RF Synchronisation Issues

Slides:



Advertisements
Similar presentations
Synchronization system for CLIC crab cavities Amos Dexter, Ben Woolley, Igor Syratchev. LCWS12, UTA October 2012.
Advertisements

Particle Accelerator Engineering, London, October 2014 Phase Synchronisation Systems Dr A.C. Dexter Overview Accelerator Synchronisation Examples Categories.
Laser / RF Timing (Engineering of Femtosecond Timing Systems)
R. Akre, P. Emma, P. Krejcik LCLS April 29, 2004 LCLS RF Stability Requirements LCLS Requirements The SLAC Linac.
R. Akre XFEL Short Bunch Measurement and July 26, 2004 LCLS Drive Laser Timing Stability Measurements XFEL Short Bunch Measurement.
Laser to RF synchronisation A.Winter, Aachen University and DESY Miniworkshop on XFEL Short Bunch Measurement and Timing.
Synchronization System for LUX John Staples, LBNL 26 July 2004.
RF Systems and Stability Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator Center.
Automation of the 805MHz cavity conditioning procedure Ajit Kurup MuCool Test Area RF Workshop, Fermilab 22 nd August 2007.
Patrick Krejcik LCLS April 7-8, 2005 Breakout Session: Controls Physics Requirements and Technology Choices for LCLS Instrumentation.
Stefan Simrock 3 rd LC School, Oak Brook, IL, USA, 2008, Radio Frequency Systems 1 Timing and Synchronization S. Simrock and Axel Winter DESY, Hamburg,
RF SYSTEM DESIGN FOR THE TOP-IMPLART ACCELERATOR V. Surrenti, G. Bazzano, P. Nenzi, L. Picardi,C. Ronsivalle, ENEA,Frascati, Italy ; F. Ambrosini, La Sapienza.
LLRF Phase Reference System The LCLS linac is broken down into 4 separate linac sections. The LCLS injector will reside in an off axis tunnel at the end.
RF Synchronization, control and stability Takuya Natsui.
RF Synchronization Activity at SPARC A.Gallo and D. Alesini, M. Bellaveglia, R. Boni, G. Di Pirro, A. Drago, A.Ghigo P. Baldini, L. Cacciotti, M. Scampati,
DMP Product Portfolio Femtosecond Lasers Trestles Ti:Sapphire lasers …… fs; nm, mW Mavericks Cr:Forsterite lasers
LLRF System for Pulsed Linacs (modeling, simulation, design and implementation) Hooman Hassanzadegan ESS, Beam Instrumentation Group 1.
Holger Schlarb, DESY Normal conducting cavity for arrival time stabilization.
The PITZ Timing System Frank Tonisch DESY - Zeuthen.
1 LLRF Pre-readiness review (26th May, 2009) 27/10/2015 LLRF performance and its limitation based on KEK's experiments Shin Michizono (KEK) KEK’s LLRF.
R. Akre RF / Timing August 11, 2004 LCLS Drive Laser Timing Stability Measurements Department of Energy Review of the Linac.
LLRF ILC GDE Meeting Feb.6,2007 Shin Michizono LLRF - Stability requirements and proposed llrf system - Typical rf perturbations - Achieved stability at.
Clustered Surface RF Production Scheme Chris Adolphsen Chris Nantista SLAC.
LLRF-05 Oct.10,20051 Digital LLRF feedback control system for the J-PARC linac Shin MICHIZONO KEK, High Energy Accelerator Research Organization (JAPAN)
Cockcroft Institute EuroTeV January 2007 ILC Crab Cavity Collaboration Cockcroft Institute : –Graeme Burt (Lancaster University) –Richard Carter (Lancaster.
1Matthias LiepeAugust 2, 2007 LLRF for the ERL Matthias Liepe.
IWLC10 CLIC Crab Cavities Amos Dexter (on behalf of the LC Crab System Collaborations) CERN 20 th October 2010.
Anders Sunesson RF Group ESS Accelerator Division
Cockcroft Institute August2008 ILC Crab Cavity LLRF Amos Dexter, Imran Tahir, Peter McIntosh, Graeme Burt, Philippe Goudket, Carl Beard, Phil Buckley,
LLRF for EUCARD Crab Cavities Graeme Burt (on behalf of Amos Dexter) Paris May 2011.
LCLS_II High Rep Rate Operation and Femtosecond Timing J. Frisch 7/22/15.
INVESTIGATIONS OF MULTI-BUNCH DIELECTRIC WAKE-FIELD ACCELERATION CONCEPT National Scientific Center «Kharkov Institute of Physics and Technology» Kharkov,
1/19/2006Frank Lenkszus Advanced Photon Source 1 ILC Timing Frank Lenkszus Controls Group Advanced Photon Source Argonne National Lab.
Ding Sun and David Wildman Fermilab Accelerator Advisory Committee
EUCARD WP12 DESY 2015 Slide 1 EuCARD-2 is co-funded by the partners and the European Commission under Capacities 7th Framework Programme, Grant Agreement.
Measurements of the X-ray/pump laser pulse timing Valery Dolgashev, David Fritz, Yiping Feng, Gordon Bowden SLAC 48th ICFA Advanced Beam Dynamics Workshop.
LCLS LLRF System October 10-13, 2005 LLRF05 B. Hong, R. Akre, A. Hill, D. Kotturi, H. Schwarz SLAC, Stanford, Menlo Park, CA 94025, USA Work supported.
Femtosecond phase measurement Alexandra Andersson CLIC Beam Instrumentation workshop.
BEPC II TIMING SYSTEM EPICS Seminar Presented by Ma zhenhan IHEP 20.August 2002.
UK LC accelerator programme Philip Burrows John Adams Institute Oxford University 1.
High Power RF Measurements Ben Woolley, Amos Dexter, Igor Syratchev. Jan Kovermann, Joseph Tagg HG2013, Trieste June 2013.
CLIC-UK Programme Status Philip Burrows John Adams Institute Oxford University 1.
High precision phase monitoring Alexandra Andersson, CERN Jonathan Sladen, CERN This work is supported by the Commission of the European Communities under.
High gradient test results from X-BOX1 Ben Woolley XBOX Team CERN, Switzerland December 2013.
Cockcroft Institute February 2008 Low Level RF for Crab Cavities (The ILC in particular) Amos Dexter, Imran Tahir, Peter McIntosh, Graeme Burt.
Instrumentation at ATF / TTF Accelerator Test Facility (KEK) Tesla Test Facility – FLASH (DESY) ESA / LCLS (SLAC) Marc Ross, SLAC.
RF low level control & synchronization A. Gallo, M. Bellaveglia, L. Cacciotti SPARC review committee – ENEA Frascati – 16/11/2005.
FLASH RF gun developments. Sven Pfeiffer for the LLRF team FEL Seminar Hamburg,
April 12 | Comparison of Sophisticated Synthesizer Concepts and Modern Step Attenuator Implementations | 2 Comparison of Sophisticated Synthesizer Concepts.
Experimental modeling of a Magnetron Transmitter for Superconducting Intensity Frontier Linacs Technical notes G. Kazakevich, V. Yakovlev, R. Pasquinelli,
LLRF 15 Daresbury Andrew Moss ASTeC, STFC Daresbury Laboratory.
MO/LO Performance Summary and Maintenance Plans Tomasz Plawski Jefferson Lab OPS Stay Retreat, July 15th, 2015.
Heung-Sik Kang Pohang Accelerator Laboratory
High-efficiency L-band klystron development for the CLIC Drive Beam High-efficiency L-band klystron development for the CLIC Drive Beam CLIC workshop,
EUCARD WP10.3 Daresbury April 2010 LLRF for EUCARD Crab Cavities Amos Dexter and Imran Tahir Daresbury 7 th April 2010.
LLRF for PXIE Brian Chase For the Project X LLRF Collaboration 1 PX Collaboration Meeting, April 2012 Berkeley - B. Chase.
CI Lecture Series Summer 2010 An Overview of IQ Modulation and Demodulation Techniques for Cavity LLRF Control.
RF Synchronization Activity
CLIC Crab Synchronisation
CLIC Crab Synchronisation
An X-band system for phase space linearisation on CLARA
Timing and synchronization at SPARC
RF Synchronisation Issues
Electric Field Amplitude (MV/m)
CEPC RF Power Sources System
RF Pulse Shaping.
LCLS Drive Laser Timing Stability Measurements
LCLS RF Stability Requirements
Linac Coherent Light Source (LCLS) LLRF Preliminary Design Review LLRF Monitor and Control System September 26, 2005 Ron Akre.
Breakout Session SC3 – Undulator
Presentation transcript:

RF Synchronisation Issues Xband Linacs for FELs Lancaster University October 2014 Red linac sections are X band Off crest acceleration provides bunch compression Phase errors in linac RF cavities gives unwanted beam energy spread in undulator Average phase in linac RF cavities must be correct to within 0.02 degrees ~ 5 fs

SLAC

SLAC achieving 0.08o stability translate to about 0.32o at XBand LCLS Klystron SLAC achieving 0.08o stability translate to about 0.32o at XBand

Timing Problems Stability Synchronisation Oscillators shift period with temperature, vibration etc. VCO shifts period with applied voltage Atomic clock Df/f ~ 10-17 ~ 1 fs per minute Synchronisation Two clocks with different periods at same place (PLL) Identical delivery time to two places (Crab Cavity Problem) Same clock at two places Resynchronisation requires constant propagation time of signal Detector with femtosecond accuracy Trigger an event at a later and a different location Needs two stable clocks which are synchronised Must be able to generate event from clock pulse with tiny jitter 10 fs looks achievable see work at DESY and MIT

Clock to cavity Extremely sensitive to modulator voltage Optical clock signal LLRF control - feedforward to next pulse based on last pulse and environment measurements Locked microwave oscillator Solid state amplifier IQ modulator Extremely sensitive to modulator voltage Solid state amplifier TWT amplifier Waveguide Klystron Every connector adds uncertainty Waveguide sensitive to temperature Pulse compressor Waveguide Cavity

CLIC Cavity Synchronisation CLIC bunches ~ 45 nm horizontal by 0.9 nm vertical size at IP. Cavity to Cavity Phase synchronisation requirement Target max. luminosity loss fraction S f (GHz) sx (nm) qc (rads) frms (deg) Dt (fs) Pulse Length (ms) 0.98 12.0 45 0.020 0.0188 4.4 0.156 So need RF path lengths identical to better than c Dt = 1.3 microns

RF path length measurement RF path length is continuously measured and adjusted 4kW 5ms pulsed 11.8 GHz Klystron repetition 5kHz Cavity coupler 0dB or -40dB Cavity coupler 0dB or -40dB Waveguide path length phase and amplitude measurement and control Forward power main pulse 12 MW Single moded copper plated Invar waveguide losses over 40m ~ 3dB -30 dB coupler -30 dB coupler Expansion joint Expansion joint LLRF Magic Tee LLRF Reflected power main pulse ~ 600 W Reflected power main pulse ~ 500 W Phase shifter trombone (High power joint has been tested at SLAC) Phase shifter trombone Waveguide from high power Klystron to magic tee can be over moded Phase Shifter Main beam outward pick up Main beam outward pick up From oscillator 48MW 200ns pulsed 11.994 GHz Klystron repetition 50Hz Vector modulation 12 GHz Oscillator Control

Digital phase detector Board Development Front end electronics to enable phase to be measure during the short pulses to an accuracy of 2 milli-degrees has been prototyped Wilkinson splitter Digital phase detector 10.7 GHz VCO PLL controller MCU Power Meter Output Input 1 DBMs Input 2 Power Meter Output

Phase measurement accuracy Accuracy depends on measurement bandwidth due to noise limitations (bandwidth determines minimum measurement time). Table below shows data for a single mixer + amplifier with 14 dBm power input: can use 4 to double accuracy and use more power. High Speed op amp Double balanced mixer Reflection from cavity 1 Variable LPF Voltage to oscilloscope /ADC Reflection from cavity 2 Pulse length Bandwidth Thermal calculation (milli-deg) RMS resolution measured (milli-deg) 0.14 ms 7 kHz 0.56 1.0 5 μs 200 kHz 3.0 4.6 33 ns 30MHz 37 57

2.54 mV/mdeg 2.17 mV/mdeg 2.17 mV/mdeg Results (from slide 7) 2.54 mV/mdeg 2.17 mV/mdeg 2.17 mV/mdeg 7 kHz 200 kHz 30MHz To oscilloscope 12 GHz Source Coax line stretchers Coax lines Coax line Splitter Mixer March 2012

Waveguide choice Waveguide type 35 meters COPPER Expansion = 17 ppm/K Mode Transmission Timing error/0.3°C Width Timing error/0.3°C length No of modes WR90(22.86x10.16mm) TE10 45.4% 210.5 fs 498.9 fs 1 Large Rectangular (25x14.5mm) 57.9% 189.3 fs 507.8 fs 2 Cylindrical r =18mm TE01 66.9% 804.9 fs 315.9 fs 7 Cylindrical r =25mm 90.4% 279.6 fs 471.4 fs 17 Copper coated extra pure INVAR 35 meters Expansion = 0.65 ppm/K Mode Transmission Timing error/0.3°C Width Timing error/0.3°C length No of modes WR90(22.86x10.16mm) TE10 45.4% 8.13 fs 19.04 fs 1 Large Rectangular (25x14.5mm) 57.9% 6.57 fs 19.69 fs 2 Cylindrical r =18mm TE01 66.9% 30.8 fs 12.1 fs 7 Cylindrical r =25mm 90.4% 10.7 fs 18.02 fs 17 Rectangular invar is the best choice as it offers much better temperature stability-> Expands 2.3 microns for 35 m of waveguide per 0.1 °C.

LLRF Hardware Requirements Fast phase measurements during the pulse (~20 ns). Full scale linear phase measurements to centre mixers and for calibration. High accuracy differential phase measurements of RF path length difference (5 μs, 5 kHz). DSP control of phase shifters. Linear Phase Detector Amp + LPF 10.7GHz Oscillator DBM DBM ADC Amp + LPF ADC DSP DBM DAC Wilkinson splitters -30 dB coupler -30 dB coupler To Cavity Magic Tee To Cavity Manual phase shifter for initial setup Fast piezoelectric phase shifter Prototype systems have been developed.