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Dynamic range beyond 100 dB for polarization mode coupling measurement based on white light interferometer

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Abstract

This paper presents a method to improve the dynamic range of white light interferometer (WLI) based polarization mode coupling (PMC) measurement system beyond 100 dB. The limitation of interference beat noise is overcame by analyzing in detail the inherent noises that have impacts on the detection sensitivity. An improved PMC measurement system and method are proposed for testing ultra-high polarization extinction ratio (PER) of polarization-related devices. The method can improve dynamic range dramatically through eliminating interference beat noise and enhancing the tested interference intensity simultaneously, which are verified theoretically and experimentally. In addition, a Y-junction with ~80 dB PER of LiNbO3 chip corresponding to a weak signal is tested as an application example. The results demonstrate that the high PER interferogram can be identified clearly and steadily with standard deviation 0.9 dB (3σ) @ ~80 dB. This proposed method is highly beneficial in fabrication and evaluation for polarization devices with ultra-high PER.

© 2016 Optical Society of America

1. Introduction

Distributed optical fiber sensing techniques have been investigated for structural imperfection evaluation, temperature detection and strain monitoring. There exist many approaches for different physical quantity detections, such as optical time domain reflectometer (OTDR) [1], optical frequency domain reflectometry (OFDR) [2], and Brillouin optical time domain analysis (B-OTDA) [3]. Different from detecting the optical characteristics of various backscattered light, distributed polarization mode coupling (PMC) measurement system based on white light interferometer (WLI) is developed by monitoring transmission light [4]. In addition to serving as sensors, the PMC system can also be applied to distributed measurement for polarization-related characteristics with high-precision [5,6]. We could obtain the distributed features of devices depending on the locations and amplitudes of interferograms, such as the angular alignment of polarization-maintaining fiber (PMF) [7], the crosstalks along interferometric fiber optic gyro (IFOG) coil [8], the polarization extinction ratio (PER) [9] and distributed birefringence dispersion [10] of integrated-optic devices.

It has been reported that the dynamic range of distributed PMC measurement system based on WLI can achieve ~90 dB [9]. Whereas, this system requires each component and device to be kept in an optimum state. The weak PMC or high PER (>80 dB) measured with PMC measurement system is vulnerable to the environment noises [11], which will be submerged in noise floor, leading to a confusing identification. Therefore, the dynamic range and detection sensitivity of PMC measurement system should be further pronouncedly improved. Several basic studies have been reported to discuss the improvement of signal to noise ratio (SNR) or dynamic range. K. Takada et al. suggested that amplifying the output power of light source [12] and reducing the detectable bandwidth could improve the detection sensitivity of optical low coherence reflectometer (OLCR) [13]. These methods increase requirements for light source and mechanical scanning stage. W. Sorin et al. declared that the effects of intensity noise could be decreased by selectively attenuating the reference power [14], which will reduce the utilization of the light source power. W. Jing et al. described the rotation angle optimization of the polarization eigenmodes in WLI to increase the SNR of the output interferogram [15]. This measurement system however has a compromise between the measurement sensitivity and the measurement error. H. Zhang et al. proposed a signal processing method based on empirical mode decomposition (EMD) to enhance the detection sensitivity by suppressing the noise from −50 dB to −60 dB [16].

This paper analyzes three typical noises—light shot noise, interference beat noise, and circuit thermal noise—of distributed PMC measurement system. We propose a PMC measurement system to improve the system dynamic range by suppressing the interference beat noise. It is verified theoretically and experimentally that the dynamic range utilizing this proposed method can be expanded beyond 100 dB. Besides, a Y-junction with chip PER of ~80 dB is tested and its corresponding interferogram can be identified clearly and steadily. This proposed method is highly beneficial in evaluation of polarization devices with ultra-high PER and improvement of dynamic range for PMC measurement system.

2. Theory analysis

2.1 Traditional PMC measurement

The schematic diagram of traditional PMC measurement based on WLI is shown in Fig. 1 [4]. The white light from a superluminescent light-emitting diode (SLD) is transmitted into a device under test (DUT). Generally, there exist couplings or polarization extinctions at the perturbation points due to the inner structural imperfectness of DUT, external perturbations or discontinuous points (such as spliced points, connections by optical adhesive). In this case, the coupling mode with tiny energy is generated at a perturbation point and the excited mode with most energy will continue to propagate along DUT. It will generate two optical paths (OPs) with orthogonal polarization eigenmodes at the perturbation point due to the birefringence Δn of DUT. The two OPs induce optical path difference (OPD) ΔnL at the output-end of PMF, where L is the PMF length between the perturbation point and the output-end of PMF. Afterwards, utilizing a scanning Mach-Zehnder interferometer (MZI), the main interferogram is detected at OPD of Δl0 and the coupling interferogram is generated by a compensation OPD of Δlc, where Δlc=Δl0+ΔnL. Finally, all the profiles of the interferograms are sampled and extracted by signal processor unit (SPU).

 figure: Fig. 1

Fig. 1 Traditional PMC measurement schematic based on WLI. (SLD: light-emitting diode, MZI: Mach-Zehnder interferometer, DUT: device under test, C: coupler, M: motor, SPU: signal processor unit, PD: photodiode, and DAQ: data acquisition.)

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As the typical noise originating from distributed PMC measurement system, light shot noise σshot2, interference beat noise σbeat2, and circuit thermal noise σcircuit2 can be represented as follows [14]

{σshot2=2eRPdcBσbeat2=2(1+V2)RPscanRPrefB/Δνσcircuit2=4KTB/Reff,
where e is the elementary charge, R is the responsivity of photodiode (PD), Pdc is the DC light intensity, B is the detection bandwidth, V is the polarization degree of light source (here V = 1), Δν is the bandwidth of light source, Pscan and Pref represent the light intensity of scanning arm and reference arm, respectively, K, T and Reff are the Boltzmann parameter, thermodynamic temperature and effective noise resistance, respectively.

Generally, a 50/50 coupler is adopted to divide the light into the two arms of MZI equally. The light intensities of scanning arm and reference arm can be written as

{Pscan=Pt+PcPref=Pt+Pc,
where Pt and Pc are the intensities of excited mode and coupling mode, respectively, in the corresponding arm of MZI. There exists a relationship of Pc=ρPt (ρ1), where ρ is the coupling coefficient introduced by perturbation point which is usually much less than 1. Therefore, Eq. (2) can be expressed as Pscan=PrefPt. Then we can obtain the final signal
{Pdc=Pscan+Pref2PtP02PtPtcos(k0Δl)Psignal=2PtPccos(k0Δl),
where P0 is the main interferogram pattern filtering the DC component, and Psignal is the intensity of coupling interferogram.

For the case of differential detections, the noise variance is given by [17]

σi2=2(σshot2+σbeat2+σcircuit2)=8eRPtB+8R2Pt2B/Δν+8KTB/Reff.
The total signal photocurrent can be written as
I02=(2RP0)28R2Pt2,
Isignal2=(2RPsignal)2=8ρR2Pt2,
where I02 and Isignal2 are the corresponding mean-square signal photocurrents of main interferogram and coupling interferogram, respectively. Therefore, the dynamic range of traditional PMC measurement with differential detections can be expressed as

DR0=I02σi2=1eB/(RPt)+B/Δν+KTB/(ReffR2Pt2).

The denominator in Eq. (6) shows that the dynamic range will be sequentially determined by the third term KTB/(ReffR2Pt2) (σcircuit2-related) and the first term eB/(RPt) (σshot2-related) when the reference powers are less than a few microwatts (~2 μw). Beyond this point, increasing the light power does not improve the dynamic range due to the limitation of interference beat noise (the second term—B/Δν).

2.2 PMC measurement with noise limitation

It has been recognized that polarization beam splitter (PBS) can separate or combine the orthogonal polarizations, which plays an important role in polarization-multiplexed transmissions [18]. Based on schematic shown in Fig. 1, the first coupler denoted by C1 in MZI is replaced by a PBS (see Fig. 2). Here, the two orthogonal polarization eigenmodes —excited mode and coupling mode introduced by DUT—are separated into the scanning arm and reference arm, respectively. Based on Eq. (2), the light intensities of scanning arm and reference arm with PBS are rewritten as

{Pscan2PtPref2Pc.
Here, the PBS with high extinction ratio (ERPBS20dB) could provide an ideal separation for the two orthogonally polarized lights.

 figure: Fig. 2

Fig. 2 PBS-calibrated system used to observe PMC utilizing WLI. (DFB: distributed feedback laser, WDM: wavelength division multiplex, PBS: polarization beam splitter, and other abbreviations are listed in Fig. 1)

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The main interferogram P0_PBS will lose its original meaning due to the PER of PBS. However, the coupling interferogram still exists and can be expressed as Psignal_PBS=22Pt2Pccos(k0Δl).

Therefore, the final photocurrent of AC signal with differential detections can be expressed as

Isignal_PBS2=(2RPsignal_PBS)2=32ρR2Pt2.
Besides, the noise variance can be rewritten as
σi_PBS2=2(σshot2+σbeat2+σcircuit2)=8ePtRB+32ρR2Pt2B/Δν+8KTB/Reff.
The dynamic range DRPBS of PBS-calibrated PMC measurement cannot be directly calculated according to Eq. (6) due to the meaningless main interferogram. In this case, DRPBS should be calibrated by a remarkable interferogram (i.e. Psignal_PBS), which is also measured in traditional PMC measurement. The relative dynamic range of PMC measurement with PBS can be rewritten as

DRPBS=I02σi_PBS2Isignal_PBS2Isignal2=4eB/(RPt)+4ρB/Δν+KTB/(ReffR2Pt2).

In comparison to Eq. (6), Eq. (10) indicates that the signal photocurrent is amplified four times, and the detection sensitivity is enhanced because the term of interference beat noise σbeat2 is ignored due to such a small coupling coefficient ρ. Accordingly, the system dynamic range of PBS-calibrated system will be improved significantly through decreasing detection sensitivity noise and increasing tested interferogram intensity simultaneously.

3. Experiments and results

3.1 PBS-calibrated PMC measurement system and method

In this section, a measurement system for verifying the dynamic range improvement is proposed. As shown in Fig. 2, the white light from a superluminescent light-emitting diode (SLD) at 1550 nm with a short coherence length (~53 μm, corresponding to full width at the half maximum of 45 nm) is divided into two beams through a 98/2 fiber coupler. 2% of the light is for monitoring the output power of light source, and the remaining light is launched into a wavelength division multiplex (WDM). Moreover, a distributed feedback (DFB) laser of 1310 nm is utilized and its light is launched into the same WDM. Then, the light transmitted through an isolator is linearly polarized by a polarizer. For simplify, the DUT is a section of PMF whose output-end is spliced with the pigtail of PBS (with operation wavelength of 1550 ± 40 nm and extinction ratio of ERPBS20dB) utilizing an alignment device—optical fiber fusion splicer (i.e. Fujikura FSM-45PM). The output light from PBS is injected into a MZI that can compensate the OPD. Afterwards, the coupling interferograms are divided by two WDMs (with operation wavelength of 1550 nm/1310 nm, insertion loss of 0.6 dB, and isolation of 50dB) [19] based on the wavelengths and finally detected with differential PDs.

To ensure the measurement accuracy, the system has been improved in many aspects based on our previous works: Firstly, a distributed feedback (DFB) laser of 1310 nm is adopted to eliminate the mechanical vibration influence of scanning motor [10] that is a conventional way for position calibration of mechanical scanning [19]. Secondly, a differential detection is completed by adopting two PDs [9]. Thirdly, a differential scanning MZI with two lenses is employed to suppress the optical power fluctuation [20].

Generally, the alignment device between the pigtail of PBS and DUT should work in 0°–0°, in which the excited mode and coupling mode introduced from DUT can be divided completely by PBS. However, when the alignment device keeps in 0°–45°, the light of excited mode and coupling mode are injected equally into the fast-axis and slow-axis of PBS’s pigtail, respectively. In this case, the PBS is similar to a 50/50 coupler. The calibrating method utilizing this proposed system as shown in Fig. 2 can be described as follows: (1) Varying optical fiber fusion splicer 0°–45° and 0°–0°, and acquiring the two temporal results, respectively. (2) Calibrating a remarkable interferogram in 0°–0° measurement to that in 0°–45°. (3) The relative dynamic range is obtained and the other interferograms corresponding weak-coupling points or ultra-high PER can be identified utilizing the results of 0°–0° measurement.

3.2 Dynamic range improvement results

A PMF with a length of 16 m is tested utilizing the PBS-calibrated PMC measurement system. The envelopes of interferograms versus scanning OPD with PBS angle 0°–45° and 0°–0° are plotted in Fig. 3(a) and 3(b), respectively. Based on scanning OPD relationship of Δl=ΔnL, interferograms P0 and P (or P in Fig. 3(c)) represent the same coupling point—the PER of system polarizer. It is well known that the real coupling intensities and dynamic range can be acquired by normalizing the main interferogram P0 of Fig. 3(a) [9]. Besides, the dynamic range can be calculated by the difference between P0 and the noise floor. In comparison with Fig. 3(a), the main interferogram in Fig. 3(b) will be meaningless due to the function of PBS. However, Fig. 3(b) indicates that the coupling value introduced by system polarizer is amplified from −18.6 dB to −12.0 dB, whereas the noise floor is decreased from −77.0 dB to −84.0 dB. When we calibrate the value of interferogram P by interferogram P, the dynamic range of PMC measurement system can be enhanced to 103.3 dB. An extra measurement with angle combination 0°–90° is shown Fig. 3(c), in which the corresponding interferograms are inverse of Fig. 3(b).

 figure: Fig. 3

Fig. 3 Experiment results of a PMF with angle combination (a) 0°–45°, (b) 0°–0°, and (c) 0°–90°. The main interferogram P0 (12.7 dB) only exists in Fig. (a). Interferograms P (−18.6 dB), P (−12.0 dB) and P (−12.2 dB) marked with red circles—as a remarkable interferogram for calibrating—represent the same coupling point introduced by the same system polarizer. Besides, the noise floors of different angle combinations are labeled by red lines.

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Similar to the above calibrated method, the measured results of dynamic range versus detector light intensity are shown in Fig. 4, where the dynamic range is expressed as DR(dB)=10lg(DR).

 figure: Fig. 4

Fig. 4 The dynamic ranges versus detector light intensity. The theoretical results influenced by different noises are illustrated as follows: (a) blue line—only by σshot2, (b) red line—only by σbeat2, (c) green line—only by σcircuit2, and (d) black line—by the total noise σi2. Some parameters are adopted that Reff=100kΩ, B = 1.2k Hz and R=0.65A/W. The experimental results with angle combination 0°–45° are marked with black points. Moreover, the experimental dynamic range calibrated by angle combinations 0°–0° and 0°–90° are marked with dark blue and light blue points, respectively.

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The theoretical calculations indicate that dominant noise sources depend on the value of the reference arm power. When the reference light power is smaller, the dynamic range is determined by the circuit thermal noise σcircuit2. With the increasing of detector power, the dynamic range cannot overcome the limitation of shot noise σshot2. At last, the dynamic range is limited by the interference beat noise σbeat2 utilizing the traditional method. However, in the smaller segment (0.1 μw– ~2 μw) of light intensity, the dynamic range by PBS-calibrated method is amplified ~6 dB because the amplitude of AC signal is doubled and the detection sensitivity will be same to traditional method due to the limitation of circuit thermal noise σcircuit2. Afterwards, in the segment of ~2 μw–33 μw, the dynamic range will be enhanced dramatically because the detection sensitivity and AC signal will be improved simultaneously. As a result, the proposed method utilizing the proposed PBS-calibrated method can overcome the limitation of interference beat noise. Additionally, it can be estimated that the relative dynamic range will be continually improved with the increasing of detector light intensity.

4. Application

4.1 Evaluating Y-junction with ultra-high chip PER

LiNbO3 integrated Y-junctions are the basic components in IFOG which contains functions of beam splitter, optical polarizer and electro-optical modulator [21]. A packaged Y-junction is usually composed of LiNbO3 chip, electrodes, one input pigtail and two output pigtails. Utilizing the system as shown in Fig. 2, the connection configuration for testing packaged Y-junction in DUT is illustrated in Fig. 5. Different from testing PMF, the linearly polarization light is equally launched into the orthogonal axes of the input pigtail of Y-junction with a 45°-rotated polarizer. The light from the output pigtail of Y-junction is spliced with the PBS’s pigtail utilizing fiber fusion splicer. The methods for full evaluation of polarization characteristics of Y-junction have been reported in Ref [9]. in detail that are beyond this paper.

 figure: Fig. 5

Fig. 5 The connection configuration for testing Y-junction utilizing PBS-calibrated system. The system polarizer (45°-rotated) is spliced to the input pigtail of Y-junction with 0° (at point A). The output pigtail of Y-junction is aligned to the input pigtail of PBS by a fiber fusion splicer (at point O).

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The results for testing Y-junction with different angle combinations are illustrated in Fig. 6(a) and 6(b), respectively. The PER of LiNbO3 chip can be distinguished by the scanning OPD

Δlε=ΔnPMF(LIA+LAB+LBC)+ΔnchipLchip,
where Lsection (section = IA, AB, BC and chip) represents the length of corresponding PMF and LiNbO3 chip, ΔnPMF and Δnchip represent the birefringences of PMF and LiNbO3 chip, respectively. Based on the relationship of scanning OPD Δl=ΔnL, interferograms A, B, C (or C) and O (or O) are induced by the coupling points A, B, C and O as shown in Fig. 5, respectively. Besides, the other interferograms B1, B2 and A2 in the inset of Fig. 5(a) are the 2nd-order couplings without the realistic perturbation points of the Y-junction [22]. Here, the analysis in detail of coupling points of Y-junction are beyond this paper and thus we only focus on the chip PER of Y-junction.

 figure: Fig. 6

Fig. 6 Intensity distribution yielded by interferograms for evaluating a Y-junction with the detection light power of 35 μw. In comparison to the traditional method with angle combination 0°–45° (blue line), two results utilizing PBS-calibrated method with angle combinations (a) 0°–0° and (b) 0°–90° are illustrated denoted by red lines, respectively. The interferograms A, B, C (or C), and O (or O) are induced by the coupling points A, B, C and O shown in Fig. 5, respectively. The chip PER of Y-junction leads to the interferograms ε and ε. Other interferograms B1, B2 and A2 are the 2nd-order coupling. Here, interferogram introduced by coupling point C could be set as the remarkable interferogram for calibrating and interferogram represented the chip PER of Y-junction are to evaluate.

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The characteristics of input pigtail of Y-junction will be suppressed due to the PER of PBS. Similar to the calibration method of PMF measurement in Section 3, the results of PBS-calibrated method is corrected by the interferograms C (and C) as a remarkable interferogram, which represents the coupling point C between the output-pigtail and LiNbO3 chip of Y-junction. As shown in Fig. 6, the traditional method with a PBS spliced at 45° can achieve a similar effect with Ref [9], in which the noise floor utilizing traditional method is ~90 dB (blue line). However, the noise floor by PBS-calibrated method can be improved to ~105 dB (red line). The results demonstrate that the values of PER with PBS-calibrated method can be distinguished clearly from the lower noise floor and higher SNR.

4.2 Evaluating Y-junction with ultra-high chip PER

To verify the repeatability of two measurement methods, the Y-junction is repeatedly measured 20 times by realigning the axes of PBS and the output pigtails PM fiber at 0°–45°, 0°–0° and 0°–90°, respectively. According to the relationship between PER and PMC of PER(dB)10lg(ε/P0)=PMC(dB), the results utilizing different angle combinations are shown in Fig. 7—the black line represents the PERs of Y-junction’s chip tested with angle 0°–45° of PBS, and the blue and red lines give the PER distributions by PBS-calibrated method. It shows that the test fluctuation of high PER utilizing the traditional method will be affected more easily.

 figure: Fig. 7

Fig. 7 Results of 20-times repeated measurement of Y-junction with different angle combinations are marked by (a) black line 0°–45°,(b) blue line 0°–0°, and (c) red line 0°–90°, respectively.

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The standard deviation of PERs utilizing traditional method (0°–45°) and PBS-calibrated method (0°–0°) are 6.5 dB (3σ) and 0.8 dB (3σ), respectively. Therefore, the average chip PER of Y-junction with 0°–0° and 0°–90° PBS-calibrated methods are calculated as follows

{PER(ε)=PER(ε¯)±Δε=80.0±0.8dBPER(ε)=PER(ε¯)±Δε=79.5±0.9dB.

As a result, the PBS-calibrated method can also obtain more stable interferograms. Additionally, the imperfect optical devices could introduce some slight extra errors. When we employ PBS with high extinction ratio and WDMs with high isolation, the dynamic range of PMC measurement system will be extended further. However, the high dynamic range is at the expense of losing the characteristics of input pigtail of Y-junction. In spite of missing some information of Y-junction’s pigtail, pursuing the ultra-high PER measurement is more significant.

5. Conclusions

We describe the noise originating from PMC measurement system and prove that the system dynamic range can be improved by suppressing the interference beat noise. The experimental results obtained from this proposed PBS-calibrated method indicate that the dynamic range can break through 100 dB. Additionally, a Y-junction with ~80 dB PER is tested as an application example and the interferogram representing the chip PER can be identified clearly. Measurement repeatability of PER is limited to 0.9 dB (3σ) @ ~80 dB. This proposed PMC measurement method is highly beneficial in evaluation of polarization devices with ultra-high PER or ultra-weak PMC.

Funding

National Natural Science Foundation of China (61422505, 61227013, 61307104); Program for New Century Excellent Talents in University (NCET-12-0623); National Key Scientific Instrument and Equipment Development Project (2013YQ040815); Specialized Research Fund for the Doctoral Program of Higher Education (20122304110022); Heilongjiang Provincial Natural Science Foundation (ZD201205); International Science & Technology Cooperation Program of China (2013DFR10340).

Acknowledgments

The Y-junction used in this work was supplied by Yong Hua and Ping Shu of Chongqing Optoelectronics Research Institute (Chongqing 400060, China). We would like to acknowledge them for the support.

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Figures (7)

Fig. 1
Fig. 1 Traditional PMC measurement schematic based on WLI. (SLD: light-emitting diode, MZI: Mach-Zehnder interferometer, DUT: device under test, C: coupler, M: motor, SPU: signal processor unit, PD: photodiode, and DAQ: data acquisition.)
Fig. 2
Fig. 2 PBS-calibrated system used to observe PMC utilizing WLI. (DFB: distributed feedback laser, WDM: wavelength division multiplex, PBS: polarization beam splitter, and other abbreviations are listed in Fig. 1)
Fig. 3
Fig. 3 Experiment results of a PMF with angle combination (a) 0°–45°, (b) 0°–0°, and (c) 0°–90°. The main interferogram P 0 (12.7 dB) only exists in Fig. (a). Interferograms P (−18.6 dB), P (−12.0 dB) and P (−12.2 dB) marked with red circles—as a remarkable interferogram for calibrating—represent the same coupling point introduced by the same system polarizer. Besides, the noise floors of different angle combinations are labeled by red lines.
Fig. 4
Fig. 4 The dynamic ranges versus detector light intensity. The theoretical results influenced by different noises are illustrated as follows: (a) blue line—only by σ shot 2 , (b) red line—only by σ beat 2 , (c) green line—only by σ circuit 2 , and (d) black line—by the total noise σ i 2 . Some parameters are adopted that R e f f = 100 k Ω , B = 1.2k Hz and R = 0.65 A / W . The experimental results with angle combination 0°–45° are marked with black points. Moreover, the experimental dynamic range calibrated by angle combinations 0°–0° and 0°–90° are marked with dark blue and light blue points, respectively.
Fig. 5
Fig. 5 The connection configuration for testing Y-junction utilizing PBS-calibrated system. The system polarizer (45°-rotated) is spliced to the input pigtail of Y-junction with 0° (at point A). The output pigtail of Y-junction is aligned to the input pigtail of PBS by a fiber fusion splicer (at point O).
Fig. 6
Fig. 6 Intensity distribution yielded by interferograms for evaluating a Y-junction with the detection light power of 35 μw. In comparison to the traditional method with angle combination 0°–45° (blue line), two results utilizing PBS-calibrated method with angle combinations (a) 0°–0° and (b) 0°–90° are illustrated denoted by red lines, respectively. The interferograms A, B, C (or C ), and O (or O ) are induced by the coupling points A, B, C and O shown in Fig. 5, respectively. The chip PER of Y-junction leads to the interferograms ε and ε . Other interferograms B 1 , B 2 and A 2 are the 2nd-order coupling. Here, interferogram introduced by coupling point C could be set as the remarkable interferogram for calibrating and interferogram represented the chip PER of Y-junction are to evaluate.
Fig. 7
Fig. 7 Results of 20-times repeated measurement of Y-junction with different angle combinations are marked by (a) black line 0°–45°,(b) blue line 0°–0°, and (c) red line 0°–90°, respectively.

Equations (13)

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{ σ s h o t 2 = 2 e R P d c B σ b e a t 2 = 2 ( 1 + V 2 ) R P s c a n R P r e f B / Δ ν σ c i r c u i t 2 = 4 K T B / R e f f ,
{ P s c a n = P t + P c P r e f = P t + P c ,
{ P d c = P s c a n + P r e f 2 P t P 0 2 P t P t cos ( k 0 Δ l ) P s i g n a l = 2 P t P c cos ( k 0 Δ l ) ,
σ i 2 = 2 ( σ s h o t 2 + σ b e a t 2 + σ c i r c u i t 2 ) = 8 e R P t B + 8 R 2 P t 2 B / Δ ν + 8 K T B / R e f f .
I 0 2 = ( 2 R P 0 ) 2 8 R 2 P t 2 ,
I s i g n a l 2 = ( 2 R P s i g n a l ) 2 = 8 ρ R 2 P t 2 ,
D R 0 = I 0 2 σ i 2 = 1 e B / ( R P t ) + B / Δ ν + K T B / ( R e f f R 2 P t 2 ) .
{ P s c a n 2 P t P r e f 2 P c .
I s i g n a l _ P B S 2 = ( 2 R P s i g n a l _ P B S ) 2 = 32 ρ R 2 P t 2 .
σ i _ P B S 2 = 2 ( σ s h o t 2 + σ b e a t 2 + σ c i r c u i t 2 ) = 8 e P t R B + 32 ρ R 2 P t 2 B / Δ ν + 8 K T B / R e f f .
D R P B S = I 0 2 σ i _ P B S 2 I s i g n a l _ P B S 2 I s i g n a l 2 = 4 e B / ( R P t ) + 4 ρ B / Δ ν + K T B / ( R e f f R 2 P t 2 ) .
Δ l ε = Δ n PMF ( L I A + L A B + L B C ) + Δ n chip L chip ,
{ P E R ( ε ) = P E R ( ε ¯ ) ± Δ ε = 80.0 ± 0.8 dB P E R ( ε ) = P E R ( ε ¯ ) ± Δ ε = 79.5 ± 0.9 dB .
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