rf synchronisation issues xband linacs for fels lancaster university october 2014 red linac sections...
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RF Synchronisation Issues
Xband Linacs for FELs
Lancaster University
October 2014
Red linac sections are X bandOff crest acceleration provides bunch compression Phase errors in linac RF cavities gives unwanted beam energy spread in undulatorAverage phase in linac RF cavities must be correct to within 0.02 degrees ~ 5 fs
RF Systems and Stability [email protected]
Linac Coherent Light Source Stanford Synchrotron Radiation LaboratoryStanford Linear Accelerator Center
LCLS Linac Review 12th December 2003 P. A. McIntosh, SLAC Klystron Dept.
X-Band Stability
NLCTA modulator voltage stability ~ 0.01%.Nominal operating voltage of 350 kV 35 V variation
XL-4 phase stability vs beam voltage = 0.0033o/VXL-4 phase stability then becomes ~ 0.12o without feedback!
L2 modulators are currently regulating to better than 0.01%!
NLCTA structure temperature tuning stability ~200 kHz/oCNeed to regulate structure temperature to 0.025oC
detuning 10 kHz
Phase variation = xs = 0.36o (for filling time s = 100 ns) without feedback!
Estimate for X-band system phase stability h = 0.48o
LCLS requirement is h = 0.50o
SLAC
SLAC achieving 0.08o stability translate to about 0.32o at XBand
LCLS Klystron
Timing Problems
• Stability Oscillators shift period with temperature, vibration etc. VCO shifts period with applied voltage Atomic clock f/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
Optical clock signal
Locked microwave oscillator
Solid state amplifier
IQ modulator
Solid state amplifier
TWT amplifier Klystron
Pulse compressor
Waveguide
Waveguide
Waveguide
Cavity
sensitive to temperature
Extremely sensitive to modulator
voltage
LLRF control - feedforward to next pulse based on last pulse and environment measurements
Every connector adds uncertainty
CLIC Cavity Synchronisation
Cavity to Cavity Phase synchronisation requirement
degrees1S
1
c
f7204rmsc
x
Target max. luminosity loss fraction S
f (GHz)
x
(nm)c
(rads)rms
(deg)t (fs) Pulse
Length (s)
0.98 12.0 45 0.020 0.0188 4.4 0.156
So need RF path lengths identical to better than c t = 1.3 microns
CLIC bunches ~ 45 nm horizontal by 0.9 nm vertical size at IP.
RF path length measurement
48MW 200ns pulsed 11.994 GHz Klystron
repetition 50Hz Vector
modulationControl
Phase Shifter
12 GHz Oscillator
Main beam outward pick up
Main beam outward pick up
From oscillator
Phase shifter trombone
(High power joint has been tested at SLAC)
Magic Tee
Waveguide path length phase and amplitude measurement and control
4kW 5s pulsed 11.8 GHz Klystron
repetition 5kHz
LLRF
Phase shifter trombone
LLRF
Cavity coupler 0dB or -40dB
Cavity coupler 0dB or -40dB
Expansion joint
Single moded copper plated Invar waveguide losses over 40m ~ 3dB -30 dB
coupler -30 dB coupler
Forward power
main pulse
12 MW
Reflected power main pulse ~ 600 W
Reflected power main pulse ~ 500 W
Waveguide from high power Klystron to magic tee can be
over moded
Expansion joint
RF path length is continuously measured and adjusted
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
PLL controller MCU10.7 GHz VCODigital phase
detector
DBMs
Power MeterOutput
Wilkinson splitter
Input 1
Power MeterOutput
Input 2
Phase measurement accuracy
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
Reflection from cavity 1
Reflection from cavity 2
Voltage to oscilloscope /
ADC
High Speed op
amp
Double balanced mixer Variable LPF
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.
March 2012 10
Results (from slide 7)
7 kHz 200 kHz 30MHz
2.54 mV/mdeg 2.17 mV/mdeg 2.17 mV/mdeg
To oscilloscope
Mixer
12 GHz Source
Splitter
Coax lines
Coax line
Coax line stretchers
Waveguide choice
Waveguide type35 meters COPPER
Expansion = 17 ppm/K
Mode Transmission Timing error/0.3°CWidth
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) TE10 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 TE01 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°CWidth
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) TE10 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 TE01 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.
Prototype systems have been developed.
Linear Phase Detector
DSPADC
ADC
MagicTee
To Cavity To Cavity
Wilkinson splitters
-30 dB coupler
DBM
DBM DBM
10.7GHz Oscillator
-30 dB coupler
Manual phase shifter for initial setup
Fast piezoelectric phase shifter
DAC
Amp + LPF
Amp + LPF