results from cw stabilized link timing distribution at lcls · results from cw stabilized link...

24
Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang Larry Doolittle John Byrd John Staples

Upload: others

Post on 12-Jun-2020

2 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Results from CW stabilized link timing distribution at LCLS

Russell WilcoxGang Huang

Larry DoolittleJohn Byrd

John Staples

Page 2: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Application and concepts• Requirement: synchronize multiple lasers to a reference signal

– Original spec was 100fs RMS maintained over 8 hours• Emphasis on reliability, as downtime is costly

• Concept: synchronize lasers to RF signal transmitted on fiber– Well-established high harmonic laser locking technique

• We demonstrated 15fs synchronization of two lasers at 2.5GHz– RF-over-fiber is cable TV technology

• All fiber telecom parts for reliability and cost• Standard telecom fiber

– Uses LBL-developed low noise digital phase detector• 0.01 degree phase sensitivity (10fs at 3GHz)

• Optical interferometer to senses fiber delay change– High temporal resolution– Low noise heterodyne interferometer

• Interferometer reports to digital phase detector, which then applies correction to received RF– No mechanical time delay adjusters

Page 3: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Environmental perturbations of fiber, cable, laser

• thermal coefficient of index is the main driver for fiber

Material Coeff. of delay per deg C ∆ delay for 1m, 1 deg.C

Steel 15 x 10^-6 50fs

Aluminum 22 x 10^-6 72fs

Fiber 8 x 10^-6 40fs

Coax, teflon -85 x 10^-6 -425fs

Coax, air heliax -10 x 10^-6 -50fs

Air (thermal) -3 x 10^-6 -10fs

Air (pressure) 2 x 10^-6 / 10 millibars 7fs / 10mbar

Air (humidity) 4 x 10^-6 / 10%RH 13fs / 10%RH

Page 4: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Schematic of one link

• FRM is Faraday rotator mirror (ends of the Michelson interferometer)• FS is optical frequency shifter• CW laser is absolutely stabilized• Transmitted RF frequency is 2856 MHz• Detection of fringes is at receiver• Signal paths not actively stabilized are temperature controlled

Rblock

0.01C

AMCWlaser

0.01C

FS

RF phasedetect,correct

opticaldelay

sensing

FRMFRM fiber 1

fiber 2d1

d2

ωFSωRF

transmitter receiver

Page 5: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Schematic of one link

• FRM is Faraday rotator mirror (ends of the Michelson interferometer)• FS is optical frequency shifter• CW laser is absolutely stabilized• Transmitted RF frequency is 2856 MHz• Detection of fringes is at receiver• Signal paths not actively stabilized are temperature controlled

Rblock

0.01C

AMCWlaser

0.01C

FS

RF phasedetect,correct

opticaldelay

sensing

FRMFRM fiber 1

fiber 2d1

d2

ωFSωRF

transmitter receiver

Page 6: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Schematic of one link

• FRM is Faraday rotator mirror (ends of the Michelson interferometer)• FS is optical frequency shifter• CW laser is absolutely stabilized• Transmitted RF frequency is 2856 MHz• Detection of fringes is at receiver• Signal paths not actively stabilized are temperature controlled

Rblock

0.01C

AMCWlaser

0.01C

RF phasedetect,correct

opticaldelay

sensing

fiber 1

fiber 2d1

d2

ωFSωRF

transmitter receiver

FS FRMFRM

Page 7: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Expansion to multiple channels

• Since all processing is at reciever, a multi-channel transmitter is not complex– 32-channel amp/splitter/ref arm fits in 8U (14”) high rack chassis

Rbfreq.locker

ref.arm

AMCWfiberlaser

RF in

ref.arm

ref.arm

100MHz beat

LLRF controllerfreq.shifter

LLRF controllerfreq.shifter

LLRF controllerfreq.shifter

Page 8: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Two-channel test interferometer

• This is an out-of-loop test to see if the interferometers are working• Also, it’s a measurement of the actual drift and noise• We installed this in LCLS, and measured tunnel and gallery 2km fibers

freq.shifter

100MHz beat

2km

freq.shifter

RF controller

2km

+50MHz

-50MHz

100MHz beatCW

fiberlaser

phase data

2m

2m

Page 9: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Test interferometer results

• Translating phase error on the 100MHz beat note to 200THz optical, the integrated jitter is ~0.25fs (assuming perfect wavelength stability)

• With 2ns total correction, the average drift is 3fs (less than one wave) per day– We later found the monotonic drift was a computation artefact

time, hoursfrequency, Hz

unlocked

lockeddifferential error

delay variation

Page 10: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Receiver functions are implementedby a digital phase detector

• 14 bit DACs• 125MHz sample rate• It controls both the interferometer and RF

phase locked loops

Page 11: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Phase detector stability test

• Blue area is temperature stabilized• Signal paths to digitizer are not delay stable

– We are measuring the phase difference between signal and reference– The calibration signal presents a common mode signal to both paths,

so that differential delay changes can be subtracted out

signal

calibration (common mode)

reference

2856MHz

Page 12: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Phase stability test results

• 24 hours, 125kHz bandwidth, 2856MHz input• Uncorrected differential temporal error, 140fs RMS• Corrected differential temporal error, 15fs RMS• We are close to the theoretical limit, given the the noise figure of the

components

Page 13: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

We tested a dual channel system

• Opt. Lett. 34, 3050 (2009)• Measurement of the differential phase variation between two stabilized links

1560nm

Rbfreq.locker

0.01C

ref.arm

AM

RF inRF in

CWfiberlaser

0.01C

+50MHz

RF phasedetection

andcorrection

ref.arm

RF in

2km

+50MHz

opticaldelay

sensing

delaydata

phasedata

Page 14: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Dual-channel results

• 1kHz bandwidth• For 2.2km, 19fs RMS over 60 hours• For 200m, 8.4fs RMS over 20 hours• 2-hour variation is room temperature

time, hours

dela

y er

ror,

fem

tose

cond

s

time, seconds

Alla

n de

viat

ion

2km data

2.2km

200m

Page 15: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

We correct for group versus phase delay

group error asfiber heats

1.6% correction added

36fsRMS

• Group delay is not equal to phase delay, due to dispersion

• A temperature dependent Sellmeier equation was fitted to previous data by Ghosh et al (IEEE JLT 12, 1338)

• We correct for group delay by adding RF delay proportional to the optical correction

ϖ+= nng ϖddn

)(2 TAn = )/)(1()(

)/)(1()(

22 λλ TETD

TCTB

−+

−+ %1)()( ≅− TnTng

dTdn

dTdng ≠and also

early testwith and withoutfeedforwardcorrection:

Page 16: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

We determine the additional correction by adjusting to minimize error in situ

• Adjust feedforward correction until error is minimized• We don’t find significant changes to this factor

– Tested mainly on multi-fiber SMF cable

TXRX2 VCO

tuneRF in

fiberundertest

shortfiber

RX1

Page 17: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Power-to-phase conversion in the photodiode is not a problem

• Near saturation, high density of photocarriers screens applied field– Carriers are not swept out, response is slowed– Why it’s not monotonic is unclear, but it’s useful

• +/- 10% power variation around zero slope point causes <10fs time shift• In practice, power is stable to this degree and we don’t have to regulate

– This is an option

-1

-0.8

-0.6

-0.4

-0.2

0

0.2

0 2 4 6 8 10 12

optical power, mW

CWlaser

attenuator

networkanalyzer

RFamp

mod

photodiode

2GHz

powermeter

data and fit fortwo diodes

Page 18: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Manufacturer knows about this, is improving diodes

• Their results were for pulses, 1GHz harmonic • We need to test these with modulated CW, which has much smaller effect• At least we don’t have to worry the effect will get worse

– New zero slope point is OK, reduces power requirements

Joshi and Datta, IEEE Phot. Tech. Lett. 21, 1360 (2009)

Page 19: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

LCLS timing scheme

• We sync to bunch arrival time monitor• The laser is treated as a VCO

undulator

phasecavity

arrivaltimemonitor

receiver

near-end hall

X6476

φ

φ

receiver

laser

experiment

modulator

CW laser

X6

divider

476

2856 and 68

120Hztrigger

sender

e-

timing information

~150m

2856

4.25

2856

Page 20: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

2-channel, out-of-loop, in situ test

• 27fs RMS in 125kHz BW• 16fs RMS in 1kHz BW• Drift is due to short cable

between receivers, room temperature

TXRX2 VCO

tune

fiberRF in

300m

5m

RX1

2856MHz

Page 21: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Laser locking configuration

• Phase compare at 2856MHz• Sync first to 68MHz to remove “bucket ambiguity”• Works better than the commercial lockbox• New arrangement uses faster diode, eliminates X6 multiplier

harmonicout (476)

sync head

RF in

RF phasedetect

andcorrect

RF out(cal.)

RF in

frep out (68)

X6

laser68 MHzpulse trainreference 2856MHz

and 4.25MHzpiezo

Page 22: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

In-loop results

• Improvements to the laser should decrease high frequency noise– Acoustic and vibration isolation– Lower noise pump

Laser control error signal125kHz BW (gray): 120fs RMS1kHz BW (black): 25fs RMS

RF control error signal125kHz BW (gray): 31fs RMS1kHz BW (black): 8fs RMS

Page 23: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

The transmitter fits in a standard rack

• VCO

• Receiver (for laser)

• Splitter

• Diagnostic

• Amplifier

• Modulator

• Wavelength locker

• CW laser

Page 24: Results from CW stabilized link timing distribution at LCLS · Results from CW stabilized link timing distribution at LCLS Russell Wilcox Gang Huang. Larry Doolittle. John Byrd. John

Conclusions, future work

• We have demonstrated a laser-to-RF sync system in an FEL– 16fs between two RF channels, 25fs laser loop error (1kHz)– Used reliably for experiments (as reported earlier)

• Easily manufacturable, expandable– First commercially produced subsystems being tested– LCLS is engineering next version, will be making 8 channels soon,

upgrading transmitter to 16 channel capability

• Future work– Improve laser control– Better synchronization measurements– Try higher frequencies