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International Journal of Trend in Scientific Research and Development (IJTSRD)
Volume 3 Issue 5, August 2019 Available Online: www.ijtsrd.com e-ISSN: 2456 – 6470
@ IJTSRD | Unique Paper ID – IJTSRD26390 | Volume – 3 | Issue – 5 | July - August 2019 Page 580
Study of Rotation Measurements with a Passive
Resonant Gyroscope Based on Hollow Core Fiber
Dr. Vinay Kumar Chaudhary
Assistant Professor, Department of Physics, Nalanda Collage of Engineering, Gokhulpur, Bihar, India
How to cite this paper: Dr. Vinay Kumar
Chaudhary "Study of Rotation
Measurements with a Passive Resonant
Gyroscope Based on Hollow Core Fiber"
Published in
International
Journal of Trend in
Scientific Research
and Development
(ijtsrd), ISSN: 2456-
6470, Volume-3 |
Issue-5, August
2019, pp.580-584,
https://doi.org/10.31142/ijtsrd26390
Copyright © 2019 by author(s) and
International Journalof Trendin Scientific
Research and Development Journal. This
is an Open Access article distributed
under the terms of
the Creative
CommonsAttribution
License (CC BY 4.0)
(http://creativecommons.org/licenses/by
/4.0)
ABSTRACT
We present rotation measurements performed with apassiveresonantoptical
fibre gyroscope. The fibre used to realize the resonant cavity was a Kagome
Hollow Core Fiber. Measurements were performed in two types of
configurations. In the first configuration, the counter propagating beams
resonate on the same cavity mode. This leads to observation of lock-in that
prevents measuring rotation rates below roughly 1°/s. In the second
configuration, the counter propagatingbeamsresonateon twodifferentcavity
modes. This leads to rotation rates measurements below 0.1°/s that are
currently limited by some drifts. We will describe in the conference possible
sources of drifts and the solutions we consider to circumvent them.
KEYWORDS: Backscattering, hollow core fiber, lock-in, passive resonant
gyroscope
I. INTRODUCTION
Recent progresses in hollow-core photonic crystal fibers (HC-PCF) and the
availability of compact and affordable single-frequencylasersrenewed interest
for resonant fiber optic gyroscope (R-FOG) [1]. Indeed, hollow-core fibers,
where light propagates mostly in air, have the advantage of significantly
reducing the Kerr effect, known as a strong limitation on thebias stabilityof the
R-FOG [2]. However, Rayleigh backscattering is still an important source of
noise as it forbids the measurements of low rotation rates [3]. Moreover
hollow-core fibres are known to exhibit quite high Rayleigh backscattering
coefficient, as defined in [4]. In previous work [5], 25 times larger Rayleigh
backscattering coefficient than that of usual single mode fiber was reported.
In [6] and [7], we indeed confirmed this tendency with
PhotonicBand GapandKagomefibersbymeasuringRayleigh
backscattering coefficientsbetweenroughly1to4×10-6m-1.
This explains why we focused on testing methods to reduce
theeffect of thebackscattering thatwe willpresentinsection
IV. Before, we first describe the optical cavity used for the
tests and then show indeed what type of dead zone we
measure.
II. FIBER AND CAVITY DESCRIPTIONS
The cavity was realized with 18m of a Kagome Fiber (see
Fig.1) designed and fabricated by XLIM and coiled with a 50
cm diameter. The fiber has anexternal diameter of435µmto
reduce its sensitivity to environmental perturbationssuchas
vibrations, acorediameter of61µmcorrespondingtoamode
field diameter of 45µm. The total transmission of this fiber
(i.e. taking into account the in/out coupling losses and the
propagation losses) is about 83 to 86% and very stable in
time (several weeks). This was not Always the case as we
could observe reductions of the transmission over time with
other fibers mainly with smaller core diameters (from 10 to
20µm). This was reported around to 1.4 µm [8] and due to
surface OH–. In our case, at 1.55µm, the origin remains
unclear (visual inspection confirmed thatthefiberendswere
clean of dust but the nanostructure appeared somehow
blurred).
Fig.1: Picture of one of the end of the fiber used and
schematic of the cavity
IJTSRD26390
International Journal of Trend in Scientific Research and Development (IJTSRD) @ www.ijtsrd.com eISSN: 2456-6470
@ IJTSRD | Unique Paper ID – IJTSRD26390 | Volume – 3 | Issue – 5 | July - August 2019 Page 581
The cavity coupling is realized in free-space with lenses L1,
L2, L3 and M1 mirror. M2 is a HR mirror and is used to
monitor the intracavity resonance through its leakage and
used to ease the alignment. The cavity is fiber-coupledtothe
external probe beams through lenses L1. Its resonance
curves, obtained by injecting a clockwise beam in the cavity,
are shown in Fig. 2 and give a finesse, defined as the ratio of
the resonance peak Full Width Half Max over the Free
Spectral range, of 33 and a contrast, defined as the ratio
between the difference of the maximum and minimum
signals over the maximum one, close of 80%. The values are
close to what can be expected when simulating the cavity
taking into account the coupler M1 transmission of 6.6%.
The Free Spectral Range (FSR) is equal to 16.1 MHz. On the
contrary to what we reported in [9] based on [10], λ/2 wave
plates are required to control the polarization inside the
cavity. This is because the fiber is much more rigid and
cannot be twisted without risk of breaking it.
Fig.2: Resonance curves. Purple: transmitted beam
detected on the photodiode PD4 thru leakage of M2
(transmission < 0.01%). Blue: reflected beam detected by
a photodiode connected in place of the fiber injecting the
counter-clockwise beam. Yellow: voltage applied to the
probe laser
III. OBSERVATION OF A LOCK-IN ZONE
The complete schematics of the gyroscope is given in Fig. 3
and is similar to has been previously reported.
Fig. 3: complete gyroscope schematic with the injection
setup including
The external laser is split into two beams that are frequency
shifted by the acousto-optic modulators (AOM) to resonate
with the same mode of the cavity. The AOMs are used to
compensate the relative variations between thelaserandthe
cavity mode frequencies. The AOM frequencies are driven
through a Pound Drever Hall locking scheme [11]. Without
rotation, the RF signals applied to the AOM have the same
frequency. Under rotation, the frequencies are different
because of the Sagnac effect [12]. We plot the gyroscope
response curve in Fig. 4, i.e the difference between the two
AOM frequencies versus the rotation rate. Above 10°/s, the
response is linear. The scale factor is about 5 kHz/(°/s), in
agreement with an approximate (because of the real
geometry of the cavity and its free-space coupler) value that
can be calculated using the usual formula
4Æ n = 2r n =5.8 kHz/(°/s)
ßL 180 ß 180
where A = nr2, L = 2nr and 2r the cavity diameter. Below
10°/s, the response tends to shift away from this ideal linear
response. Below 5 to 6°/s, the behavior of the gyroscope
becomes noisy and chaotic, switching from a state where the
AOMs frequencies are identical (locked state) to a transient
state where they tend to be different making a more
quantitative analysis more difficult.
Fig. 4: gyroscope response curve
In Fig. 5 below, we show the difference between the
frequencies of the RF signals applied to the two AOMs
without rotation (except earth). It is in the few Hz range and
we believe is a signature of the lock-in phenomenon.
Fig. 5: time evolution (in s) of the frequency without
applied rotation
IV. METHOD TO REDUCE THE DEAD ZONE
Several methods havebeen proposedintheliteraturesuchas
suppression of the carriers [13]. An illustration of its
beneficial effects can be found in [16] for instance. More
sophisticated versions with complex modulation schemes
werealsodemonstratedin[14],[15].However,aspointedout
in [16], the effectiveness of this technique is limited by the
carrier suppression level.
International Journal of Trend in Scientific Research and Development (IJTSRD) @ www.ijtsrd.com eISSN: 2456-6470
@ IJTSRD | Unique Paper ID – IJTSRD26390 | Volume – 3 | Issue – 5 | July - August 2019 Page 582
We propose to test a different method in which we probe the
cavity with counter-propagating beams that resonate with
different modes of thecavity. This ensures that,evenwithout
rotation, the frequency splitting is not null. We tested this
configuration with two AOMs inducing frequency shifts
centered around +110MHz and -110MHz so that the counter
propagating beams are frequency- separated by 13 FSR.
Indeed, we were able to measure rotation rates down to
0.05°/s as can be seen on the improved gyroscope response
curve given in Fig. 6.
However, at such low rotation rates, the measurements
begin to be limited by slow fluctuations of the AOMs
frequencies without rotation as can be seen in Fig. 7. This
can be easily understood as the frequency splitting between
the two counter propagating waves in this configuration
depends not only of the Sagnac shift but also on the FSR that
is prone to fluctuate. However, when using two AOMs of the
same order (+1), so that the two resonating beam
frequencies are only separated by one FSR, we did not
observe the reduction (by a factor of roughly 20) of these
drifts that we expected.
Fig.6: improved gyroscope response curve without lock-in
Fig.7: Sagnac response of the gyroscope at a rotation rates
of ±0.05°/s. In order to retrieve the Sagnac phase shifts,
the AOMs frequency must be added explaining the average
value of 225 MHz.
We thus decided to implement a method to measure the FSR
and the rotation rate simultaneously that we describe in the
next section.
V. METHOD TO MEASURE BOTH THE CAVITY FREE
SPECTRAL RANGE AND THE ROTATION RATE
We previously reported such an architecture [17] in which
the laser beam was separated into three beams, two of them
circulating in the same direction in the cavity while thethird
one was counter circulating. One of them is used to lock the
laser while the two others are, as described in the section III
of this paper, frequency shifted by two AOMs. Each beam is
lockedonadifferentresonance andtheFSRandrotationrate
can be retrieved from the frequencies applied to the AOMs.
However webelieve this solution faces some limitationsdue
the locking of the laser (butitwould be the same if the cavity
length were locked on a stable reference laser). If for some
reasons, the laser is not at resonance anymore with the
cavity, the control loop will apply a correction signal to the
laser so that its frequency converges toward the cavity
resonance in a time depending on the control loop
bandwidth. However, this transient time during which the
laser frequency varies also impacts the AOM control loops
and induces some noises in the AOMfrequencies.
We thus tested a configuration (see Fig. 8) in which the laser
is not locked (frequency or shifts will impact in the same
manner the three beams) using three AOMs inducing
frequency shifts of 110, -110 and 42MHz.
Fig. 8: schematic of the gyroscope configuration with three
AOMs. The cavity FSR is now 16.4 MHz
Without rotation, combining the three AOM frequencies
gives three measurements of 13, 9 and 4 FSRs. The FSR
results are given in Fig. 9. As can be seen the FSR are rather
stable but there is a bias in the measurements.
Fig. 9: FSR measurements (in Hz) deduced from the
frequencies of the three AOMs
When one looks closer at the evolution of the three signals,
further problems appear, as shown in Fig. 10. The scales of
the fluctuations are not identical even whenthecurvesseem
International Journal of Trend in Scientific Research and Development (IJTSRD) @ www.ijtsrd.com eISSN: 2456-6470
@ IJTSRD | Unique Paper ID – IJTSRD26390 | Volume – 3 | Issue – 5 | July - August 2019 Page 583
to overlap. We are thus investigating the origins of these
discrepancies that could be many. Residual Amplitude
Modulation (RAM) could be one of the sources but we
implemented the scheme described in [18] and we do not
see any signature (at least with our level of accuracy) in the
electrical spectrums of the intensities after the phase
modulators. We are also investigating the symmetry of the
resonance peaks that is known to induce a bias if not good
enough.
Fig. 10: zoom on the FSR variations deduced from the
measurements of 4, 9 and 13 FSR.
VI. CONCLUSON
We report, for what we believe is the first time, observation
on the phenomenon of lock-in a passive resonant gyroscope
with hollow-core fiber. We demonstrated that this issue can
be solved by probing the cavity on two different modes.
Indeed, this approach leads to a reduction of the lock-in
threshold by several orders of magnitude. However, the
sensitivity of the gyroscope is then limited by the FSR
fluctuations. We propose and test architecture to measure
both the rotation rate and the FSR simultaneously. We also
present our ongoing efforts to reduce the discrepancies in
the FSR measurements for this architecture to enhance the
gyroscope performances. We will report at the conference
our latest progress in this direction.
REFERENCES
[1] G. A. Sanders, L. K. Strandjord, and T. Qiu, “Hollow core
fiber optic ring resonator for rotation sensing”, in
Optical Fiber Sensors 2006 (OpticalSocietyof America,
2006), paper ME6
[2] K. Iwatsuki, K. Hotate, and M. Higashiguchi,“Kerr effect
in an optical passive ring-resonator gyro,”J.Lightwave
Technol. 4, 645 (1986)
[3] F. Zarinetchi et S. Ezekiel, “Observation of lock-in
behavior in a passive resonator gyroscope”, Opt. Lett.
11, 401 (1986).
[4] P. Gysel, and R. K. Staubli (1990),“Statisticalproperties
of Rayleigh backscattering in single-mode fibers”,
Journal of Light wave Technology 8(4), 561-567.
[5] S. Lloyd, V. Dangui, M. Digonnet, S. Fan, and G. S. Kino,
“Measurement of reduced backscattering noise in
laser-driven fiber optic gyroscopes,” Opt. Lett., vol. 25,
no. 2, pp. 121–123,2010.
[6] A. Ravaille, G. Feugnet, I. Fsaifes, A. Baz, B. Debord, F.
Gérôme, G. Humbert, F. Benabid and F. Bretenaker,
(2017). In-situ measurement of backscattering in
hollow-core fiber based resonant cavities. IEEE
Photonics Journal, 9(4), 1-7.
[7] A. Ravaille, G. Feugnet, B. Morbieu, I. Fsaifes, A. Baz, B.
Debord, G. Humbert, F. Benabid and F. Bretenaker
(2017, June). Measurement of backscatteringin hollow
core photonic crystal fiber based resonant cavities. In
Lasers and Electro-Optics Europe & European
Quantum ElectronicsConference(CLEO/Europe-EQEC,
2017 Conference on) (pp. 1-1). IEEE.
[8] I. Gris-Sanchez and J.C. Knight(2012).Time-dependent
degradation of photonic crystal fiber attenuation
around OH absorption wavelengths. Journal of Light
wave Technology, 30(23), 3597-3602.
[9] I. Fsaifes, G. Feugnet, A. Baz, A. Ravaille, B. Debord, F.
Gérôme, G. Humbert, S. Schwartz, F. Benabid and F.
Bretenaker (2016, June). Hollow-core photonic-
bandgap fiber resonator for rotation sensing. InLasers
and Electro-Optics (CLEO), 2016 Conference on (pp.1-
2). IEEE.
[10] M. Terrel, M. J.F. Digonnet, and S. Fan, “Polarization
controller for hollow-core fiber”, Opt. Lett. 32, 1524
(2007).
[11] R. W. P. Drever, J.L. Hall, F.V. Kowalski, J. Hough, G. M.
Ford, A.J. Munley, H. Ward, H. (1983). Laser phase and
frequency stabilization using an optical resonator.
Applied Physics B, 31(2), 97-105.
[12] G. Sagnac (1913).L'éther lumineuxdémontrépar l'effet
du vent relatif d'éther dans un interféromètre en
rotation uniforme. CR Acad. Sci., 157, 708-710.
[13] K. Iwatsuki, K. Hotate and M. Higashiguchi (1984).
Effect of Rayleigh backscattering in an optical passive
ring-resonator gyro. Applied Optics, 23(21), 3916-
3924.
[14] K. Hotate, K. Takiguchi, and A.Hirose, ‘‘Adjustment-free
method to eliminate the noise induced by the
backscattering in an optical passive ring-resonator
gyro,’’ IEEE Photon. Technol. Lett., vol. 2, no. 1, pp.75-
77, Jan. 1990.
International Journal of Trend in Scientific Research and Development (IJTSRD) @ www.ijtsrd.com eISSN: 2456-6470
@ IJTSRD | Unique Paper ID – IJTSRD26390 | Volume – 3 | Issue – 5 | July - August 2019 Page 584
[15] K. Suzuki, K. Takiguchi, and K. Hotate, “Monolithically
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66–72, Jan. 2000.
[16] H. Ma, Z. He and K. Hotate (2011). Reduction of
backscattering induced noise by carriersuppression in
waveguide-type optical ring resonator gyro. Journal of
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[17] S. Schwartz, G. Feugnet, .B. Morbieu, N. El Badaoui, G.
Humbert, F. Benabid, I. Fsaifes and F. Bretenaker
(2017, November). New approaches in opticalrotation
sensing. In International Conference on Space Optics—
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[18] W. Zhang, M. J. Martin, C. Benko, J. L. Hall, J. Ye, C.
Hagemann, T. Legero, U. Sterr, F. Riehle, G. D. Cole and
M. Aspelmeyer(2014). Reductionofresidual amplitude
modulation to 1× 10-6 for frequency modulation and
laser stabilization. Optics letters, 39(7), 1980-1983

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Study of Rotation Measurements with a Passive Resonant Gyroscope Based on Hollow Core Fiber

  • 1. International Journal of Trend in Scientific Research and Development (IJTSRD) Volume 3 Issue 5, August 2019 Available Online: www.ijtsrd.com e-ISSN: 2456 – 6470 @ IJTSRD | Unique Paper ID – IJTSRD26390 | Volume – 3 | Issue – 5 | July - August 2019 Page 580 Study of Rotation Measurements with a Passive Resonant Gyroscope Based on Hollow Core Fiber Dr. Vinay Kumar Chaudhary Assistant Professor, Department of Physics, Nalanda Collage of Engineering, Gokhulpur, Bihar, India How to cite this paper: Dr. Vinay Kumar Chaudhary "Study of Rotation Measurements with a Passive Resonant Gyroscope Based on Hollow Core Fiber" Published in International Journal of Trend in Scientific Research and Development (ijtsrd), ISSN: 2456- 6470, Volume-3 | Issue-5, August 2019, pp.580-584, https://doi.org/10.31142/ijtsrd26390 Copyright © 2019 by author(s) and International Journalof Trendin Scientific Research and Development Journal. This is an Open Access article distributed under the terms of the Creative CommonsAttribution License (CC BY 4.0) (http://creativecommons.org/licenses/by /4.0) ABSTRACT We present rotation measurements performed with apassiveresonantoptical fibre gyroscope. The fibre used to realize the resonant cavity was a Kagome Hollow Core Fiber. Measurements were performed in two types of configurations. In the first configuration, the counter propagating beams resonate on the same cavity mode. This leads to observation of lock-in that prevents measuring rotation rates below roughly 1°/s. In the second configuration, the counter propagatingbeamsresonateon twodifferentcavity modes. This leads to rotation rates measurements below 0.1°/s that are currently limited by some drifts. We will describe in the conference possible sources of drifts and the solutions we consider to circumvent them. KEYWORDS: Backscattering, hollow core fiber, lock-in, passive resonant gyroscope I. INTRODUCTION Recent progresses in hollow-core photonic crystal fibers (HC-PCF) and the availability of compact and affordable single-frequencylasersrenewed interest for resonant fiber optic gyroscope (R-FOG) [1]. Indeed, hollow-core fibers, where light propagates mostly in air, have the advantage of significantly reducing the Kerr effect, known as a strong limitation on thebias stabilityof the R-FOG [2]. However, Rayleigh backscattering is still an important source of noise as it forbids the measurements of low rotation rates [3]. Moreover hollow-core fibres are known to exhibit quite high Rayleigh backscattering coefficient, as defined in [4]. In previous work [5], 25 times larger Rayleigh backscattering coefficient than that of usual single mode fiber was reported. In [6] and [7], we indeed confirmed this tendency with PhotonicBand GapandKagomefibersbymeasuringRayleigh backscattering coefficientsbetweenroughly1to4×10-6m-1. This explains why we focused on testing methods to reduce theeffect of thebackscattering thatwe willpresentinsection IV. Before, we first describe the optical cavity used for the tests and then show indeed what type of dead zone we measure. II. FIBER AND CAVITY DESCRIPTIONS The cavity was realized with 18m of a Kagome Fiber (see Fig.1) designed and fabricated by XLIM and coiled with a 50 cm diameter. The fiber has anexternal diameter of435µmto reduce its sensitivity to environmental perturbationssuchas vibrations, acorediameter of61µmcorrespondingtoamode field diameter of 45µm. The total transmission of this fiber (i.e. taking into account the in/out coupling losses and the propagation losses) is about 83 to 86% and very stable in time (several weeks). This was not Always the case as we could observe reductions of the transmission over time with other fibers mainly with smaller core diameters (from 10 to 20µm). This was reported around to 1.4 µm [8] and due to surface OH–. In our case, at 1.55µm, the origin remains unclear (visual inspection confirmed thatthefiberendswere clean of dust but the nanostructure appeared somehow blurred). Fig.1: Picture of one of the end of the fiber used and schematic of the cavity IJTSRD26390
  • 2. International Journal of Trend in Scientific Research and Development (IJTSRD) @ www.ijtsrd.com eISSN: 2456-6470 @ IJTSRD | Unique Paper ID – IJTSRD26390 | Volume – 3 | Issue – 5 | July - August 2019 Page 581 The cavity coupling is realized in free-space with lenses L1, L2, L3 and M1 mirror. M2 is a HR mirror and is used to monitor the intracavity resonance through its leakage and used to ease the alignment. The cavity is fiber-coupledtothe external probe beams through lenses L1. Its resonance curves, obtained by injecting a clockwise beam in the cavity, are shown in Fig. 2 and give a finesse, defined as the ratio of the resonance peak Full Width Half Max over the Free Spectral range, of 33 and a contrast, defined as the ratio between the difference of the maximum and minimum signals over the maximum one, close of 80%. The values are close to what can be expected when simulating the cavity taking into account the coupler M1 transmission of 6.6%. The Free Spectral Range (FSR) is equal to 16.1 MHz. On the contrary to what we reported in [9] based on [10], λ/2 wave plates are required to control the polarization inside the cavity. This is because the fiber is much more rigid and cannot be twisted without risk of breaking it. Fig.2: Resonance curves. Purple: transmitted beam detected on the photodiode PD4 thru leakage of M2 (transmission < 0.01%). Blue: reflected beam detected by a photodiode connected in place of the fiber injecting the counter-clockwise beam. Yellow: voltage applied to the probe laser III. OBSERVATION OF A LOCK-IN ZONE The complete schematics of the gyroscope is given in Fig. 3 and is similar to has been previously reported. Fig. 3: complete gyroscope schematic with the injection setup including The external laser is split into two beams that are frequency shifted by the acousto-optic modulators (AOM) to resonate with the same mode of the cavity. The AOMs are used to compensate the relative variations between thelaserandthe cavity mode frequencies. The AOM frequencies are driven through a Pound Drever Hall locking scheme [11]. Without rotation, the RF signals applied to the AOM have the same frequency. Under rotation, the frequencies are different because of the Sagnac effect [12]. We plot the gyroscope response curve in Fig. 4, i.e the difference between the two AOM frequencies versus the rotation rate. Above 10°/s, the response is linear. The scale factor is about 5 kHz/(°/s), in agreement with an approximate (because of the real geometry of the cavity and its free-space coupler) value that can be calculated using the usual formula 4Æ n = 2r n =5.8 kHz/(°/s) ßL 180 ß 180 where A = nr2, L = 2nr and 2r the cavity diameter. Below 10°/s, the response tends to shift away from this ideal linear response. Below 5 to 6°/s, the behavior of the gyroscope becomes noisy and chaotic, switching from a state where the AOMs frequencies are identical (locked state) to a transient state where they tend to be different making a more quantitative analysis more difficult. Fig. 4: gyroscope response curve In Fig. 5 below, we show the difference between the frequencies of the RF signals applied to the two AOMs without rotation (except earth). It is in the few Hz range and we believe is a signature of the lock-in phenomenon. Fig. 5: time evolution (in s) of the frequency without applied rotation IV. METHOD TO REDUCE THE DEAD ZONE Several methods havebeen proposedintheliteraturesuchas suppression of the carriers [13]. An illustration of its beneficial effects can be found in [16] for instance. More sophisticated versions with complex modulation schemes werealsodemonstratedin[14],[15].However,aspointedout in [16], the effectiveness of this technique is limited by the carrier suppression level.
  • 3. International Journal of Trend in Scientific Research and Development (IJTSRD) @ www.ijtsrd.com eISSN: 2456-6470 @ IJTSRD | Unique Paper ID – IJTSRD26390 | Volume – 3 | Issue – 5 | July - August 2019 Page 582 We propose to test a different method in which we probe the cavity with counter-propagating beams that resonate with different modes of thecavity. This ensures that,evenwithout rotation, the frequency splitting is not null. We tested this configuration with two AOMs inducing frequency shifts centered around +110MHz and -110MHz so that the counter propagating beams are frequency- separated by 13 FSR. Indeed, we were able to measure rotation rates down to 0.05°/s as can be seen on the improved gyroscope response curve given in Fig. 6. However, at such low rotation rates, the measurements begin to be limited by slow fluctuations of the AOMs frequencies without rotation as can be seen in Fig. 7. This can be easily understood as the frequency splitting between the two counter propagating waves in this configuration depends not only of the Sagnac shift but also on the FSR that is prone to fluctuate. However, when using two AOMs of the same order (+1), so that the two resonating beam frequencies are only separated by one FSR, we did not observe the reduction (by a factor of roughly 20) of these drifts that we expected. Fig.6: improved gyroscope response curve without lock-in Fig.7: Sagnac response of the gyroscope at a rotation rates of ±0.05°/s. In order to retrieve the Sagnac phase shifts, the AOMs frequency must be added explaining the average value of 225 MHz. We thus decided to implement a method to measure the FSR and the rotation rate simultaneously that we describe in the next section. V. METHOD TO MEASURE BOTH THE CAVITY FREE SPECTRAL RANGE AND THE ROTATION RATE We previously reported such an architecture [17] in which the laser beam was separated into three beams, two of them circulating in the same direction in the cavity while thethird one was counter circulating. One of them is used to lock the laser while the two others are, as described in the section III of this paper, frequency shifted by two AOMs. Each beam is lockedonadifferentresonance andtheFSRandrotationrate can be retrieved from the frequencies applied to the AOMs. However webelieve this solution faces some limitationsdue the locking of the laser (butitwould be the same if the cavity length were locked on a stable reference laser). If for some reasons, the laser is not at resonance anymore with the cavity, the control loop will apply a correction signal to the laser so that its frequency converges toward the cavity resonance in a time depending on the control loop bandwidth. However, this transient time during which the laser frequency varies also impacts the AOM control loops and induces some noises in the AOMfrequencies. We thus tested a configuration (see Fig. 8) in which the laser is not locked (frequency or shifts will impact in the same manner the three beams) using three AOMs inducing frequency shifts of 110, -110 and 42MHz. Fig. 8: schematic of the gyroscope configuration with three AOMs. The cavity FSR is now 16.4 MHz Without rotation, combining the three AOM frequencies gives three measurements of 13, 9 and 4 FSRs. The FSR results are given in Fig. 9. As can be seen the FSR are rather stable but there is a bias in the measurements. Fig. 9: FSR measurements (in Hz) deduced from the frequencies of the three AOMs When one looks closer at the evolution of the three signals, further problems appear, as shown in Fig. 10. The scales of the fluctuations are not identical even whenthecurvesseem
  • 4. International Journal of Trend in Scientific Research and Development (IJTSRD) @ www.ijtsrd.com eISSN: 2456-6470 @ IJTSRD | Unique Paper ID – IJTSRD26390 | Volume – 3 | Issue – 5 | July - August 2019 Page 583 to overlap. We are thus investigating the origins of these discrepancies that could be many. Residual Amplitude Modulation (RAM) could be one of the sources but we implemented the scheme described in [18] and we do not see any signature (at least with our level of accuracy) in the electrical spectrums of the intensities after the phase modulators. We are also investigating the symmetry of the resonance peaks that is known to induce a bias if not good enough. Fig. 10: zoom on the FSR variations deduced from the measurements of 4, 9 and 13 FSR. VI. CONCLUSON We report, for what we believe is the first time, observation on the phenomenon of lock-in a passive resonant gyroscope with hollow-core fiber. We demonstrated that this issue can be solved by probing the cavity on two different modes. Indeed, this approach leads to a reduction of the lock-in threshold by several orders of magnitude. However, the sensitivity of the gyroscope is then limited by the FSR fluctuations. We propose and test architecture to measure both the rotation rate and the FSR simultaneously. We also present our ongoing efforts to reduce the discrepancies in the FSR measurements for this architecture to enhance the gyroscope performances. We will report at the conference our latest progress in this direction. REFERENCES [1] G. A. Sanders, L. K. Strandjord, and T. Qiu, “Hollow core fiber optic ring resonator for rotation sensing”, in Optical Fiber Sensors 2006 (OpticalSocietyof America, 2006), paper ME6 [2] K. Iwatsuki, K. Hotate, and M. Higashiguchi,“Kerr effect in an optical passive ring-resonator gyro,”J.Lightwave Technol. 4, 645 (1986) [3] F. Zarinetchi et S. Ezekiel, “Observation of lock-in behavior in a passive resonator gyroscope”, Opt. Lett. 11, 401 (1986). [4] P. Gysel, and R. K. Staubli (1990),“Statisticalproperties of Rayleigh backscattering in single-mode fibers”, Journal of Light wave Technology 8(4), 561-567. [5] S. Lloyd, V. Dangui, M. Digonnet, S. Fan, and G. S. Kino, “Measurement of reduced backscattering noise in laser-driven fiber optic gyroscopes,” Opt. Lett., vol. 25, no. 2, pp. 121–123,2010. [6] A. Ravaille, G. Feugnet, I. Fsaifes, A. Baz, B. Debord, F. Gérôme, G. Humbert, F. Benabid and F. Bretenaker, (2017). In-situ measurement of backscattering in hollow-core fiber based resonant cavities. IEEE Photonics Journal, 9(4), 1-7. [7] A. Ravaille, G. Feugnet, B. Morbieu, I. Fsaifes, A. Baz, B. Debord, G. Humbert, F. Benabid and F. Bretenaker (2017, June). Measurement of backscatteringin hollow core photonic crystal fiber based resonant cavities. In Lasers and Electro-Optics Europe & European Quantum ElectronicsConference(CLEO/Europe-EQEC, 2017 Conference on) (pp. 1-1). IEEE. [8] I. Gris-Sanchez and J.C. Knight(2012).Time-dependent degradation of photonic crystal fiber attenuation around OH absorption wavelengths. Journal of Light wave Technology, 30(23), 3597-3602. [9] I. Fsaifes, G. Feugnet, A. Baz, A. Ravaille, B. Debord, F. Gérôme, G. Humbert, S. Schwartz, F. Benabid and F. Bretenaker (2016, June). Hollow-core photonic- bandgap fiber resonator for rotation sensing. InLasers and Electro-Optics (CLEO), 2016 Conference on (pp.1- 2). IEEE. [10] M. Terrel, M. J.F. Digonnet, and S. Fan, “Polarization controller for hollow-core fiber”, Opt. Lett. 32, 1524 (2007). [11] R. W. P. Drever, J.L. Hall, F.V. Kowalski, J. Hough, G. M. Ford, A.J. Munley, H. Ward, H. (1983). Laser phase and frequency stabilization using an optical resonator. Applied Physics B, 31(2), 97-105. [12] G. Sagnac (1913).L'éther lumineuxdémontrépar l'effet du vent relatif d'éther dans un interféromètre en rotation uniforme. CR Acad. Sci., 157, 708-710. [13] K. Iwatsuki, K. Hotate and M. Higashiguchi (1984). Effect of Rayleigh backscattering in an optical passive ring-resonator gyro. Applied Optics, 23(21), 3916- 3924. [14] K. Hotate, K. Takiguchi, and A.Hirose, ‘‘Adjustment-free method to eliminate the noise induced by the backscattering in an optical passive ring-resonator gyro,’’ IEEE Photon. Technol. Lett., vol. 2, no. 1, pp.75- 77, Jan. 1990.
  • 5. International Journal of Trend in Scientific Research and Development (IJTSRD) @ www.ijtsrd.com eISSN: 2456-6470 @ IJTSRD | Unique Paper ID – IJTSRD26390 | Volume – 3 | Issue – 5 | July - August 2019 Page 584 [15] K. Suzuki, K. Takiguchi, and K. Hotate, “Monolithically integrated resonator micro optic gyro on silica planar lighwave circuit,” J. Lightw. Technol., vol. 18, no. 1, pp. 66–72, Jan. 2000. [16] H. Ma, Z. He and K. Hotate (2011). Reduction of backscattering induced noise by carriersuppression in waveguide-type optical ring resonator gyro. Journal of Lightwave Technology, 29(1), 85-90. [17] S. Schwartz, G. Feugnet, .B. Morbieu, N. El Badaoui, G. Humbert, F. Benabid, I. Fsaifes and F. Bretenaker (2017, November). New approaches in opticalrotation sensing. In International Conference on Space Optics— ICSO 2014 (Vol. 10563, p. 105633Y). International Society for Optics and Photonics. [18] W. Zhang, M. J. Martin, C. Benko, J. L. Hall, J. Ye, C. Hagemann, T. Legero, U. Sterr, F. Riehle, G. D. Cole and M. Aspelmeyer(2014). Reductionofresidual amplitude modulation to 1× 10-6 for frequency modulation and laser stabilization. Optics letters, 39(7), 1980-1983