Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

In-situ adjustable fiber-optic piezometer based on parallelly structured external Fabry-Perot interferometers with Vernier effect and its harmonics

Open Access Open Access

Abstract

Translating interferometric applications into practical field use with the required flexible precision and measurement range, is a recognized challenge. We report an in-situ adjustable fiber-optic piezometer based on parallelly structured external Fabry-Perot interferometers (EFPIs) with the Vernier effect and its harmonics. By accommodating the EFPI structure with an adjustable and a fixed cavity length, the EFPIs are utilized as a referencing fiber piezometer (RFP), and a sensing fiber piezometer (SFP), respectively. The Vernier effect with amplified sensitivity is formed by connecting the RFP and SFP in parallel via a 3 dB optical coupler. By simply tuning the cavity length of the RFP, the magnification factor M of the Vernier effect is in-situ continuously adjustable. Using the two prototypes SFP1 and SFP2, water level measurement is performed in the fundamental Vernier effect (FVE) mode and the harmonic Vernier effect (HVE) mode. Experimental results demonstrate that in the FVE mode, the sensitivity can be predictably tuned from −0.15 nm/cm to −7.02 nm/cm with M=1∼48 for SFP1, and −0.31 nm/cm to −7.22 nm/cm with M=1∼23 for SFP2. In the HVE mode, the sensitivity can be further enhanced as high as −9.08 nm/cm, while the sensing performance fluctuates during the adjusting process. Benefiting from the merits of in-situ adjustable sensitivity and measurement range, simplicity of composition, robustness, and remote sensing capability, the proposed scheme can be applied to various practical applications.

© 2021 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement

1. Introduction

Piezometers are geotechnical sensors that are used to measure pore water pressure (PWP) in the soil, earth/rock fills, foundations, and concrete structures [1]. In the last decades, piezometers have been widely used in construction control, stability investigation, shallow underground works [2], groundwater pressure study [3] and monitoring of slope failure [4], landslides [5], earth dams [6], embankments [7], etc. As compared with traditional electrical piezometers [8,9], the unique advantages of optical fiber-based piezometers such as immune to electromagnetic interference (EMI) and their multiplexing potential bring them widespread attention [10,11]. Among them, the FBG and interference-based piezometers [12,13] are two typical representatives, showing stable and reliable characteristics. However, their performance in terms of sensitivity or resolution can be further improved.

The Vernier effect, firstly used in a Vernier caliper, can significantly enhance detection accuracy and is widely used in many measurement fields by utilizing the overlapping effect of two scales [14]. In recent years, the Vernier effect has been employed in optical fiber sensing technology, in which two interferometers are connected in cascade or parallel structures [15]. These two interferometers can be the same such as the Mach-Zehnder interferometers (MZIs) [16], Michelson interferometers (MIs) [17], Sagnac interferometer (SIs) [18], Fabry-Perot interferometers (FPIs) [19], microfiber knot resonators (MKRs) [20], fiber couplers [21], or combinations of any two of them [2225]. Due to its magnification mechanism, the Vernier effect appears to be a promising solution for sensing applications with real-time controllable performance. Xu et al. [26] proposed a sensitivity-controllable refractive index sensor based on a reflective θ-shaped microfiber resonator that cooperated with the Vernier effect. However, the sensing structure is difficult to manufacture, and its adjustment is not conducive to practical applications. Wang et al. [27] proposed an ultra-sensitive gas pressure sensor based on the Vernier effect with a controllable amplification factor, but it is difficult to achieve continuous adjustment on-site based on their femtosecond processing and splicing manufacturing process. For practical applications, an in-situ continuously adjustable fiber-optic sensor based on the Vernier effect is desired, which has yet been reported in literature.

The harmonic Vernier effect (HVE) [2830], different from the slight optical path difference between two interferometers in the fundamental Vernier effect (FVE), has multiple relationships between the optical path differences of interferometers. Based on the HVE method, Gomes et al. [31] achieved a giant refractometric sensitivity (a magnification factor over 850) by combining the extreme optical Vernier effect and modal interference, further amplifying the detectable range compared with the FVE method.

In this article, an in-situ adjustable fiber-optic piezometer based on a parallelly structured EFPI with both the FVE and HVE is theoretically and experimentally demonstrated. The EFPI is simply formed by a fiber ferrule connector/flat contact (FC/FC) connector and an aluminum foil pasted on a thin metal plate. When accommodating the EFPI structure, a referencing fiber piezometer (RFP) and a sensing fiber piezometer (SFP) are formed by using an adjustable and a fixed cavity length, respectively. By connecting the RFP and SFP in parallel, the Vernier effect with amplified sensitivity is formed. By simply tuning the cavity length of the RFP, the magnification factor M of the Vernier effect is in-situ continuously adjustable. Since the RFP is not used for measurement (e.g. installed in a borehole or pressure chamber), tuning of its cavity length can be done on spot thus achieving an in-situ adjustment of sensor sensitivity. A water level measurement is carried out in both the FVE and HVE modes on two prototypes SFP1 and SFP2. In the FVE mode, the sensitivity can be predictably tuned from −0.15 nm/cm to −7.02 nm/cm with M=1∼48 for SFP1, and −0.31 nm/cm to −7.22 nm/cm with M=1∼23 for SFP2. In the HVE mode, the sensitivity can be further enhanced up to −9.08 nm/cm but with a fluctuated performance during the adjusting process. In addition, the advantages of the proposed scheme such as in-situ adjustable sensitivity, tunable working range, simplicity of composition, robustness, and remote sensing capability, further facilitate its potential for practical applications.

2. Experimental setup and principle

2.1 Single EFPI

The schematic of the EFPI structure with air cavity is shown in Fig. 1, which is simply formed by an FC/FC connector and a piece of aluminum foil (99.99% purity, 20 µm thickness, 3 mm diameter) pasted on a circular metal plate (0.75 mm thickness, 15 mm radius). The entire optical structure is well protected and accommodated by a cylindrical component made of aluminum alloy. One physical piezometer prototype as a reference interferometer is also shown in Fig. 1, indicating its compact and robust characteristics. It is worth noting that the components of the air cavity are connected by fine threads, enabling its adjustment function of the RFP. In other words, the cavity length and the free spectrum range (FSR) of the RFP can be adjusted in real-time by rotating the threaded part as needed. In addition, it would be good for miniaturization and adaptation of fiber piezometer by integrating the sensing head into a single fiber structure, the easily available components in our case make the sensing structure simple, low-cost, robust, durable and benefit its practical applications.

 figure: Fig. 1.

Fig. 1. Schematic diagram of EFPI structure and one prototype of the EFPI piezometer as reference interferometer.

Download Full Size | PDF

In Fig. 1, the incident beam and the reflected beams are represented by a black arrow and red arrows, respectively. The reflected beams will recombine in the fiber, resulting in a typical interference fringe pattern as output. For a typical EFPI of either the RFP or the SFP, the output intensity can be expressed as [32]:

$$I = {I_1} + {I_2} + 2\sqrt {{I_1}{I_2}} \cos ({\phi _{FP}} + {\phi _0}), $$
where I1 and I2 are the light intensities of the reflected beams by the interfaces of the FC/FC connector and the aluminum foil, respectively, ϕ0 is the initial phase of the EFPI; and ϕFP is the phase difference of the two reflected light beams. Assuming ϕ0=0, the resonant wavelength would satisfy the phase condition as [22]:
$${\phi _{FP}} = \frac{{2\pi \ast 2L}}{{{\lambda _m}}} = 2m\pi, $$
$${\lambda _m} = \frac{{\textrm{2}L}}{m}, $$
where for a peak wavelength, the interference order $m = k$; for a dip wavelength, $m = ({\textrm{2}k\textrm{ + 1}} )\textrm{/2}$; and k is a positive integer. L is the cavity length of the EFPI. The FSR of the interference fringe of the EFPI can be given by [33,34]
$$FS{R_{FP}} = {\lambda _m} - {\lambda _{m + 1}} = \frac{{{\lambda _m} \cdot {\lambda _{m + 1}}}}{{\textrm{2}L}} \approx \frac{{{\lambda ^\textrm{2}}}}{{\textrm{2}L}}. $$

The observed wavelength variation relative to the cavity length variation induced by external pressure can be expressed as

$$\Delta {\lambda _\textrm{m}} = \frac{{{\lambda _\textrm{m}}}}{{{L_\textrm{0}}}}\frac{{dL}}{{dP}}\Delta P, $$
where L0 is the initial cavity length of the EFPI.

2.2 Parallel structured EFPI

Based on the principle and physical prototypes of the single EFPI, the parallel structured EFPI is constructed as shown in Fig. 2, in which the RFP prototype and the SFP prototype are connected in parallel through a 3 dB optical coupler. An interrogator (Miron Optics Si255 1460∼1620 nm, 1 pm resolution) is used to illuminate the optical path and collect spectral data. The collected data are processed and displayed on a computer.

 figure: Fig. 2.

Fig. 2. Schematic diagram of parallel structured EFPI.

Download Full Size | PDF

As described above, the RFP has an adjustment function on the cavity length, i.e., the FSR of the interference fringe of the RFP is adjustable by tuning the fine threads. Thus, the spectra of the RFP and the SFP with similar but slightly different FSRs can be easily acquired as shown in the dashed red box in Fig. 2. The total transmission spectrum from the superimposition of the two individual fiber piezometers is displayed on the computer. The light intensity of the total transmission can be expressed as [35]

$$I\textrm{ = }{I_R}\textrm{ + }{I_S} \approx A + B\cos \frac{{{\phi _{RFP}} + {\phi _{SFP}}}}{2}\cos \frac{{{\phi _{RFP}} - {\phi _{SFP}}}}{2}, $$
where ${I_R}$ and ${I_S}$ are the reflected light intensities of the RFP and SFP, respectively, ${\phi _{RFP}} = {{4\pi {L_R}} / \lambda }$ and ${\phi _{SFP}} = {{4\pi {L_S}} / \lambda }$ represent the phase difference of the RFP and the SFP, respectively; ${L_R}$ and ${L_S}$ are the cavity lengths of the RFP and the SFP; and A and B are the constants determined by the reflectivity of multiple reflective interfaces of the two EFPIs.

2.3 Fundamental Vernier effect

The concept of the Vernier effect comes from the caliper which has two rulers with a slight scale difference. Similarly, by adjusting the cavity length of the RFP to be slightly different from that of the SFP, the optical Vernier effect can be readily achieved. The transmission dips will overlap again after several orders, which leads to a periodic envelope in the Vernier-effect spectrum. As observed in Fig. 2, the Vernier-effect spectrum consists of a series of fringes with different amplitudes in a periodic envelope trend. The FSR of the Vernier-effect envelope can be described as [36,37]:

$$FS{R_e} = \frac{{FS{R_S}FS{R_R}}}{{|{FS{R_S} - FS{R_R}} |}}\textrm{ = }\left|{\frac{{{\lambda_m}{\lambda_{m + 1}}}}{{2({L_S} - {L_R})}}} \right|. $$

As compared to the single SFP, the envelope of the Vernier effect shows sensitivity magnification. The magnification factor M is an important indicator of the Vernier effect, which can be given by two definitions [28,29]. The first one is defined as the magnification ratio from the FSR of the single sensing interferometer to that of the Vernier envelope, expressed as

$$M = \frac{{FS{R_e}}}{{FS{R_S}}}\textrm{ = }\frac{{FS{R_R}}}{{|{FS{R_S} - FS{R_R}} |}}\textrm{ = }\left|{\frac{{{L_S}}}{{{L_S} - {L_R}}}} \right|. $$

As shown in Eq. (7) and (8), both the FSRs and the M-factor of the envelope are determined by the cavity lengths of the EFPIs that form the Vernier effect. The other definition of M is related to the sensing performance, which is the magnification ratio from the wavelength shift of the single sensing interferometer to that of the Vernier envelope, expressed as

$$M = \frac{{{S_{envelope}}}}{{{S_{SFP}}}}\textrm{ = }\frac{{\Delta {\lambda _e}}}{{\Delta {\lambda _m}}}. $$

It is worth noting that, by adjusting the cavity length of the RFP LR, the FSR of the Vernier envelope and the M-factor can be well controlled and tuned, enabling its adjustable features in-situ. This will be further verified in the experimental part.

2.4 Harmonic Vernier effect

In the above section of the fundamental Vernier effect (FVE), the two interferometers have a slight difference in the optical path, i.e., cavity lengths. However, in the harmonic Vernier effect (HVE), the cavity length of one EFPI is multiples of the other. Based on the HVE, the sensitivity can be further amplified to a significant level as compared to the FVE [28].

Due to the in-situ adjustable function of our proposed RFP and SFP scheme, the HVE structure can be easily obtained. Compared with increasing the cavity length of RFP, reducing the cavity length of RFP is more conducive, as it renders greater spectral contrast and smaller optical loss. Here in the case of spectral output, reducing the cavity length of RFP is equivalent to increasing the cavity length of the SFP. Thus, the optical path length of the SFP is considered to be increased by i-times the cavity length of the RFP (LS = LS + iLR). i is a positive integer defined as the order of the HVE; the HVE degrades to the FVE when i = 0. Then the FSR of the SFP can be given follow:

$$FSR_S^i = \left|{\frac{{{\lambda_m}{\lambda_{m + 1}}}}{{2({L_S} + i{L_R})}}} \right|. $$

To form a typical Vernier effect spectrum, the FSRs of the two interferometers will overlap at resonant dips when this match condition is satisfied: $FSR_e^i = kFS{R_R} = [{(i + 1)k + 1} ]FSR_S^i$, with $k = {{FSR_S^i} / {[{FS{R_R} - (i + 1)FSR_S^i} ]}}$. Therefore, the FSR of the lower envelope can be written in the form of

$$FSR_e^i = \left|{\frac{{FS{R_R}FSR_S^i}}{{FS{R_R} - (i + 1)FSR_S^i}}} \right|. $$

The FSR of the HVE internal envelope and the corresponding M-factor can be given by [28]

$$FSR_{ie}^i = \left|{\frac{{(i + 1)FS{R_R}FSR_S^i}}{{FS{R_R} - (i + 1)FSR_S^i}}} \right|= (i + 1)FSR_e^i, $$
$${M^i} = \frac{{FSR_{ie}^i}}{{FSR_S^i}} = \left|{\frac{{(i + 1)FS{R_R}}}{{FS{R_R} - (i + 1)FSR_S^i}}} \right|= (i + 1)M. $$

It is clear that compared to the FVE, the FSR and sensitivity of the HVE are both increased by a factor of i+1. Thus, the HVE appears to be a promising way to further improve the performance of the sensor. However, when i is increased, the slight cavity length difference i.e. ${L_S} - (i + 1){L_R}$ between the two EFPIs becomes harder to maintain as compared to the FVE. This will complicate the adjustment process of the magnification factor, which will be demonstrated in the following experimental part.

3. Results and discussion

3.1 Single EFPI

To verify the above theory, two prototypes of the EFPI piezometer, SFP1 and SFP2 are manufactured. Their corresponding output spectra are shown in Fig. 3(a), where the black and red curves represent the spectra of SFP1 and SFP2 with fringe contrasts of 7.5 dB and 25 dB, respectively. It is noted that their FSRs are 3.04 nm and 6.76 nm, which means that according to Eq. (4), the initial cavity lengths are approximately 398 µm and 178 µm, respectively.

 figure: Fig. 3.

Fig. 3. (a) Initial spectra of sensing fiber piezometers SFP1 and SFP2, (b) Wavelength variation of SFP1 and SFP2 along with water level.

Download Full Size | PDF

The performance of SFP1 and SFP2 is tested by performing a water level measurement. Their spectrum variations under distinct water levels are shown in Fig. 3(b), in which the spectra are recorded and displayed in vertical offset. As the water level increases from 0 cm to 20 cm in steps of 5 cm, the blue shift process shown by the blue dashed arrows can be observed clearly. The blue shift phenomenon can be explained by Eq. (3) that increasing water pressure reduces the resonant wavelength. The relationships between the wavelength and the water level of SFP1 and SFP2 are also depicted in Fig. 3(b), where the linear fittings reveal their sensitivities of −0.15 nm/cm, and −0.31 nm/cm, respectively.

3.2 Fundamental Vernier effect

The Vernier effect based on two piezometer prototypes SFP1 and SFP2 is demonstrated in a water level measurement with an experimental setup illustrated in Fig. 4. The SFP with fixed cavity length and The RFP with adjustable cavity length as indicated by the blue arrows are connected in parallel configuration through a 3 dB optical coupler. The SFP is immersed in water, and the water level varies from 0 to 20 cm at a step of 5 cm. The corresponding spectra data are collected and recorded by the interrogator. By tuning the cavity length of the RFP, both SFP1 and SFP2 in the FVE and HVE modes are tested in this water level measurement for comparison.

 figure: Fig. 4.

Fig. 4. Experimental setup for water level test.

Download Full Size | PDF

In the FVE mode, a slight cavity length difference between the RFP and the SFP will cause a periodical envelope in the Vernier fringes as shown on the computer screen in Fig. 4. The envelope shifts along with the water level are recorded as shown in Fig. 5(a). The dip of the lower envelope for observation experiences an obvious blue shift as indicated by the dashed blue arrow. The M-factor from FSR can be roughly counted from the envelope fringes, that is, the number of FSR fringes of a single sensing SFP contained in one period of the envelope. Here about 10 fringes are contained as shown by the red lines, implying an M-factor of about 10. The corresponding relationship between the wavelength and the water level is depicted in Fig. 5(b), where the sensing curve of the single SFP1 is also depicted as a comparison. An actual M-factor of 9.56 from measurement sensitivity is acquired, amplifying a sensitivity of −0.15 nm/cm of the single SFP1 to a sensitivity of −1.41 nm/cm of SFP1 in an FVE mode.

 figure: Fig. 5.

Fig. 5. (a) Spectra under water level test with one vernier structure M=10; (b) Relationship between wavelength and water level compared with that of single SFP1.

Download Full Size | PDF

By continuously tuning the cavity length of the RFP and counting the FSR fringes in one period of the envelope, the M-factor or measurement sensitivity of the SFP1 in the FVE mode can be well controlled and adjusted. The output spectra are shown in Fig. 6(a), in which the number of the fringe in one period of the envelope or the M-factor is adjusted to be 6, 10, 14, and 48. The corresponding wavelength shifts under these tuned states as a function of the water level are recorded and depicted in Fig. 6(b), where the sensing curve of the single SFP1 is also included for comparison. It reveals that the sensitivity of the single SFP1 (−0.15 nm/cm) is continuously magnified to be −0.82 nm/cm, −1.41 nm/cm, −2.08 nm/cm, and −7.02 nm/cm with corresponding sensing M-factors of 5.59, 9.56, 14.09, and 47.57, respectively. These results indicate that the function of in-situ adjustable sensitivity is realized based on the SFP1 in the FVE mode. However, when the sensitivity is amplified to a large multiple (the green line), the measurement range is narrowed, which is limited by the 160 nm wavelength range of the interrogator.

 figure: Fig. 6.

Fig. 6. (a) Vernier spectra of SFP1 with a magnification factor of 6, 10, 14, and 48; (b) Corresponded relationships between the wavelength shifts and the water level.

Download Full Size | PDF

To further verify the in-situ adjustable function, effectiveness, and repeatability of the proposed scheme in the FVE mode, the same measurement process is repeated on the piezometer prototype SFP2 which has a shorter cavity length. The Vernier spectra with M-factors from FSR continuously adjusted from 4, 9, 13, to 23, are shown in Fig. 7(a). The corresponding sensing curves under these tuning states are depicted in Fig. 7(b), showing the actual sensing M-factors from 3.81, 9.17, 13.07, to 23.48. Similar to the SFP1 in FVE mode, when the sensitivity is amplified to a large multiple, the measurement range becomes narrower as shown by the green line. It should be noted that the sign of sensitivity changes, that is, the negative sensitivity of the single SFP2 becomes positive in the FVE mode. This can be explained by the relationship ${L_{SFP\textrm{2}}} < {L_{RFP}} < {L_{SFP\textrm{1}}}$, so the wavelength shift will undergo a sign change as compared with the SFP1 in the FVE mode.

 figure: Fig. 7.

Fig. 7. (a) Vernier spectra of SFP2 with magnification factors of 4, 9, 13, and 23; (b) Corresponding relationships between the wavelength shifts and the water level.

Download Full Size | PDF

3.3 Harmonic Vernier effect

Based on the HVE, as mentioned before, the sensitivity can be further amplified to a significantly higher level. To verify it, the prototypes SFP1 and SFP2 are also tested in the HVE mode. As shown in Fig. 8(a), the harmonic Vernier spectrum of SFP1 with harmonic order i=1 shows two internal envelopes in red and pink. And the cross point of the two internal envelopes can be the observation point during the measurement as shown in Fig. 8(b), which indicates an obvious blue shift.

 figure: Fig. 8.

Fig. 8. (a) Harmonic Vernier spectrum of SFP1 with i=1 and (b) corresponding spectra shifts with the water level.

Download Full Size | PDF

By tuning the cavity length of the RFP, the spectra under different harmonic orders i=1, 2, 3 are obtained as shown in Fig. 9(a), including the spectrum in FVE mode (i=0, M=6) for comparison. The number of the internal envelopes is equal to i+1. By observing the shift of the cross point, the corresponding sensing curves under i=1, 2, 3 are shown in Fig. 9(b), where the sensitivity is magnified to be −4.38 nm/cm, −9.08 nm/cm, and −2.52 nm/cm. The corresponding M-factors are 29.70, 61.57 and 17.07 as compared to the single SFP1.

 figure: Fig. 9.

Fig. 9. (a) Harmonic Vernier spectra of SFP1 with i=1, 2, 3, and (b) corresponding sensing curves.

Download Full Size | PDF

Similarly, SFP2 in the HVE mode is also tested. The spectra under different harmonic orders i=1, 2, 3 are shown in Fig. 10(a), including the spectrum in FVE mode (i=0, M=4) as a comparison. By observing the shift of the cross point, the corresponding sensing curves under i=1, 2, 3 are shown in Fig. 10(b). The sensitivity is magnified to be −7.45 nm/cm, −4.20 nm/cm, and −1.38 nm/cm, with corresponding M-factors of 24.22, 13.65 and 4.48 as compared to the single SFP2, respectively.

 figure: Fig. 10.

Fig. 10. (a) Harmonic Vernier spectra of SFP2 with i=1, 2, 3, and (b) corresponding sensing curves.

Download Full Size | PDF

Both SFP1 and SFP2 in the HVE mode do not show a continuous increase in sensitivity as expected when the harmonic order changes in integers. This may be attributed to the manual adjustment of the reference states (tuning the fine threads) in the FVE mode. It can be improved by using a more sophisticated adjustment apparatus but sacrificing the cost-effectiveness and simplicity of the system at the same time. Nevertheless, SFP1 and SFP2 in the HVE modes still show further magnified sensitivities up to −9.08 nm/cm and −7.45 nm/cm, respectively, as compared to the FVE mode.

3.4 Performance comparison

The performance comparison of the above-mentioned demodulation schemes (single SFP, SFP in FVE mode, SFP in HVE mode) is listed in Table 1, in terms of the sensitivity, resolution, M-factor by FSR, M-factor by sensitivities and measurement range. Compared with the single SFP with fixed sensitivity, both the FVE mode and HVE mode show obvious magnification on sensitivity, showing ∼µm level water level sensing resolution. Sensing structure in the HVE mode further enhances the performance as compared to the FVE mode. For in-situ continuous adjustment, the FVE mode shows better controllability on the sensing M-factor, and the HVE mode does not show a consistent increase on the sensing M-factor. It is worth noting that the sensor resolution values listed in the table are derived from the ratio of instrument’s demodulation resolution to sensor sensitivity, which is only used as an index for comparison. In practical applications, the sensing error would increase along with the enhancement of sensitivity. The actual measurement resolution would be affected by the noise floor induced by the external environment and reading error from data processing.

Tables Icon

Table 1. Performance Comparison of Demodulation Schemes

Besides, limited by the wavelength range of the interrogator, the measurement range of the proposed schemes is inversely proportional to measurement sensitivity. In fact, the measurement range can be expanded by adopting a widened wavelength range of the interrogator or OSA, but this will also increase the system cost. To clarify the variation trends of these two important performance indicators, their numerical changes are represented by the histogram shown in Fig. 11. The results of SFP1 in the single sensing mode, FVE mode and HVE mode are shown in Fig. 11(a), and those of SFP2 are shown in Fig. 11(b). Their sensitivities are indicated in the black color while measurement range in red, and the corresponding arrows show their adjustment process. As demonstrated, compared with the single SFP, the measurement sensitivity can be significantly magnified in both the FVE and HVE modes. The FVE mode shows continuously adjustable performance, while the HVE mode shows fluctuation in performance with the tuning process despite that it can achieve higher sensitivity. Besides, the variation trend of the measurement range shows the completely opposite trend as compared with that of the sensitivity.

 figure: Fig. 11.

Fig. 11. Performance comparison between FVE and HVE of proposed piezometer.

Download Full Size | PDF

4. Conclusion

In summary, we theoretically and experimentally demonstrated an in-situ adjustable fiber-optic piezometer based on a parallelly structured EFPIs by utilizing the Vernier effect. By simply adjusting the cavity length of the RFP, a water level measurement is performed in both the FVE and HVE modes using prototypes SFP1 and SFP2. In the FVE mode, the sensitivity can be predictably tuned from −0.15 nm/cm to −7.02 nm/cm with magnification factor M from 1 to 48 for SFP1, and −0.31 nm/cm to −7.22 nm/cm with M from 1 to 23 for SFP2. In the HVE mode, the sensitivity can be further enhanced up to −9.08 nm/cm but with an inconsistent performance with the adjustment process as compared to the FVE mode. Moreover, the device is featured with in-situ adjustable sensitivity, tunable measurement range, simplicity of composition, robustness, and remote sensing capability, which make it attractive in various practical applications.

Funding

National Natural Science Foundation of China (12104350); Science and Engineering Research Council (1992200001); Taishan Scholar Project of Shandong Province (tsqn201909067).

Disclosures

The authors declare no conflicts of interest.

Data availability

Data underlying the results presented in this paper are not publicly available at this time but may be obtained from the authors upon reasonable request.

References

1. A. J. Mazur, L. M. Schouten, W. Y. Lam, and P. H. Setiawan, “Nude vibrating wire piezometer installations-no filter response zone and no engineered grout,” in Proceedings of the Ninth Symposium on Field Measurements in Geomechanics, Australian Centre for Geomechanics, (Academic, 2015), pp. 487–500.

2. J. Zhao, J. Chen, X. Zhang, J. Ning, and Y. Zhang, “Distribution characteristics of floor pore water pressure based on similarity simulation experiments,” Bull. Eng. Geol. Environ. 79(9), 4805–4816 (2020). [CrossRef]  

3. M. M. Nistor, H. Rahardjo, A. Satyanaga, K. Z. Hao, Q. Xiaosheng, and A. W. L. Sham, “Investigation of groundwater table distribution using borehole piezometer data interpolation: Case study of Singapore,” Eng. Geol. 271, 105590 (2020). [CrossRef]  

4. S. Chaulya and G. M. Prasad, Sensing and monitoring technologies for mines and hazardous areas: monitoring and prediction technologies (Elsevier, 2016).

5. C. Zet, C. Foşalău, and D. Petrişor, “Pore water pressure sensor for landslide prediction,” IEEE Sens. J. 1–4 (2015).

6. M Dilawari, Forecasting models for the displacements and the piezometer levels in a concrete arch dam (McGill University, 2018).

7. I. S. Jung, Anomaly Detection of Piezometer Data Collected from Embankment Dams (Carnegie Mellon University, 2015).

8. C. N. Dourado, Characterizing Aquitard Properties from the response of Grouted Vibrating Wire Piezometers to Surface Loading (University of Saskatchewan, 2018).

9. A. J. Merritt, J. E. Chambers, W. Murphy, P. B. Wilkinson, L. J. West, S. Uhlemann, P. I. Meldrum, and D. Gunn, “Landslide activation behaviour illuminated by electrical resistance monitoring,” Earth Sur. Proc. Land. 43(6), 1321–1334 (2018). [CrossRef]  

10. A. B. Huang, C. C. Wang, J. T. Lee, and Y. T. Ho, “Applications of FBG-based sensors to ground stability monitoring,” J. Rock Mech. Geotech. Eng. 8(4), 513–520 (2016). [CrossRef]  

11. Y. T. Ho, Y. L. Wang, L. C. Chang, T. P. Wang, and J. P. Tsai, “Optical system for monitoring groundwater pressure and temperature using fiber Bragg gratings,” Opt. Express 29(11), 16032–16045 (2021). [CrossRef]  

12. W. Q. Feng, Z. Y. Liu, H. Y. Ta, and J. H. Yin, “The pore water pressure sensor based on Sagnac interferometer with polarization-maintaining photonic crystal fiber for the geotechnical engineering,” Measurement 90, 208–214 (2016). [CrossRef]  

13. D. Inaudi, R. Walder, and R. Bulatao, “Fabry-Perot Fiber Optic Sensors for Civil and Geotechnical Monitoring of Large Structures,” Struct. Health Monit. 2019.

14. A. D. Gomes, H. Bartelt, and O. Frazão, “Optical Vernier Effect: Recent Advances and Developments,” Laser Photonics Rev. 15(7), 2000588 (2021). [CrossRef]  

15. Y. Liu, X. Li, Y. N. Zhang, and Y. Zhao, “Fiber-optic sensors based on Vernier effect,” Measurement 167, 108451 (2021). [CrossRef]  

16. H. Liao, P. Lu, X. Fu, X. Jiang, W. Ni, D. Liu, and J. Zhang, “Sensitivity amplification of fiber-optic in-line Mach–Zehnder Interferometer sensors with modified Vernier-effect,” Opt. Express 25(22), 26898–26909 (2017). [CrossRef]  

17. S. Zhang, L. Yin, Y. Zhao, A. Zhou, and L. Yuan, “Bending sensor with parallel fiber Michelson interferometers based on Vernier-like effect,” Opt. Laser Technol. 120, 105679 (2019). [CrossRef]  

18. P. Robalinho, A. Gomes, and O. Frazão, “Colossal enhancement of strain sensitivity using the push-pull deformation method,” IEEE Sens. J. 21(4), 4623–4627 (2021). [CrossRef]  

19. X. Yang, S. Wu, H. Cheng, J. Ma, S. Wang, S. Liu, and P. Lu, “Simplified highly-sensitive gas pressure sensor based on harmonic Vernier effect,” Opt. Laser Technol. 140, 107007 (2021). [CrossRef]  

20. Z. Xu, Q. Sun, B. Li, Y. Luo, W. Lu, D. Liu, P. P. Shum, and L. Zhang, “Highly sensitive refractive index sensor based on cascaded microfiber knots with Vernier effect,” Opt. Express 23(5), 6662–6672 (2015). [CrossRef]  

21. Y. Jiang, Y. Yi, G. Brambilla, and P. Wang, “Ultra-high-sensitivity refractive index sensor based on dual-microfiber coupler structure with the Vernier effect,” Opt. Lett. 45(5), 1268–1271 (2020). [CrossRef]  

22. S. Wang, S. Wang, R. B. Jin, M. Feng, S. Wu, L. Zhang, and P. Lu, “All-optical demodulation fiber acoustic sensor with real-time controllable sensitivity based on optical Vernier effect,” IEEE Photonics J. 11(4), 1–11 (2019). [CrossRef]  

23. Y. Yang, Y. Wang, Y. Zhao, J. Jiang, X. He, W. Yang, Z. Zhu, W. Gao, and L. Li, “Sensitivity-enhanced temperature sensor by hybrid cascaded configuration of a Sagnac loop and a FP cavity,” Opt. Express 25(26), 33290–33296 (2017). [CrossRef]  

24. J. Li, M. Zhang, M. Wan, C. Lin, S. Huang, C. Liu, Q. He, X. Qiu, and X. Fang, “Ultrasensitive refractive index sensor based on enhanced Vernier effect through cascaded fiber core-offset pairs,” Opt. Express 28(3), 4145–4155 (2020). [CrossRef]  

25. L. Liu, T. Ning, J. Zheng, L. Pei, J. Li, J. Cao, X. Gao, and C. Zhang, “High-sensitivity strain sensor implemented by hybrid cascaded interferometers and the Vernier-effect,” Opt. Laser Technol. 119, 105591 (2019). [CrossRef]  

26. Z. Xu, Y. Luo, D. Liu, P. P. Shum, and Q. Sun, “Sensitivity-controllable refractive index sensor based on reflective θ-shaped microfiber resonator cooperated with Vernier effect,” Sci. Rep. 7(1), 1–8 (2017). [CrossRef]  

27. Q. H. Wang, X. Liu, and D. N. Wang, “Ultra-sensitive gas pressure sensor based on vernier effect with controllable amplification factor,” Opt. Fiber Technol. 61, 102404 (2021). [CrossRef]  

28. A. D. Gomes, M. S. Ferreira, J. Bierlich, J. Kobelke, M. Rothhardt, H. Bartelt, and O. Frazão, “Optical harmonic Vernier effect: A new tool for high performance interferometric fiber sensors,” Sensors 19(24), 5431 (2019). [CrossRef]  

29. A. D. Gomes, M. S. Ferreira, J. Bierlich, J. Kobelke, M. Rothhardt, H. Bartelt, and O. Frazão, “Hollow microsphere combined with optical harmonic Vernier effect for strain and temperature discrimination,” Opt. Laser Technol. 127, 106198 (2020). [CrossRef]  

30. P. M. R. Robalinho, A. D. Gomes, and O. Frazao, “High enhancement strain sensor based on Vernier effect using 2-Fiber loop mirrors,” IEEE Photonics Technol. Lett. 32(18), 1139–1142 (2020). [CrossRef]  

31. A. D. Gomes, J. Kobelke, J. Bierlich, J. Dellith, M. Rothhardt, H. Bartelt, and O. Frazão, “Giant refractometric sensitivity by combining extreme optical Vernier effect and modal interference,” Sci. Rep. 10(1), 1–14 (2020). [CrossRef]  

32. L. Liu, P. Lu, S. Wang, X. Fu, Y. Sun, D. Liu, J. Zhang, H. Xu, and Q. Yao, “UV adhesive diaphragm-based FPI sensor for very-low-frequency acoustic sensing,” IEEE Photonics J. 8(1), 1–9 (2016). [CrossRef]  

33. S. Wang, P. Lu, L. Liu, H. Liao, Y. Sun, W. Ni, X. Fu, X. Jiang, D. Liu, J. Zhang, H. Xu, Q. Yao, and Y. Chen, “An infrasound sensor based on extrinsic fiber-optic Fabry–Perot interferometer structure,” IEEE Photonics Technol. Lett. 28(11), 1264–1267 (2016). [CrossRef]  

34. S. Wang, W. Ni, L. Zhang, P. Lu, Y. Yang, and L. Wei, “Fiber-Based Infrasound Sensing,” in Advanced Fiber Sensing Technologies, L. Wei, ed. (Springer, Singapore, 2020).

35. T. Nan, B. Liu, Y. Wu, J. Wang, Y. Mao, L. Zhao, T. Sun, and J. Wang, “Ultrasensitive strain sensor based on Vernier effect improved parallel structured fiber-optic Fabry-Perot interferometer,” Opt. Express 27(12), 17239–17251 (2019). [CrossRef]  

36. Y. Zhao, M. Dai, Z. Chen, X. Liu, M. S. A. Gandhi, Q. Li, and H. Y. Fu, “Ultrasensitive temperature sensor with Vernier-effect improved fiber Michelson interferometer,” Opt. Express 29(2), 1090–1101 (2021). [CrossRef]  

37. X. Zhao, Y. Zhang, W. Zhang, Z. Li, Y. Yue, and T. Yan, “Ultrasensitive Fabry–Perot Strain Sensor Based on Vernier Effect and Tapered FBG-in-Hollow Silica Tube,” IEEE Sens. J. 21(3), 3035–3041 (2021). [CrossRef]  

Data availability

Data underlying the results presented in this paper are not publicly available at this time but may be obtained from the authors upon reasonable request.

Cited By

Optica participates in Crossref's Cited-By Linking service. Citing articles from Optica Publishing Group journals and other participating publishers are listed here.

Alert me when this article is cited.


Figures (11)

Fig. 1.
Fig. 1. Schematic diagram of EFPI structure and one prototype of the EFPI piezometer as reference interferometer.
Fig. 2.
Fig. 2. Schematic diagram of parallel structured EFPI.
Fig. 3.
Fig. 3. (a) Initial spectra of sensing fiber piezometers SFP1 and SFP2, (b) Wavelength variation of SFP1 and SFP2 along with water level.
Fig. 4.
Fig. 4. Experimental setup for water level test.
Fig. 5.
Fig. 5. (a) Spectra under water level test with one vernier structure M=10; (b) Relationship between wavelength and water level compared with that of single SFP1.
Fig. 6.
Fig. 6. (a) Vernier spectra of SFP1 with a magnification factor of 6, 10, 14, and 48; (b) Corresponded relationships between the wavelength shifts and the water level.
Fig. 7.
Fig. 7. (a) Vernier spectra of SFP2 with magnification factors of 4, 9, 13, and 23; (b) Corresponding relationships between the wavelength shifts and the water level.
Fig. 8.
Fig. 8. (a) Harmonic Vernier spectrum of SFP1 with i=1 and (b) corresponding spectra shifts with the water level.
Fig. 9.
Fig. 9. (a) Harmonic Vernier spectra of SFP1 with i=1, 2, 3, and (b) corresponding sensing curves.
Fig. 10.
Fig. 10. (a) Harmonic Vernier spectra of SFP2 with i=1, 2, 3, and (b) corresponding sensing curves.
Fig. 11.
Fig. 11. Performance comparison between FVE and HVE of proposed piezometer.

Tables (1)

Tables Icon

Table 1. Performance Comparison of Demodulation Schemes

Equations (13)

Equations on this page are rendered with MathJax. Learn more.

I = I 1 + I 2 + 2 I 1 I 2 cos ( ϕ F P + ϕ 0 ) ,
ϕ F P = 2 π 2 L λ m = 2 m π ,
λ m = 2 L m ,
F S R F P = λ m λ m + 1 = λ m λ m + 1 2 L λ 2 2 L .
Δ λ m = λ m L 0 d L d P Δ P ,
I  =  I R  +  I S A + B cos ϕ R F P + ϕ S F P 2 cos ϕ R F P ϕ S F P 2 ,
F S R e = F S R S F S R R | F S R S F S R R |  =  | λ m λ m + 1 2 ( L S L R ) | .
M = F S R e F S R S  =  F S R R | F S R S F S R R |  =  | L S L S L R | .
M = S e n v e l o p e S S F P  =  Δ λ e Δ λ m .
F S R S i = | λ m λ m + 1 2 ( L S + i L R ) | .
F S R e i = | F S R R F S R S i F S R R ( i + 1 ) F S R S i | .
F S R i e i = | ( i + 1 ) F S R R F S R S i F S R R ( i + 1 ) F S R S i | = ( i + 1 ) F S R e i ,
M i = F S R i e i F S R S i = | ( i + 1 ) F S R R F S R R ( i + 1 ) F S R S i | = ( i + 1 ) M .
Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.