design for eRHIC Yichao Jing and Vladimir Litvinenko FLS2012, Newport News, VA 3/8/2012.
Transverse optics 2: Hill’s equation Phase Space Emittance & Acceptance Matrix formalism Rende Steerenberg (BE/OP) 17 January 2012 Rende Steerenberg (BE/OP)
M. LindroosNUFACT06 School Accelerator Physics Transverse motion Mats Lindroos.
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.
LCLS-II Transverse Tolerances Tor Raubenheimer May 29, 2013.
FEL Beam Dynami cs FEL Beam Dynamics T. Limberg FEL driver linac operation with very short electron bunches.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, N.Kazarinov.
~ gun3.9 GHz cavity Bunch compressor 3 ILC cryomodules 45 deg. spectro injector main linac user area disp. area transport line Overview of.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, A.Drozhdin, N.Kazarinov.
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.
Max Cornacchia, Paul Emma Stanford Linear Accelerator Center Max Cornacchia, Paul Emma Stanford Linear Accelerator Center  Proposed by M. Cornacchia (Nov.
1 Plan and Opportunities for Migration and Integration of the Photoinjector into New Muon Lab Mike Church AAC Review - 12/5/06.
Beam Dynamics and FEL Simulations for FLASH Igor Zagorodnov and Martin Dohlus Beam Dynamics Meeting, DESY.
A bunch compressor design and several X-band FELs Yipeng Sun, ARD/SLAC , LCLS-II meeting.
EMMA Extraction / Diagnostic line Bruno Muratori STFC, Daresbury Laboratory 01/09/08.
A U.S. Department of Energy Office of Science Laboratory Operated by The University of Chicago Office of Science U.S. Department of Energy Containing a.
Overview of Booster PIP II upgrades and plans C.Y. Tan for Proton Source group PIP II Collaboration Meeting 03 June 2014.
S. Molloy, P. Emma, J. Frisch, R. Iverson, M. Ross, D. McCormick, M. Woods, SLAC, CA, USA S. Walston, Lawrence Livermore National Laboratory, CA, USA V.
1 Alternative Bunch Compressor 30 th Sep KNU Eun-San Kim.
Tuesday, 02 September 2008FFAG08, Manchester Stephan I. Tzenov1 Modeling the EMMA Lattice Stephan I. Tzenov and Bruno D. Muratori STFC Daresbury Laboratory,
XFEL Beam Dynamics Meeting Bolko Beutner, DESY Velocity Bunching Studies at FLASH Bolko Beutner, DESY XFEL Beam Dynamics Meeting
T. Limberg Position of the 3rd Harmonic System. Injector (with first Bunch Compression Stage) 2 European XFEL MAC May 2010 T. Limberg.
Kiyoshi Kubo Electron beam in undulators of e+ source - Emittance and orbit angle with quad misalignment and corrections - Effect of beam pipe.
By Verena Kain CERN BE-OP. In the next three lectures we will have a look at the different components of a synchrotron. Today: Controlling particle trajectories.
July LEReC Review July 2014 Low Energy RHIC electron Cooling Jorg Kewisch, Dmitri Kayran Electron Beam Transport and System specifications.
P. Urschütz - CTF3 Collaboration Meeting 2007 CTF3 commissioning & operation in 2006 P. Urschütz for the CTF3 operations team  Commissioning of the Delay.
Awake electron beam requirements ParameterBaseline Phase 2Range to check Beam Energy16 MeV MeV Energy spread (  ) 0.5 %< 0.5 % ? Bunch Length (
Michael Röhrs On-crest slice emittance measurements Michael Roehrs.
Lecture 4 - E. Wilson –- Slide 1 Lecture 4 - Transverse Optics II ACCELERATOR PHYSICS MT 2009 E. J. N. Wilson.
Christopher Gerth & Christopher Behrens Mini-Workshop on Longitudinal Diagnostics for FELs 11/12 March 2013, PSI, Villigen TDS induced energy spread.
X-band Based FEL proposal
PAL-XFEL Commissioning Plan ver. 1.1, August 2015 PAL-XFEL Beam Dynamics Group.
B. Marchetti R. Assmann, U. Dorda, J. Grebenyuk, Y. Nie, J. Zhu Acknowledgements: C. Behrens, R. Brinkmann, K. Flöttmann, M. Hüning,
Sub-Task HOM-BPM HOM based Beam Position Monitors – Planned and Extant Measurements N. Baboi, DESY, Hamburg EuCARD WP 10: SRF, Annual Review Meeting.
Review of Alignment Tolerances for LCLS-II SC Linac Arun Saini, N. Solyak Fermilab 27 th April 2016, LCLS-II Accelerator Physics Meeting.
Frank Stulle, ILC LET Beam Dynamics Meeting CLIC Main Beam RTML - Overview - Comparison to ILC RTML - Status / Outlook.
OPERATED BY STANFORD UNIVERSITY FOR THE U.S. DEPT. OF ENERGY 1 Alexander Novokhatski April 13, 2016 Beam Heating due to Coherent Synchrotron Radiation.
Beam dynamics for an X-band LINAC driving a 1 keV FEL
Sara Thorin, MAX IV Laboratory
For Discussion Possible Beam Dynamics Issues in ILC downstream of Damping Ring LCWS2015 K. Kubo.
Slice Parameter Measurements at the SwissFEL Injector Test Facility
Andrei Shishlo ORNL SNS Project Florence, Italy November 2015
Have a chance to operate your own beam at CERN
Longitudinal Diagnostics for start-up
Linac optimisation for the New Light Source
Thermal emittance measurement Gun Spectrometer
R. Bartolini Diamond Light Source Ltd
Diagnostics overview and FB for the XFEL bunch compressors
Injector: What is needed to improve the beam quality?
Lecture 4 - Transverse Optics II
Simulation Calculations
ICFA Mini-Workshop, IHEP, 2017
Linac/BC1 Commissioning P
Lecture 4 - Transverse Optics II
High Level Physics Applications for LCLS Commissioning
Linac Diagnostics Patrick Krejcik, SLAC April 24, 2002
Linac Diagnostics Commissioning Experience
Operational Experience with LCLS RF systems
Evgenij Kot XFEL beam dynamics meeting,
Recent Measurements in ACC1 (12.9. & )
Presentation transcript:

Influence of the Third Harmonic Module on the Beam Size Maria Kuhn University of Hamburg Bachelor Thesis Presentation

FLASH Layout after the 2009 Upgrade Important elements of the beam line for emittance measurements Third harmonic module ACC39 Bunch compressor BC2 Diagnostics DBC2 Undulator – SASE process Why emittance measurement? for standard operation: beam with low transverse emittance in high-current peak indicator for beam size/ quality we determine the projected transverse emittance

Bunch Compression Four-bending-magnetic chicane curved sections: path length difference because of energy chirp of bunch head to tail acceleration off-crest small momentum: bunch head large momentum: bunch tail curvature of longitudinal phase space due to RF non-linear longitudinal compression forms the beam solution: third harmonic system

Third Harmonic Module Linearisation of longitudinal phase space after the first bunch compressor ACC39 off: long bunch tails, asymmetric bunches ACC39 on: linearises RF‘s sine shape

Third Harmonic Module Linearisation of longitudinal phase space after the first bunch compressor ACC39 off: long bunch tails, asymmetric bunches ACC39 on: linearises RF‘s sine shape overall RF field is flattened more effective bunch compression uniform intensity bunches

Third harmonic module cavity Problems: wakes are 3x stronger than in 1.3 GHz module non-symmetric structure Consequences: beam off-axis electrons are deflected transverse kicks Influence of Wake-Fields on Transverse Emittance

Third harmonic module cavity Problems: wakes are 3x stronger than in 1.3 GHz module non-symmetric structure Consequences: beam off-axis electrons are deflected transverse kicks Coupling of charged particles HOM field is excited cross section: wake-fields projected emittance grows

Data Analysis Diagnostic Section DBC2: four OTR monitors with well known transfer matrices measurement of transverse charge distribution

Data Analysis Diagnostic Section DBC2: four OTR monitors with well known transfer matrices measurement of transverse charge distribution calculation of the RMS beam size σ Phase space ellipse Twiss parameters √ √

Emittance Measurement Beam Size and 90% intensity cut

Emittance Measurement Beam Size and 90% intensity cut Normalized emittance: Emittance determination: (fit with χ 2 -method)

Trajectory Bump

Trajectory Amplitude in ACC39 Transfer matrix formulation Solution of equation of motion

Trajectory Amplitude in ACC39 Transfer matrix formulation Solution of equation of motion R1

Trajectory Amplitude in ACC39 Transfer matrix formulation Solution of equation of motion with R2 R3

Trajectory Amplitude in ACC39 Transfer matrix formulation Solution of equation of motion Resulting amplitude in the middle of the 3.9 GHz module with R4 R5

Results Emittance Measurement from 2010 Emittance Measurement from 2009 Diamonds: 3GUN Circles: 1GUN+2GUN Relative change of normalized emittance for different horizontal and vertical bump amplitudes

Error Analysis Image Analysis – Error of the beam size: 3% - 5% – Calibration of OTR monitors: 3% Emittance Calculation – Transfer matrices – Energy error: 2% quadrupole k-value – Error of normalized emittance: 2% horizontal and 4% vertical plane Trajectory – Calibration of steerer : 3% – Energy error (s.a.) – BPM calibration: 10% - 15% Statistical Errors – Beam size (CCD camera) < 5% Overall: 10% - 20% neglected

Conclusion The third harmonic module linearises the longitudinal phase space For standard operation the new system does not alter the projected transverse emittance The influence of wake-fields from the ACC39 cavities can be neglected

Results II Example plot x versus x‘ correlation between amplitude (x or y) and slope (x‘ or y‘) is linear at extreme amplitude: additional angle in the centre of the module Horizontal amplitude of 2.5mm in ACC39 Angle of 0.5mrad in the middle Additional amplitude at the end of the module of 0.5mm