femtosecond optical synchronization systems for xfels
DESCRIPTION
Femtosecond optical synchronization systems for XFELs. A. Winter, F. Ö. Ilday, J. Chen, F. Kärtner, H. Schlarb, F. Ludwig, P. Schmüser DESY Hamburg, MIT 19.9.2005 LLRF Workshop, CERN Oct. 2005. Overview. Requirements Optical synchronization systems Conclusion and Outlook. - PowerPoint PPT PresentationTRANSCRIPT
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Femtosecond optical synchronization systems for XFELs
A. Winter, F. Ö. Ilday, J. Chen, F. Kärtner, H. Schlarb, F. Ludwig, P. Schmüser
DESY Hamburg, MIT 19.9.2005
LLRF Workshop, CERN Oct. 2005
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Overview
• Requirements
• Optical synchronization systems
• Conclusion and Outlook
•Optical master oscillator•Optical timing distribution•RF reconversion•Synchronization of other laser systems•Test in accelerator environment
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Requirements
• Provide stability ~x-ray pulse width (down to ~10 fs)– Amplitude and phase stability in cavities (10-4, 0.01deg) in most
critical sections– Provide ultra-stable reference to select locations with
femtosecond stability – Synchronize probe systems to reference with ~10 fs stability
• Precise reference frequency generation and distribution system required– “femtosecond” synchronization means systems follow reference
with low added timing jitter and have intrinsic high-frequency timing jitter both, ~fs
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Master LaserOscillator
stabilized fibers
fiber couplers RF-optical
sync module
RF-opticalsync module
low-level RFlow-noisemicrowaveoscillator
low-bandwidth lock
remote locations
Synchronization System Layout
• A master mode-locked laser producing a very stable pulse train• The master laser is locked to a microwave oscillator for long-term stability
• length stabilized fiber links transport the pulses to remote locations• other lasers can be linked or RF can be generated locally
Optical to opticalsync module Laser
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Timing stabilized fiber linksPZT-based
fiber stretcher
Master Oscillator
SMF link 1 - 5 km
isolator50:50
coupler
fine cross-correlator
“coarse”RF-lock
Output coupler
FaradayMirror<50 fs
ultimately < 1 fs
• transmit ~500 fs pulses via dispersion compensated fiber links• assuming no fluctuations faster than T=2nL/c.
L = 1 km, n = 1.5 => T=10 µs, fmax = 100 kHz
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Optical Pulse Train(time domain)
TR = 1/fR
f… ..
fR 2fR nfR (n+1)fR
BPF
Photodiode
fnfR
t
TR/n
LNA
Direct Detection to Extract RF from the Pulse Train
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Timing jitter measurements
• signal converted to electronic domain by photodector• harmonic (~1GHz) or repetition rate filtered• phase noise measured with Signal Source Analyzer
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Amplitude noise of various fiber laser
0.03% rms for Er-doped fiber laser (EDFL)0.04% rms for Yb-doped fiber laser (YDFL)0.1% rms for Ti:Sapphire
Some of the quietest lasers around (3x-10x better than typical TiSa)
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Timing Jitter of fiber lasers
• All measurements scaled to 1 GHz • Noise floor limited by photodetection• Theoretical noise limit ~1 fs
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Direct seeding laser systems
Er-doped fiber
input pulse(~500 fs)
pump coupler
975 nm pump diode
single-mode fiber
~100 fs @ 775 nmto Ti:Sapphire
amplifier
SHG
PPLN
Direct seeding a Ti:sapphire amplifier after pulse shaping with self-compression to ~100 fs (~1 nJ @ 1550 nm & ~0.3 nJ @ 775 nm)
Nonlinear pulse shaping
(amplifier & compression)
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Direct seeding laser systems
Er-doped fiber
input pulse
stretcher fiber
pump coupler
975 nm pump diode
bulk grating compressor
(high energy)
air-core photonic crystal fiber (< 1 uJ)
OR
10 uJ, ~100 fs pulses at
1550 nm
975 nm pump diode
Amplification to high energy with nonlinear pulse shaping (~1 J @ 1550 nm, low repetition frequency)
Er-doped fiber
input pulse(~500 fs)
pump coupler
975 nm pump diode
single-mode fiber
~100 fs @ 775 nmto Ti:Sapphire
amplifier
SHG
PPLN
Direct seeding a Ti:sapphire amplifier after pulse shaping with self-compression to ~100 fs (~1 nJ @ 1550 nm & ~0.3 nJ @ 775 nm)
Nonlinear pulse shaping
(amplifier & compression)
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Very little amplitude noise added
0.033%
0.018%
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Very little phase noise added
29 fs
27 fs
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System Test in Accelerator environment
• Can lab results be transferred to real environment ?
• Test done at MIT Bates laboratory:– Locked EDFL to Bates master oscillator
– Transmitted pulses through 1km total of laid out fiber
– Close loop on fiber length feedback
~ 500 meters
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Setup
•1km return of fiber
•Passive temperature stabilization of 500 m
•RF feedback for fiber link
•EDFL locked to 2.856 GHz Bates master oscillator
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Results
• Fiber link extremely stable without closing loop (60 fs for 0.1 Hz…5 kHz)• Closing feedback loop reduces noise (12 fs for 0.1 Hz .. 5kHz)• No significant noise added at higher frequencies
• Can be stabilized to eventually sub-fs level using optical cross-correlation.
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Transmitted frequency
• Added jitter due to phase lock: ~30 fs (10 Hz..2 kHz)• Total jitter added (link, phase lock, increase at high frequency) < 50 fs• Overall improvement 272 fs vs. 178 fs (10Hz .. 20 MHz)• Spurs are technical noise!
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Conclusion and Outlook• Successful demonstration of complete system in accelerator
environment over 1 km fiber link
• sub-20 fs jitter added during transmission (0.1Hz .. 20MHz)
• 178 fs absolute phase noise limited by MO (10Hz .. 20 MHz)
• Most timing jitter is technical noise which can be eliminated.
• Stable, uninterrupted operation over weeks.
• Following a few years of development: < 10 fs