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ORIGINAL RESEARCH article

Front. Phys., 30 September 2022
Sec. Atomic and Molecular Physics

Light intensity correction for quartz-enhanced photoacoustic spectroscopy using photothermal baseline

Xiang Chen,Xiang Chen1,2Mai Hu,Mai Hu2,3Hao Liu,Hao Liu2,3Lu YaoLu Yao2Zhenyu XuZhenyu Xu2Ruifeng Kan
Ruifeng Kan2*
  • 1Jinlin Institute of Technology, Nanjing, China
  • 2Hefei Institute of Physical Science, Chinese Academy of Sciences, Hefei, China
  • 3University of Science and Technology of China, Hefei, China

A convenient method of light intensity correction for quartz-enhanced photoacoustic spectroscopy (QEPAS) using photothermal baseline is demonstrated. The laser beam passes through the prongs of the quartz tuning fork (QTF) and then focused on the root of the prongs. First harmonic (1f) analysis is utilized to process the simultaneously induced photoacoustic and photothermal signals. The optical path length for photothermal spectroscopy is minimized to millimeter level, yielding negligible gas absorption. The demodulated 1f signal can be regarded as the superposition of the photoacoustic signal and the non-absorption photothermal baseline. A good linear relationship (R2 = 0.999) is observed between amplitude of photothermal baseline and light intensity. QEPAS signal normalized by photothermal baseline shows a good immunity to light intensity variation. An excellent linear response between normalized QEPAS signal and gas concentration is achieved. According to the Allan deviation analysis, the minimum detection limit for CH4 is 0.31 ppm at an integration time of 1,200 s. With this strategy, the precise gas concentration and accurate light intensity of a QEPAS system can be simultaneously obtained with only a single QTF. Compared with the light intensity correction using a photodetector or a power meter, this method entails a low cost and small footprint. It is promising to mitigate the influence from light intensity drift in long-term field measurement of QEPAS systems.

1 Introduction

Quartz-enhanced photoacoustic spectroscopy has been widely employed in trace gas sensing due to its immunity to environmental noise, high detection sensitivity and small size [14]. When modulated laser emission is in resonance with gas analyte, its successive non-radiative relaxation [57] can generate acoustic waves. Acoustic microresonators with appropriate configurations are usually employed to improve the photoacoustic sensitivity [79]. The QEPAS signal is proportional to light intensity, while laser intensity-induced fluctuations could be eliminated with simple compensation process by synchronously measuring the laser intensity variation [1013] using a photodetector or a power meter. Hence, precise gas concentration can be obtained in long-term filed applications. However, additional photodetector (PD) or power meter will bring detection errors and biases and needs to be calibrated periodically. Moreover, the PD or power meter will entail a high cost and complexity especially for mid-infrared or terahertz laser-based QEPAS system. Furthermore, it can be much more complex to handle light intensity drifts when the light system comprises multiple lasers of different wavelengths or instantaneous broadband spectral coverage [1417], especially when the responsivity of the PD or the power meter varies with wavelength.

Similar to QEPAS, the QTF can also be used as the high-performance photothermal transducer for quartz-enhanced photothermal spectroscopy (QEPTS) [1820]. While the laser radiation modulated at the resonance frequency hits the surface of the QTF, the prongs will vibrate due to the light-thermo elastic conversion. The piezoelectric current is then converted to output voltage by a trans-impedance amplifier and the harmonic components can be retrieved with a lock-in amplifier. QEPTS is a non-contact measurement technique that can be used for remote gas detection [2123]. With the application of scanned wavelength modulation strategy, offset of the demodulated 1f component is proportional to the light intensity and can be utilized to trace the fluctuations of light intensity [24]. However, this requires tricky modulation to stay within the resonance curve of the high quality tuning fork, which makes it less convenient in the application of QPEAS-based sensors.

To mitigate the light intensity drift easily during long-term field measurement for QEPAS systems, we report a method of light intensity correction using photothermal baseline. The CH4 absorption line at 1,653.72 nm, as an example, is experimentally investigated. The distributed feedback (DFB) fiber-coupled semiconductor laser is controlled with scanned wavelength modulation technology. Output laser beam passes through the prongs of the QTF and then focused on the root of the prongs so as to inspire photoacoustic and photothermal signals simultaneously. To minimize the gas absorption for QEPTS, the optical path length is designed as short as 8 mm. First harmonic analysis is performed to process the raw photoacoustic-thermal signals. The relationship between light intensity and photothermal baseline is explored. The concentration calibration and Allan deviation analysis are performed to evaluate the sensor performance. With the 1f analysis, precise gas concentration and accurate light intensity can be concurrently detected.

2 Principles of quartz-enhanced photoacoustic spectroscopy and quartz-enhanced photothermal spectroscopy

When a DFB laser is modulated by a sinusoidal modulation current, the laser frequency v(t) and output intensity I(t) can be expressed as [25, 26]

v(t)=v¯+acos(ωt)(1)
I(t)=I0¯[1+i0cos(ωt+1)+i2cos(2ωt+2)](2)

where v¯ is the laser center frequency, a is the modulation depth, ω is the modulation frequency, I0¯ is the average laser intensity, i0 and i2 represent the linear and nonlinear intensity modulation amplitude, 1 and 2 are the phase shifts of the linear and nonlinear term. The non-linear orders of the output intensity beyond 2 are neglected because of their weak amplitudes. The absorption coefficient for QEPAS can be expanded into a Fourier series [27]:

α(v)=CNSφ(v)=n=0Hn(v¯,a)cos(nωt)(3)

where C is the gas concentration, N is the total molecular density, S is the line strength, φ(v) is the normalized line shape function, Hn is the nth order Fourier coefficient of absorption for QEPAS. The QEPAS signal is given by

SQEPAS=kQEPASI(t)α(v)(4)

where kQEPAS is the constant of the photoacoustic spectroscopy. For the sake of simplicity, the phase shift between gas absorption and photoacoustic signal is neglected. Eq. 4 can be further described as

SQEPAS=kQEPASI0¯[1+i0cos(ωt+1)+i2cos(2ωt+2)]n=0Hn(v¯,a)cos(nωt)(5)

Mathematically, demodulating the signal means multiplying Eq. 5 by cos(ωt) and taking the average over one period of the modulation signal. As a result, the first harmonic component of QEPAS signal can be expressed as

X1f_QEPAS=12kQEPASI0¯[H1+i0(H0+12H2)cos1+12i2(H1+H3)cos2](6)

The Fourier coefficients of absorption for QEPAS with orders larger than 3 are strictly equal to 0. According to Eq. 6, the first harmonic component of QEPAS signal is proportional to laser intensity and gas concentration. Also, the first harmonic component for QEPAS will turn to zero for non-absorption conditions, which makes QEPAS a background-free technique. The QEPTS signal is given by [28].

SQEPTS=kQEPTSI(t)(1SPCLφ(v))(7)

where kQEPTS is the constant of the photothermal spectroscopy, P is the gas pressure, L is the optical path length. Similar to QEPAS, Eq. 7 can be described as

SQEPTS=kQEPTSI0¯[1+i0cos(ωt+1)+i2cos(2ωt+2)](1m=0hm(v¯,a)cos(mωt))(8)

where hm is the mth order Fourier coefficient of absorption for QEPTS. Demodulating the QEPTS signal with the in-phase reference signal, the first harmonic component of QEPTS can be expressed as

X1f_QEPTS=12kQEPTSI0¯[h1+i0(1+h0+12h2)cos1+12i2(h1+h3)cos2](9)

According to Eq. 6 and Eq. 9, the main differences between 1f photoacoustic and photothermal signals are the non-absorption background and the response coefficient. If L is short enough to generate a thin absorption, the absorption part of QEPTS can be neglected and Eq. 9 can be simplified as

X1f_QEPTS=12kQEPTSI0¯i0cos1(10)

Hence, the non-absorption first harmonic signal of QEPTS is independent from the h factors and is proportional to laser intensity. If we can obtain the photoacoustic and photothermal signals simultaneously, the QEPAS signal is equal to zero theoretically and the QEPTS signal is proportional to light intensity in the non-absorption area of the spectrum. By normalizing the QEPAS signal to the non-absorption first harmonic signal of QEPTS, the dependence of QEPAS on laser intensity can be intrinsically removed.

3 Experimental setup

Figure 1 shows the schematic diagram of the research on light intensity correction for QEPAS using photothermal signal. A distributed feedback fiber-coupled semiconductor laser with a center wavelength of 1,654 nm is utilized as the light source and is operated by the home-made temperature and current driver. The CH4 absorption line located at 1,653.72 nm is investigated in this experiment. A sinusoidal wave at the resonant frequency of the QTF is superimposed with another sinusoidal wave of 0.04 Hz to modulate the injection current of the DFB laser. The modulation and scanning signals are generated by a waveform generator (SDG1032X, Siglent) and are superposed using a home-made adder. Reference signal used for demodulation is also generated by the waveform generator. The modulated laser beam is collimated with the fiber collimator (FC) and then passes through the prongs of the QTF. A pair of on-beam acoustic micro-resonators are employed to increase the amplitudes of QEPAS signal. A reflector coated with gold film (R>99%) is utilized to reflect the transmission beam to the root of the two prongs of the QTF. The laser beam diameter at the two focusing positions is calculated to be about 0.15 mm. With this configuration, the photoacoustic and photothermal signals can be simultaneously generated. Since the optical path length for QEPTS is only 8 mm, the corresponding gas absorption can be neglected. Piezoelectric current induced by photoacoustic and photothermal effects is converted to voltages by a low noise trans-impedance pre-amplifier with a 10 MΩ feedback resistor. A lock-in amplifier (RS865A, Stanford Research Systems) is used to retrieve the combined 1f component from the photoacoustic-thermal signal. Data acquisition of the 1f signal is performed by a data acquisition device (USB 6363, National Instruments) with a sampling rate of 2 kS/s and a vertical resolution of 16 bits. The raw 1f signal is averaged over 10 scans to enhance the signal-to-noise ratio. All data processing is implemented by a computer.

FIGURE 1
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FIGURE 1. Schematic diagram of the experimental setup. FC: fiber collimator; MR: micro-resonators; R: reflector.

4 Results and discussion

4.1 Frequency response of quartz tuning fork

The properties of the QTF are investigated via a function generator. Sinusoidal signal ranging from 32701.00 Hz to 32741.00 Hz with a step of 1.00 Hz is injected into the QTF. Peak value of output signal from the QTF is recorded with the data acquisition device and the response curve can be well fitted by a Lorentz profile. As shown in Figure 2, the intrinsic resonant frequency and bandwidth are measured as 32721.60 Hz and 6.81 Hz, respectively, yielding a quality factor of 4,804. In the following experiments, the modulation frequency of 32721.60 Hz for CH4 detection is selected and the corresponding 1f signal is retrieved to demonstrate the method of light intensity correction for QEPAS sensor.

FIGURE 2
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FIGURE 2. Frequency response curve of the QTF fitted with the Lorentz profile.

4.2 Modulation signal optimization

The laser modulation depth, which relates to the modulation current, should be optimized to improve the amplitude of the 1f signal. The sinusoidal scanning signal of 0.04 Hz, superimposed with a sinusoidal modulation signal of 32721.60 Hz is utilized to modulate the laser current. CH4 gas sample of a fixed concentration is injected into the photoacoustic cell with a flow rate of 50 ml/min. The 1f components of different modulation currents are obtained by demodulating the output signals from the QTF. Figure 3 depicts the relationship between the 1f amplitude and modulation current. The maximum 1f amplitude is achieved while the modulation current is 35 mA. Therefore, the optimized modulation current of 35 mA is selected for CH4 detection in the subsequent investigations.

FIGURE 3
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FIGURE 3. 1f signal amplitudes of CH4 corresponding to varied modulation currents.

4.3 Investigation on light intensity correction

To demonstrate the method of light intensity correction for QEPAS using photothermal baseline, the output light intensity is adjusted by an attenuator from 4.03 mW to 16.82 mW. Standard gas samples of 500-ppm CH4 and pure N2 are introduced into the photoacoustic cell selectively with a flow rate of 50 ml/min and the measured 1f components under different laser intensities are recorded. The modulation signal during one scanning cycle is shown in Figure 4A. Figure 4B demonstrates typical 1f signals under different conditions while the light intensity is 16.82 mW. The solid red line indicates the QEPAS signal of 500-ppm CH4 without QEPTS signal by blocking the reflector. The dotted blue line indicates the photoacoustic-thermal signal of 500-ppm CH4 while the reflector is installed. The solid blue line indicates the photothermal signal while the reflector is installed and photoacoustic cell is filled with pure N2. It could be seen that the demodulated photoacoustic-thermal signal can be regarded as the superposition of the photoacoustic signal and the non-absorption photothermal baseline. Moreover, the amplitude of the photothermal baseline is barely interfered by the gas absorption. The photoacoustic signal becomes negligible compared to the photothermal signal in the non-absorption area during one scanning cycle.

FIGURE 4
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FIGURE 4. (A) The modulation signal during one scanning cycle; (B) Typical 1f signals under different conditions.

Figure 5A depicts the measured 1f photoacoustic-thermal signals under different light intensities. The relationship between amplitude of the photothermal baseline and light intensity is plotted in Figure 5B. An excellent linear relationship is observed with a correlation coefficient of 0.999. The relationship between peak-to-peak amplitude of the photoacoustic-thermal signal and light intensity is plotted in Figure 6A, also indicating an excellent linear relationship (R2 = 0.999). Figure 6B shows the peak-to-peak amplitudes of the photothermal-acoustic signals normalized by the amplitudes of the photothermal baselines under different light intensities. It can be seen that the peak-to-peak amplitude change of the photothermal-acoustic signal induced by varying light intensity can be corrected accurately with the photothermal baseline. The maximum deviation of the normalized peak-to-peak amplitude is within 0.7% under different light intensity from 4.03 mW to 16.82 mW.

FIGURE 5
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FIGURE 5. (A) Photoacoustic-thermal signals under different light intensities; (B) Amplitudes of photothermal baselines under different light intensities.

FIGURE 6
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FIGURE 6. (A) Peak-to-peak values of photoacoustic-thermal signals under different light intensities; (B) Normalized peak-to-peak values of photoacoustic-thermal signals under different light intensities.

4.4 Concentration calibration

The response of the detection system at different concentrations of gas samples is investigated. Pure N2 and standard gas samples of CH4 (200 ppm, 300 ppm, 400 ppm, 500 ppm, 600 ppm, 700 ppm, 800 ppm) are introduced into the photoacoustic cell successively at a flow rate of 50 ml/min. Raw 1f photoacoustic-thermal signals under different gas concentrations are demonstrated in Figure 7A. The peak-to-peak values of photoacoustic-thermal signals normalized by the amplitudes of photothermal baselines are calculated and a good linear relationship (R2 = 0.998) between gas concentration and peak-to-peak value for different gas samples is observed in Figure 7B.

FIGURE 7
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FIGURE 7. (A) Photoacoustic-thermal signals under different gas concentrations; (B) Calibration of the detection responsivity.

4.5 Allan deviation

The minimum detection limit of the detection system for CH4 is studied as a function of integration time. The standard gas sample of 500-ppm CH4 is introduced into the photoacoustic cell continuously and the peak-to-peak value of photothermal-acoustic signal normalized by photothermal baseline is recorded during a long time period. Allan deviation analysis is performed and the experimental results are plotted in Figure 8. The 25-s detection limit of 2.72 ppm for CH4 is achieved. With an optimum integration time of about 1,200 s, the minimum detection limit for CH4 can be improved to 0.31 ppm.

FIGURE 8
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FIGURE 8. Allan deviation analysis.

5 Conclusion

In this article, we have reported a convenient method of light intensity correction for QEPAS using photothermal baseline. To illustrate its feasibility, the laser beam passes through the prongs of the QTF and then focuses on the root of the prongs. The photoacoustic and photothermal signals are induced simultaneously on the same QTF. Since the optical path length for photothermal spectroscopy is as short as 0.8 cm, the corresponding gas absorption can be neglected. With the 1f analysis, precise gas concentration and accurate light intensity for CH4 detection can be obtained at the same time. QEPAS signal normalized by photothermal baseline shows a good immunity to light intensity changes. An excellent linear response between normalized QEPAS signal and gas concentration is observed. According to the Allan deviation analysis, a minimum detection limit of 0.31 ppm for CH4 is achieved. With this detection strategy, laser intensity-induced fluctuations of the QEPAS signal could be eliminated conveniently with the photothermal baseline. Compared with the light intensity correction using a photodetector or a power meter, this method entails a low cost and a small footprint. It will be promise to handle light intensity drifts when the light system comprises multiple lasers of different wavelengths or instantaneous broadband spectral coverage, especially when the responsivity of the PD or the power meter varies with wavelength. The proposed method will also work while there is a phase shift between laser intensity and the excited sound wave. While laser absorption along the path becomes significant for photothermal signal, the 1f signal can still be regarded as the superposition of the photoacoustic and photothermal signal. We can increase the scanning range of the injection current of the laser to obtain the non-absorption area in the spectrum. However, due to the absorption of the photothermal signal, peak-to-peak value of the 1f signal in the absorption area may change subsequently. Since the installation and adjustment of the internal reflector may be complicated, an improved structure with a reflector located outside the photoacoustic cell will be studied further.

Data availability statement

The raw data supporting the conclusions of this article will be made available by the authors, without undue reservation.

Author contributions

XC, Data curation, Formal analysis, Methodology, Writing—original draft. MH, Conceptualization, Visualization, Writing—review and editing. HL, Formal analysis, investigation. LY, Software, Validation. ZX, Resources, Validation. RK, Writing—review and editing.

Funding

This research was supported by the National Key Research and Development Project (2019YFB2006003), the Foundation from the Key Laboratory of Environmental Optics and Technology (2005DP173065-2021-03), and the Strategic Priority Research Program of the Chinese Academy of Sciences (XDA22020502).

Conflict of interest

The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.

Publisher’s note

All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.

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Keywords: photoacoustic spectroscopy, quartz tuning fork, photothermal spectroscopy, laser intensity correction, first harmonic analysis

Citation: Chen X, Hu M, Liu H, Yao L, Xu Z and Kan R (2022) Light intensity correction for quartz-enhanced photoacoustic spectroscopy using photothermal baseline. Front. Phys. 10:1009843. doi: 10.3389/fphy.2022.1009843

Received: 02 August 2022; Accepted: 15 September 2022;
Published: 30 September 2022.

Edited by:

Karol Krzempek, Wrocław University of Science and Technology, Poland

Reviewed by:

Jean-Michel Melkonian, Office National d'Études et de Recherches Aérospatiales, France
Xiaohui Li, Shaanxi Normal University, China

Copyright © 2022 Chen, Hu, Liu, Yao, Xu and Kan. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

*Correspondence: Ruifeng Kan, kanruifeng@aiofm.ac.cn

Disclaimer: All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article or claim that may be made by its manufacturer is not guaranteed or endorsed by the publisher.