Long-distance frequency transfer over an urban fiber link
using optical phase stabilization
H. Jiang,1 F. Kéfélian,2 S. Crane,1,3 O. Lopez,2 M. Lours,1 J. Millo,1 D. Holleville,1
P. Lemonde,1 Ch. Chardonnet,2 A. Amy-Klein,2 G. Santarelli1,*
1LNE-SYRTE, Observatoire de Paris, CNRS, 61 avenue de l'Observatoire, 75014 Paris, France
2Laboratoire de Physique des Lasers (LPL), UMR 7538, CNRS and Université Paris 13, 99 av. J.-
B. Clément, 93430 Villetaneuse, France
3Permanent address: United States Naval Observatory, 3450 Massachusetts Avenue NW,
Washington, DC 20392, USA
*Corresponding author: email@example.com
We transferred the frequency of an ultra-stable laser over 86 km of urban fiber. The link is
composed of two cascaded 43-km fibers connecting two laboratories, LNE-SYRTE and LPL
in Paris area. In an effort to realistically demonstrate a link of 172 km without using spooled
fiber extensions, we implemented a recirculation loop to double the length of the urban fiber
link. The link is fed with a 1542-nm cavity stabilized fiber laser having a sub-Hz linewidth.
The fiber-induced phase noise is measured and cancelled with an all fiber-based
interferometer using commercial off the shelf pigtailed telecommunication components. The
compensated link shows an Allan deviation of a few 10-16 at one second and a few 10-19 at
OCIS codes: 060.2360, 120.3930.
The transfer of ultra-stable frequencies between distant laboratories is required by many
applications in time and frequency metrology, fundamental physics, particle accelerators and
astrophysics. Remote clock comparisons are currently performed using satellites, either directly by
Two-Way Satellite Time and Frequency Transfer, or indirectly through the Global Positioning
System carrier phase measurement. However, both methods are limited by instability of 10-15 after
one day of averaging time  and are consequently insufficient to transfer modern cold atom
microwave frequency standards having demonstrated frequency stability of a few 10-16 at one day
Progress on satellite-based links may lower the noise floor to the 10-16 range at one day and
advanced space missions such as “ACES” (Atomic Clocks Ensemble in Space)  and “T2L2” 
are being designed to make comparisons in the high 10-17 at one day. However, even if achieved,
such performance would be insufficient for the next generation of optical clocks. Optical clocks
using a trapped single ion or cold atoms confined in lattice are expected to reach instability level of
10-17 or better at one day and will consequently require even more stable frequency transfer systems
[5,6]. Moreover the assets of the accuracy and stability of the optical clock are critically related to
an efficient way to compare remote clocks with short averaging time. Beyond metrology, high-
resolution clock comparison is essential for advanced tests in fundamental physics, such as tests of
the fundamental constants stability .
To overcome current space link limitations, the transmission of frequency standards over
optical fiber has been investigated for several years . This technique takes advantage of the fact
that fiber has low attenuation, high reliability and the potential for phase noise cancellation.
Microwave frequency transmission using amplitude modulation of an optical carrier
demonstrated instability as low as 2×10-18 at one day over 86 km [9,10,11]. Direct optical frequency
transfer [12,13,14,15] can provide even better stability and be extended to greater distance. Indeed,
optical frequency transfer is less sensitive to link attenuation, due to heterodyne detection. In
addition, the higher carrier frequency gives much better resolution for measuring link-induced
phase noise. In 2007, two pioneering experiments of optical frequency transfer over a fiber link of
more than 200 km were reported [13,14]. Both experiments used fiber spool extension of an urban
link and demonstrated the feasibility of a full optical link with instability in the 10-18 range. Since
last year several German research laboratories have been connected by 1000 km of dedicated fiber
from the national research network and the stabilization of the link is under development .
These are the first milestones towards continental scale fiber links.
In this paper, we report the transmission of a sub-Hz linewidth optical frequency reference
over an 86 km length, which we doubled in a second step to an extended length of 172 km through
a recirculation loop. After the description of the cavity-stabilized laser used to test the link, we
present the scheme of the link-induced phase noise compensation system. The frequency stability
performance of an 86-km urban fiber link is then reported and, finally, the link length is extended to
172 km and characterized.
2. LASER SOURCE
Two identical ultra low noise laser sources have been developed using 1542-nm 1-2-kHz linewidth
commercial fiber lasers stabilized on two identical ultra-stable cavities by the Pound-Drever-Hall
method . The cavity consists of a 10-cm ULE spacer and two optically contacted ULE mirrors,
giving a measured finesse of ~ 800,000. The cavity, specially designed to minimize the vibration
sensitivity in all spatial directions , is mounted horizontally and sits on four Viton pads. It is
placed in a vacuum chamber with pressure below 10-7 mbar and the entire system is on a vibration-
isolation platform in an acoustical isolation box. About 2 μW of optical power, including ~ 30% in
the phase modulation sidebands, are typically sent onto the cavity with a coupling efficiency better
than 60%. A 350-kHz bandwidth locking is achieved using a double-pass acousto-optic modulator
with a cat’s eye retroreflector. The stabilized output of the laser can provide up to 10 mW of optical
To measure the laser frequency noise power spectral density, the two independent cavity
stabilized lasers are mixed on a photodetector, and the down-converted beat-note signal is measured
with a dynamic signal analyzer after frequency-to-voltage conversion. The phase noise power
spectral density versus Fourier frequency of the laser is presented on Fig. 1. Except for some
spurious peaks between 40 Hz and 100 Hz, it is largely below the phase noise of a 1-Hz linewidth
white frequency noise laser (dashed line on Fig. 1). The integrated phase noise from 1 Hz to 10 kHz
is below 0.2 rad rms (root mean square). The fractional frequency instability (Allan deviation) was
also calculated from the frequency counted beat-note signal and was found less than 2×10-15 at 1 s
and 10-14 at 100 s after a 0.3-Hz/s drift was removed.
3. COMPENSATED LINK SETUP
Fig. 2 shows the scheme of the compensated link based on the principle first described in . The
ultra-stable laser light is divided into two parts using a fiber coupler. One arm provides the
reference signal for stability measurement and fiber-induced phase noise compensation, while the
other arm is connected to the link through an optical circulator (OC) followed by acousto-optic
modulator AOM1 (with frequency f1 ≈40 MHz). To compensate for the phase noise φp accumulated
along the fiber due to acoustical, mechanical and thermal perturbations, part of the signal at the
remote end is retraced back to the link through an optical circulator, after frequency shifting by
acousto-optic modulator AOM2 (with frequency f2=70 MHz). This return signal, which passes
twice through the link and experiences a phase noise 2φp, is mixed at the local end with the
reference signal on photodiode PD1. The beat note at frequency 2f1+f2 is phase locked to a stable
RF synthesizer using AOM1 driven by a voltage controlled oscillator. The phase-lock loop applies
the correction φc=-φp to the AOM1 frequency f1, thus to the optical signal phase and consequently
actively cancels the fiber-induced phase noise at the remote end of the fiber link. To magnify the
dynamic range of the servo loop and hence improve its robustness, a digital frequency divider by 40
has been used just ahead of the phase detector. The optical frequency (phase) instability of the link
is defined as the difference between the local and remote end optical frequencies (phases). It is
measured on the beat-note at frequency f1+f2 provided by mixing the single trip and the reference
optical signals on photodiode PD2. Two polarization controllers are employed for optimizing the
beat-note signal amplitudes. The compensation system is entirely fibered and uses only commercial
off the shelf pigtailed telecommunications components.
4. TRANSMISSION OVER 86 KM
LPL and LNE-SYRTE, located in Paris area, are linked by a pair of 43-km telecommunication
fibers. Each fiber is composed of various sections of buried cables of the metropolitan network
spliced together. The attenuation of each fiber is about 12 dB. By connecting the two ends of the
fibers at LPL, the link length is extended to 86 km with local end and remote end both located in
Fig. 3 shows the 86-km link optical phase noise power spectral density versus Fourier frequency,
without and with compensation. The beat note provided by PD2 is frequency divided by 40 and
down mixed to DC, the phase noise power spectral density is then measured with a dynamic signal
analyzer. It exhibits a roughly 1/f 2 roll-off from 1 Hz to 100 Hz with a wide bump between 10 Hz
and 100 Hz, and 1/f 4 behavior above 100 Hz. The integrated phase noise from 1 Hz to 1 kHz is
equal to 19.2 rad and 0.4 rad (rms), without and with compensation respectively (corresponding to
15 fs and 0.3 fs rms timing jitter). Beyond 1 kHz, the phase noise rolls down to the measurement
system floor and is negligible. The 0.4 rad (rms) corresponds to 85% of the optical power in the
carrier. The phase noise of the transmitted laser is only slightly degraded by the transfer and the
laser coherence time is therefore preserved at the output of the compensated link. This is an
important point for applications requiring distribution of narrow linewidth sources.
Laser phase noise can corrupt the link-induced phase noise measurement. Indeed, on PD2
are mixed two optical signals coming from the same source but delayed by 430-µs (due to the 86-
km propagation in the fiber). This generates on the beat-note signal a delayed self-heterodyne
interferometric phase noise  due to the laser phase noise, in addition to the link-induced phase
noise to be compensated. This additional phase noise contribution can be calculated from the laser
phase noise (shown on Fig. 1) and is displayed in Fig. 3 (c). It shows that the laser phase noise is
sufficiently low and does not limit the performance of the stabilization.
Fig. 4 displays the experimental fiber-induced optical phase noise rejection for the 86-km
link versus Fourier frequency calculated by dividing the phase noise power spectral densities of the
compensated and uncompensated links. We have performed the Laplace domain analysis of the
compensation scheme and obtain an analytical expression of the rejection transfer function (black
dashed line on Fig. 4) . This analysis reveals that the optimum proportional gain is about the
inverse of the link single trip time (2300 for an 86-km link) and that the rejection frequency
bandwidth is limited to 1/4ttrip (~ 600 Hz) where ttrip is the one-way trip delay in agreement with
. Moreover, this analysis shows that the integrator used in the phase-lock loop improves
rejection only in a limited frequency range. Indeed, as already pointed out in , at low frequency
the rejection is limited by the link delay and scales as (f.ttrip)2 (red dotted line on Fig. 4)
independently of the loop gain. Our calculations are in good agreement with the measurements as
shown on Fig. 4.
For long term frequency stability characterization, the Allan deviation is the most common tool
and is typically obtained using frequency counter measurements. The original Allan deviation
defined in  can only be calculated from frequency samples obtained with a classical, or “π-type”,
counter using a uniform average over the measurement gate time. Indeed, modern enhanced-
resolution, or “Λ-type”, counters have been shown to lead , not to the classical Allan deviation,
but to a quantity proportional to the modified Allan deviation . Consequently, we measure the
classical Allan deviation of the fractional frequency instability introduced by the link with a four-
channel π-type frequency counter. This counter is dead-time free in order to avoid bias in the
calculation of the Allan deviation . We measure simultaneously the frequency instability of the
compensated link and the frequency instability of the compensation signal (at the voltage controlled
oscillator output), which represents the free running fiber frequency noise. The beat-note between
the remote end and local end optical signals provided by PD2 is frequency divided by 40 and band
limited by a tracking filter based on a low noise quartz oscillator giving a measurement bandwidth
of ~10 Hz. This bandwidth is larger than the inverse of the gate time.
Fig. 5 shows the fractional frequency overlapping Allan deviation of the 86-km link with and
without compensation for several days of continuous operation. The Allan deviation scales down
with a 1/τ slope from 1 s to 100 s. The bump at 250 s, which corresponds to the half cycle time of
the air conditioning system, is due to thermal effects in the sections of the interferometric system
that are not actively compensated. After 1000 s of averaging time, the Allan deviation levels off in
the low 10-19 range probably also limited by the uncompensated section of the system. Without
filtering, the Allan deviation is 10 times higher. This is consistent with the fact that the Allan
deviation of a white phase noise is proportional to the square root of the noise bandwidth.
5. TRANSMISSION OVER 172 KM
Previous extended link results have been demonstrated by adding spooled fiber to an urban link
[13,14,15]. To simulate a longer link with a more realistic phase noise, we devised a new scheme,
represented in Fig. 6, to pass twice through the 86-km link leading to a full urban link of 172 km.
The optical signal is fed into the 86-km link through an optical coupler. At the end of the 86-km
link, a “frequency shifter mirror” is connected. This “mirror” consists of a unidirectional loop based
on an optical circulator and an acousto-optic modulator. An Erbium doped fiber amplifier (EDFA1)
with 17-dB gain is also implemented in order to compensate for losses due to recirculation (12 dB
due to the double pass combiner losses, 5 dB due to the optical circulator and AOM2 losses). As a
result, this is equivalent to a 172-km span link without intermediate optical amplifier and the
resulting phase noise is similar to the noise of a real 172-km telecom network link. A second optical
amplifier (EDFA2) was added at the remote end to amplify the return signal. Temperature
variations in EDFAs induce phase fluctuations, which degrade the long-term frequency stability. In
order to correctly compensate for this effect, the output optical signal should pass once through the
EDFAs when the round trip signal should pass twice. This is naturally the case for EDFA1, but not
for EDFA2. This is overcome by adding a recirculation loop around EDFA2. To easily identify the
output and round trip signals AOM3 is inserted in this loop. At the output of PD1 the beat-note
signal at frequency 2(f1+f2)+f3+f4 is appropriate for link compensation while at the output of PD2
the beat-note signal at f1+f2 is used to derive the link stability (fi is the frequency of the AOM i).
This set-up could be simplified by using a bi-directional EDFA.
Fig. 7 displays the 172-km link phase noise power spectral density, without and with
compensation. As expected, the correction bandwidth is half the one obtained for the 86-km link
due to a double roundtrip delay. Moreover, at low frequency, the fiber-induced phase noise
rejection is 4 times lower than with the 86-km link, in agreement with the delay-limitation effect
discussed in section 4. The integrated phase noise from 1 Hz to 1 kHz is equal to 53 rad and 2.4 rad
(rms), without and with compensation respectively.
Fig. 8 shows the fractional frequency instability of the 172-km link. The Allan deviation is
about 4×10-16 at 1 second and in the range of 10-19 at 1 hour with a 10-Hz measurement bandwidth.
The system floor is measured by replacing the urban fiber with an optical attenuator having the
In addition to data obtained with π-type counter we have used a Λ-type counter, without the
10-Hz filter, to allow comparison with the results of [14,15] obtained with 76 km of urban fiber,
175 km of spooled fiber and four in-line EDFA. To avoid dead-time, the gate time of the counter
was set equal to the averaging time for averaging time ≤ 100 s. Data obtained with Λ-type counter
are shown with green star points on Fig. 8. They are better than with π-type counter, due to an
additional filtering of the phase noise. The Allan deviation is calculated for every averaging time
with the classical formula and not with the modified Allan deviation (as in reference [14,15] for
averaging time >10s). Indeed, when original Allan deviation formula is used, Λ-type counters report
directly a quantity similar to the modified Allan deviation. For comparison, the use of the modified
Allan deviation would lead in our case to a reduction factor of 2/3 on the Allan deviation for
averaging time above 100 s. Results are found similar to the data presented in [14,15]. Data
obtained with longer averaging times show that frequency instability keeps falling off until 5000 s
and reach 3×10-19 with the Λ-type counter at 3000 s.
Comparison between the two configurations is not straightforward. First, the link noise
process is not time stationary due to urban environmental fluctuations. Moreover when the length of
the fiber is virtually doubled by the recirculation technique the phase noise power spectral density
of the free running link is twice the one of a single pass double length fiber, as detailed below.
Under the assumption that the fiber phase noise is uniformly spatially distributed, the phase
noise power spectral density is proportional to the length of the fiber. However, with the
recirculation technique the laser wave experiences twice the phase fluctuation at each point of the
fiber. These two contributions of each point are correlated for times longer than the single span
fiber delay tfiber, they therefore add up coherently. Consequently, for Fourier frequencies below
1/4tfiber, the phase noise power spectral density of a 2L-km link realized by recirculation is expected
to be four times that of an L-km fiber. One can therefore anticipate that the phase noise power
spectral density for the recirculated link is twice larger than would be expected for a real link of
172-km. Consequently the stability results obtained for the recirculated link should be considered
as an upper bound for a real link of the same length.
It is conceivable to extend the length of the link up to continental scales, 1000 km or more.
In a single segment approach however, major difficulties will arise. Firstly, fiber attenuation will
make mandatory in-line bidirectional amplifiers in order to provide sufficient power at the output
and allow phase locking at the local end. As discussed in section 5, bidirectional amplifiers phase
noise is cancelled within the control bandwidth. However, when cascading amplifiers, amplified
spontaneous emission can be very large and will require the use of narrow band optical filters to
overcome a significant degradation of the signal-to-noise ratio at both ends [14, 15]. Secondly, the
reduced bandwidth of the servo-loop and the reduced noise rejection level both due to the delay
effect (See Section 4) will degrade the performance of the transmission. We have empirically
observed that the phase noise exhibits a 1/f2 dependence in the free running link. Assuming a linear
dependence of the phase noise power on the length of the link L Allan deviation scales as L3/2
[14,15]. One could hence expect an Allan deviation below 10-14 at one second for a 1000-km single
segment link in a 10-Hz measurement bandwidth, averaging down as 1/τ to the noise floor of the
An alternative approach is to split the long distance link in shorter compensated segments
using intermediate stations. Each one will achieve three functions, to send back part of the received
signal to the previous station, to amplify (and filter if necessary) the received signal, to compensate
the phase noise induced by the following segment. The maximum distance of each segment will
depend on the fiber phase noise distribution, attenuation and on the total link length. This multiple
segment approach allows for an increased correction bandwidth and enhances the resolution of the
system. This would enable much better performance down to a level where the coherence of the
laser itself can be transferred, as demonstrated in section 4.
Beside the limitations due to the length of the link an other possible source of transmission
degradation is related to spurious back reflections which always occurs in a fiber system. They are
due to connector interfaces (typically -40dB to -60 dB), Rayleigh backscattering (typically -40 dB
with SMF fiber) and splicing points. These effects can be enhanced when online bidirectional
amplifiers are used. However, optical frequency transfer over fiber is not sensitive to single back-
reflection as back-reflected waves do not receive the correct frequency offsets from the AOMs in
our scheme and are consequently easily discriminated. This is not the case when double back-
reflections are considered. Double back-reflected waves lead to additional phase and amplitude
noise that is proportional to the fraction of the optical field double back-reflected. Since double
back-reflections occur identically on the way there and the way back, the double back-reflection
optical phase noise are also cancelled by the compensation system. Consequently, back-reflections,
even strong, do not limit the stability of the link.
We have demonstrated a long-distance link for metrological optical frequency transfer using optical
phase stabilization over a dedicated fiber that lies buried beneath the urban environment of Paris,
France. Frequency transfer was demonstrated with instability of 1.5×10-16 at 1 s and integrates down
to the range of 10-19 at 500 s over 86 km. We have simulated a link at twice this distance via
recirculation in the fiber to represent the phase noise of a 172-km urban link. It shows instability of
4×10-16 at 1 s and a few 10-19 at 10,000 s, which is better than the anticipated performance of optical
To broaden the use of this technique to more users and reach longer distances, an appealing
solution is to use the existing research, educational as well as commercial optical communication
networks that connect a large number of physics laboratories. This will require addressing several
difficulties. For instance, such a link will have to coexist with telecommunication traffic via the use
of wavelength division multiplexing. Another crucial point is that fibers in classical optical
telecommunication networks are used in a unidirectional way, whereas the compensation technique
will require bi-directional operation. Yet one more significant hurdle being that restricted access to
the fiber network infrastructure will require the design of an ultra-stable link that functions in a
virtually flawless fashion. We are currently developing solutions to make compatible the frequency
transfer technique and the optical communication networks, in particular to bypass unidirectional
optical amplifiers and to allow the transparent coexistence of the ultrastable signal and the data
modulated signal. This is the next challenging step towards a network for ultra stable frequency
We acknowledge funding support from the Agence Nationale de la Recherche (ANR BLAN06-
3_144016). SYRTE is a Unité Mixte de Recherche of CNRS, Observatoire de Paris and UPMC.
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Fig. 1. Phase noise power spectral density versus Fourier frequency of the stabilized laser (solid line)
and of a 1-Hz linewidth white frequency noise laser (dashed line)
Fig. 2. Full scheme of the optical frequency transfer over fiber; AOM: acousto-optic modulator; PD:
photodiode; PLL: phase locked loop; PC: polarization controller: OC: optical circulator; RF synth:
Fig. 3. Phase noise power spectral density versus Fourier frequency of the (a) free running, (b)
compensated 86-km link and (c) delayed self-heterodyne beat note. Dashed line represents the
phase noise of a 1-Hz linewidth laser.
Fig. 4. Fiber noise rejection for 86-km link, experimental data (blue line) and analytical data with
proportional gain equal to 2300 and integrator gain equal to 50 (black dashed line). Red dotted line
represents the delay-induced rejection floor.
Fig.5. Fractional frequency instability of the 86-km free running link (blue triangle) and
compensated link (black squares), versus averaging time. The measurement frequency bandwidth is
Fig. 6. Scheme of the 172-km link (EDFA : Erbium Doped Fiber Amplifiers, AOM, PD, see Fig.3.)
Fig. 7. Phase noise power spectral density of the (a) free running, and (b) compensated 172-km link.
Fig. 8. Fractional frequency instability of the 172-km free running link (blue triangle), compensated
link with 10-Hz measurement bandwidth (black squares), and with Λ-type counter (green stars).
Empty triangles correspond to the experimental set-up floor (see text).
Phase noise power spectral density [rad
Fourier Frequency [Hz]
Phase noise power spectral density [rad
Fourier Frequency [Hz]
Rejection transfer function
Fourier Frequency [Hz]
proportional gain limited
Averaging Time [s]
EDFA 1EDFA 1
EDFA 2 EDFA 2
" Mirror "
See Fig. 2
See Fig. 2
Figure 7 Download full-text
Phase noise power spectral density [rad
Fourier Frequency [Hz]
Averaging time [s]