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Study of a periodic spectral fluctuation existing in a fibered optical feedback cavity-enhanced absorption spectroscopy (OF-CEAS)


A special periodic spectral fluctuation is observed during the study of a fibered high sensitivity optical feedback cavity-enhanced absorption spectroscopy (OF-CEAS) for the measurement of trace gas. This spectral fluctuation is different from some phenomenon observed in former OF-CEAS which contain a resonant cavity with V-shaped configuration, such as the etalon effect and the spectral ripple effect. To reveal why this phenomenon happens and how it works, a series of hypothesis are proposed and tested, and the results show that the multi-beam interference of resonance light at the input mirror of the resonant cavity is the main reason for this phenomenon. Based on the multi-beam interference theory, a mathematical modeling of this phenomenon is built, and the theoretical analyses agree well with the experimental results. Some methods to eliminate this phenomenon are proposed and implemented, and the 1σ noise equivalent absorption coefficient of 7.6 × 10− 10 cm− 1 Hz-1/2 is attained with this robust and compact OF-CEAS system.


There is an urgent requirement for fast, high sensitivity, low detection limit and real-time trace-gas detectors for atmospheric sciences, environmental monitoring, agriculture process control and medical diagnostics nowadays [1, 2]. For example, the multi-component analysis of gas is a significant but hard work in breath gas analysis when concentration of some gas species are large and others are at extremely small, and this is extremely correlative for monitoring the exhaled human breath which contains many kinds of breath molecules at trace level. Ordinary gas analytical techniques for multi-components analysis are mass spectrometry (MS) or gas chromatography (GC) [3]. However, these techniques require expensive equipment and complicated sample preparation which makes real-time measurement not feasible. Detectors based on high finesse optical resonant cavity can achieve accurate and quantificational trace-gas detection with high sensitivity and fast response; in addition, these techniques can provide real-time analysis owing to their noninvasive and simple sample preparation features [4]. Owing to these characteristics, these methods appear to be the most promising in trace gas detection.

When the single-wavelength narrow linewidth semiconductor laser is applied in optical resonant cavity absorption spectroscopy, it seems to be the optimal selection for the detection of small gas molecules which present separated absorption lines. For example, the distributed feedback (DFB) diode laser is commercially available owing to the development needs of optical fiber communication. These compact laser source present a low power, meanwhile they provide a continuous frequency-tuning range which is extremely wider comparing to the full width at half maximum (FWHM) of molecular absorption line. Small gas molecules such as CO, CO2, NH3, HCN, C2H6, H2O, and H2S all show strong and narrow fundamental vibrational transitions in middle-infrared, simultaneously, overtone transitions lie in the near-infrared band are one to two orders of magnitude weaker in line strength. However, in the near-infrared spectral region, the DFB semiconductor lasers and photo-detectors are relatively cheaper, and these devices perform higher capability at room temperature compared to the devices working in middle-infrared region.

In the application of laser absorption spectroscopy using high finesse optical resonant cavity, representatively, cavity-enhanced absorption spectroscopy (CEAS) and cavity ring-down spectroscopy (CRDS) [5], some undesirable phenomenon often occurs in the absorption spectrum, such as the etalon effect and the spectral ripple effect [6]. These effects usually lead to the decline of system performance and restrict its applications. Therefore, it is very significant to explore why these effects happen and how they work, and find ways to eliminate or weaken their influence on the system performance [7, 8]. In this paper, a compact and robust OF-CEAS setup is presented with some fibered components. Owing to the easy replacement of DFB laser for this fibered setup, different gas molecules can be detected with the same device, as long as the selected wavelengths are in the spectral range of the cavity mirrors. A different periodic spectral fluctuation existing in absorption spectroscopy is observed during the study of this OF-CEAS experimental setup. Therefore, ways to prevent and eliminate this phenomenon is proposed. These works are significant to guide the design of fibered OF-CEAS system with V-shaped cavity and to improve the system performance.

Experimental apparatus

The minimum detectable absorption coefficient of ordinary spectrometer can be up to 10− 4 cm− 1, while it can be up to 10− 9 cm− 1 for the OF-CEAS and OF-CRDS techniques [9]. At first, CEAS was presented by Engeln et al. [10] as an improvement of CRDS in 1998. In principle, CEAS and CRDS have similar operation concept. In both techniques, the base of the experimental system is a high finesse optical resonant cavity which is formed with high reflectivity mirrors, and the high quality cavity generates a long effective optical length which can be thousands of times longer than the cavity length. In this paper, we present a fibered OF-CEAS system, and the apparatus is shown in Fig. 1. In our experimental setup, the optical cavity has a typical V-shaped configuration in which two equal arms (250 mm) forming a folded angle of 7.4°. The glass-ceramic is used as the cavity body for its ultralow expansion coefficient (~ 10− 8/°C), and the cavity mirrors are fabricated with fused quartz (diameter is 25 mm). Among them, the incident mirror (M0) is a plane mirror, M1 and M2 are spherical mirrors with 2 m radius, and the device combining M2 and a piezoelectric ceramic transducer (PZT) is used to adjust the cavity length in a tiny region. The ultra-low loss coating lie in the central area of the mirrors (R ≈ 99.99% at 1530 ± 30 nm, diameter is 10 mm). Finally, the cavity’s main body and three mirrors constitute a steady optical cavity length of 500 mm.

Fig. 1
figure 1

Schematic diagram of the OF-CEAS experimental setup employing a V-shaped cavity and a fibered DFB laser diode. The direct reflection at M0 will not return to the DFB, while part transmission light of the intra-cavity resonant field offers frequency selective optical feedback. The PZT2 mounted on the fiber collimator is used to modulate the phase of the feedback light, and the PZT1 mounted on M2 can adjust the cavity length to obtain cavity resonance

As shown in Fig. 1, this V-shaped cavity can obtain the resonant optical feedback while avoiding the direct reflection at M0. In this experimental setup, the light from DFB laser diode is coupled into a single-mode polarization maintaining (PM) fiber, then the pigtail output is connected with the port1 of a PM fiber coupler (90:10, 1550 nm Center Wavelength), and the port2 and port3 of this fiber coupler are connected with a fiber collimator (F240APC-1550, Thorlabs, Newton, NJ, USA) and a photo-detector (PDA400, Thorlabs, Newton, NJ, USA), respectively. The collimated light from the fiber collimator is then injected into the V-shaped cavity at M0. When the cavity resonance occurs, part of resonant light return to the laser diode, and PZT2 can actively optimize the feedback light phase versus the laser diode output. As we know, a small fraction of feedback resonant light can efficiently narrow the linewidth of the laser diode and also stabilize the laser frequency on the cavity’s resonance frequency automatically [11]. This is extremely valuable to sensitively detect the narrow separated absorption lines of gas molecule. It should be noted that the fibered DFB laser diode used in this setup doesn’t include an optical isolator which would prevent feedback light from the resonant cavity.

For traditional CEAS system, the spectral resolution is usually limited by the free spectral range (FSR) of the resonant cavity [12]. While in our setup, the PZT1 mounted on M2 can precisely modulate the cavity length to achieve the cavity’s resonance for each fixed laser frequency, and the spectral resolution is mainly determined by frequency tuning resolution of the DFB diode laser. Therefore, the spectral resolution of this scheme can be efficiently improved to about 0.002 cm− 1. Furthermore, in this setup, the optical feedback ratio can be regulated by applying replaceable PM fiber coupler which have different coupling ratio. For automatic operation, voltage signals of the photo-detectors are digitized with a 24-bit dynamic signal acquisition and generation device (NI-PCI-4461, 204.8 kS/s, National Instrument, Austin, TX, USA). An analogic feedback circuit for PZT2 modulation is applied, which apply the cavity mode profile as presented in transmission signal during a laser scan to generate a real-time error signal. Signal processing and control signal generation are simultaneously achieved with self-compiled software based on LabVIEW. Finally, the fitting of absorption spectra based on HITRAN database and the calculation of gas concentration are obtained after each laser scan.

Experimental phenomenon and theoretical analysis

Our primary investigation is performed with residual air in the cavity, and a fibered 1531 nm DFB diode laser is used to match several absorption lines of H2O around 6530 cm− 1. Owing to the high precision DFB diode laser driving system, high resolution of frequency tuning is attained. In the case of current tuning from 40 to 120 mA, the range is about 2.75 cm− 1 in the spectral range of 6528.95~6531.70 cm− 1 by setting its operating temperature at 25 °C. In Fig. 2, the normalized voltage signals of PD1 is presented, it is obvious that this spectrum is a combination of a periodic signal and some absorption lines.

Fig. 2
figure 2

The normalized OF-CEAS cavity transmission signal presenting a periodic spectral fluctuation include three strong absorption lines of molecular H2O

As we know, some periodic spectral signals existing in CRDS and CEAS have been observed and studied, including the spectral ripple effect and the etalon effect. The etalon effect existing in the Fabry-Perot etalon has been widely studied during the past decays [13, 14], it is caused by the multiple-beam interference at two reflecting surfaces of the Fabry-Perot etalon. The spectral ripple is mainly caused by the small mirror defects or dust particles of the folded mirror, and it has been studied by J. Morville [15] and Z. Q. Tan [16] in detail. Comparing the spectral ripple effect with the transmitted light intensity signal observed in Fig. 2, the period of this spectral signal is totally different from the spectral ripple’s period. According to the theory of spectral ripple effect, the period of this signal indicates that the length of V-Shaped cavity is just about 12 mm if this periodic spectral fluctuation is caused by the spectral ripple effect. Obviously, this length is not coincident with the cavity length L. It seems that this periodic signal in Fig. 2 is much more similar with the etalon effect. Considering that M1 and M2 are not parallel surface mirrors, and a prism is optically glued on M1 to eliminate the potential etalon effect caused by M2, this phenomenon is most likely caused by the incident mirror (M0, the thickness d is 6 mm). The incident mirror can be regarded as a Fabry-Perot cavity with a light incidence angle of 3.7° (with the surface Light intensity reflectivity R0 = 3.32% and R1 ≈ 99.99% for λ = 1530 nm). The incident light (shown in Fig. 3a as A) split into multiple beams (shown in Fig. 3a as A-1, A-2…) before coupling into the cavity, and the intra-cavity resonance light (shown in Fig. 3b as B and Fig. 3c as C) incident upon M0 with an incidence angle of 3.7° from the opposite direction, and also split into multi beams by the two surfaces of M0. This reflecting process will generate an optical path difference between these beams.

Fig. 3
figure 3

The incident mirror. In (a), the incident light A split into multiple beams, A-1 and A-2 can generate the intra-cavity resonance. b shows that the feedback light B (which is produced by incident beam A-1) split into multiple beams before coupled into the fiber collimator; c shows that the feedback light C (which is produced by incident beam A-2) split into multiple beams before coupled into the fiber collimator

Considering the theoretical output beam diameter of fiber collimator (1.6 mm) and the waist diameter of intra-cavity resonance light (1.14 mm), only the 1st and 2nd level transmitting light are considered. Therefore, when these beams are coupled into the fiber with an Anti-reflection (AR) coated aspheric lens, the multi-beam interference phenomenon occurs in both the light intensity of feedback light and the cavity transmitting light. Considering the incident light A as:

$$ {E}_i(t)={A}_0\cdot {e}^{-i\left(\omega t+ kx\right)},\left(\omega =2\pi \nu \right) $$

Here we assume the resonance field of the V-shaped cavity to be fundamental TEM0,0 mode, and the laser beam is Gaussian. Due to the limitation of the fiber collimator (diameter of AR coated aspheric lens is 11 mm), only qualified feedback light beam can be coupled into the fiber, distance between two adjacent transmitting beams is l0 = 2d cos α tan α1. Since M1 and M2 are spherical mirrors with 2 m radius, the waist of the Gaussian beam is exactly on the incident mirror, and the radius of waist size is ω0 = 0.57 mm. Here, by the integral operation, the total coupling light of the transmitting light field is calculated as:

$$ {E}_T={A}_0\cdot \sqrt{\left(1-{r}_0^2\right)\left(1-{r}_1^2\right)\left(1-{r}_2^2\right)}\cdot {e}^{-i\left(\omega t+ kx\right)}\cdot {e}^{-i\left({\delta}_0+{\delta}_1\right)}\cdot \left(1+{\varphi}_0{r}_0{r}_1{e}^{-i2{\delta}_0}\right)\cdot \phi $$

The total coupling light of the feedback light field is:

$$ {\displaystyle \begin{array}{l}{E}_F={A}_0\cdot \left(1-{r}_0^2\right)\left(1-{r}_1^2\right){r}_2\cdot {e}^{-i\left(\omega t+ kx\right)}\cdot {e}^{-i2\left({\delta}_0+{\delta}_1\right)}\\ {}\cdot \left(1+{\varphi}_1{r}_0{r}_1{e}^{-i2{\delta}_0}+{\varphi}_0{\varphi}_2{r}_0{r}_1{e}^{-i2\left({\delta}_0+{\delta}_1\right)}+{\varphi}_0{r}_0^2{r_1^2}_1{e}^{-i2\left(2{\delta}_0+{\delta}_1\right)}\right)\cdot \phi \end{array}} $$

Here \( {\delta}_0= nd\cdot \frac{2\pi }{\lambda }/\cos \left(\alpha \right) \), \( {\delta}_1={\delta}_2=L\cdot \frac{2\pi }{\lambda } \), \( \phi =\raisebox{1ex}{$1$}\!\left/ \!\raisebox{-1ex}{$1-{r}_1^2{r}_2{r}_3{e}^{-i2\left({\delta}_1+{\delta}_2\right)}$}\right. \), n is the reflective index of quartz glass (n = 1.444), d is the thickness of M0 (d = 6 mm), L is the length of each cavity arm (L = 250 mm), and α is the incidence angle (α = 3.7°). r0, r1, r2, and r3 represent the amplitude reflectivity of the mirror surface (\( {r}_0^2=3.32\% \), \( {r}_1^2={r}_2^2={r}_3^2\approx 99.99\% \)), φ0, φ1 and φ2 are the coupling coefficient of incident beam A-2, B-2 and C-2, respectively (φ0 ≈ 80 % , φ1 ≈ 80 % , φ2 ≈ 100%). The coupling coefficient is mainly determined by the optical path difference between these beams and the optical axis of cavity (or optical axis of output laser), as well as the diameter of laser beam.

To confirm this assumption, we did some adjustments with this experimental setup. The fiber coupler in Fig. 1 is replaced by a 2 × 2 PM Fiber Coupler (50:50, 1550 nm Center Wavelength), and the feedback light is divided into two portions. One of them is connected to PD2 to observe the feedback light intensity, and another one returns to the DFB laser diode. According to our multi-beam interference assumption and simulation based on Formula (2) and (3), the interference phenomenon in feedback light intensity is strengthened for it passes through M0 twice. As shown in Figs. 4 and 5, the experimental results confirm to the theoretical simulation very well, obviously, the spectral fluctuation in the feedback light is more obvious than which in the transmitted light.

Fig. 4
figure 4

The cavity transmitted light signal (black) and the simulation results (red). The simulation results include the interference effect calculated using the Formula (2) and simulation of the absorptions based on HITRAN 2012 (P = 1.0 atm, T = 25 °C)

Fig. 5
figure 5

The feedback light signal (black) and the simulation results (red). The simulation results includes the interference effect calculated using the Formula (3) and simulation of the absorptions based on HITRAN 2012 (P = 1.0 atm, T = 25 °C)

In Fig. 4, the black dots are the transmitted light intensity signal measured by PD1. The red dots show the calculated result based on Formula (2) and HITRAN 2012 database, which contain the periodic spectral fluctuation and several absorption lines of H2O around 6530 cm− 1. The comparison of the measured spectra in Figs. 4 and 5 show that the amplitude of the periodic spectral fluctuation in feedback light signal is larger than which in transmitted light signal. It should be noted that the concentration of H2O in Figs. 4 and 5 has a preset value of 1.5%, and the simulation results is revised after the effective value is calculated in Fig. 6.

Fig. 6
figure 6

a shows the transmitted light signal of the developed OF-CEAS system; b shows the absorption coefficient spectrum (black) and Voigt fitting of the absorptions of molecular H2O (red and green) based on HITRAN 2012 (P = 1.0 atm, T = 25 °C); the bottom shows the fit residual

Since that these experimental results agree well with the mathematical modeling results, the main cause of this periodic spectral fluctuation is determined to be the multi-beam interference of resonance light at the incident mirror (M0). Methods to eliminate or weaken this effect are proposed as follows:

  1. 1)

    The surface of M0 are wedged;

  2. 2)

    The surface of M0 is coated with anti-reflecting film;

  3. 3)

    A prism is optically glued on the backside of M0;

  4. 4)

    Increase the thickness of M0 (show as d).

In methods 1 and 3, the non-parallel surfaces of M0 will eliminate the interference terms. With respect to method 2, the reflectivity R0 is reduced when the surface is coated with anti-reflection film, and the interference terms will decrease as shown in Formula (2) and (3). In method 4, the distance between two adjacent transmitting beams is l0, it is obvious that l0 is proportional to d (the thickness of M0). When l0 is larger enough, the beam A-2 will not be resonant considering the limited area of film (diameter ϕ = 10 mm), and the beam B-2 will not be coupled into the fiber because of the diameter of fiber collimator (diameter ϕ = 11 mm).

In all these methods mentioned above, all the interference terms can be totally eliminated with methods 1 and 3. However, the observed periodic spectral fluctuation in this fibered OF-CEAS setup does not appear in typical “open light path” OF-CEAS system, the usage of a prism makes our experimental setup more flexible. In general, we think “A prism is optically glued on the backside of M0” is the most simple and practical method for our experimental setup. To verify its effectiveness, a right angle prism with a sharp angle of 27 degrees is optically glued on the backside of M0. The OF-CEAS signal is measured again with the same measurement subject, and the result is shown in Fig. 6a. Apparently, the periodic spectral fluctuation disappears, and this experimental result coincides with the analyses described above.

Figure 6 shows a single laser scan of our OF-CEAS system in about 10 s. The 1531 nm DFB diode laser is tuned to match several absorption lines of H2O around 6530 cm− 1 (the strongest absorption line intensity is 2.926 × 10‐24 cm‐1/(molecule × cm‐2) at 6530.05 cm‐1 according to HITRAN database). The absorption coefficient α is determined by the transmitted intensity (I) with the OF-CEAS formula [17]:

$$ \alpha =\frac{1\hbox{-} {R}_{eff}}{L_0}\left(\sqrt{\frac{I_0}{I}}-1\right) $$

where L0 is the physical cavity length, Reff is the equivalent reflectivity of mirrors which is determined by the “empty cavity” ring-down time (τ0), therefore, (1-Reff) represents the cavity optical loss in a single pass. The reference intensity signal (I0) was confirmed by the transmitted light intensity without absorption.

The ultra-low loss coating is designed and manufactured by ourselves (R ≈ 99.99% at 1530 ± 30 nm). In this experimental setup, a fast fibered optical switch can be placed between the DFB laser diode and the fiber coupler to produce instantaneous interruption of the laser (10 ns). When the cavity is filled with pure N2, the “empty cavity” ring-down time τ0 is determined to be τ0 = 7.75 μs at 1531.4 nm, corresponding to a cavity loss of (1-Reff) = 215 ppm in a single pass. For each mirror, the effective value of light intensity reflectivity is determined to be 99.98925%, the approximate value of 99.99% is used during the simulation of Formula (2) and (3). The residuals of the fitting indicate that the 1σ noise equivalent absorption coefficient of 7.6 × 10− 10 cm− 1 Hz-1/2 is achieved, corresponding to a minimum detectable absorption coefficient of αmin = 3.4 × 10− 9 cm− 1. Using the relation α = n*σ (σ represents the absorption cross-section for a predetermined gas) [18], the concentration of H2O in the cavity is calculated as 1.46%. The higher performance can be obtained by the fitting of repeated absorption coefficient spectra, and a better minimum detectable absorption coefficient of αmin = 1.1 × 10− 9 cm− 1 is achieved after the averaging of 10 laser scans.


We have presented a novel fibered OF-CEAS system with an enhanced spectral resolution. This OF-CEAS system require fewer optical components, it is suitable to the achievement of robust, low power, compact, and economical instruments for trace gas detection. For the periodic spectral fluctuation appearing in the primary investigation of this OF-CEAS system, its mechanism is analyzed and the mathematical model is proposed, and the experimental results agree well with the theoretical simulation. Some technical proposals are proposed to eliminate this periodic spectral fluctuation, and the experimental results show that this spectral fluctuation can be eliminated efficiently when a prism is optically glued on the backside of the incident mirror. With these improvement, the 1σ noise equivalent absorption coefficient of 7.6 × 10− 10 cm− 1 Hz-1/2 is achieved in a single scan within 10 s, and real-time measurement of some trace gas at the ppb level can be achieved. The sensor based on this fibered OF-CEAS is compact, robust and economically available, it can offer accurate selectivity, high sensitivity, non-invasive and real time monitoring as well as no harm for patients when it is applied in human breath diagnosis. The next step of our work is exploiting the performance of this fibered OF-CEAS in the measurement of ammonia and hydrogen cyanide existing in exhaled human breath gas, the detection limit of this system would permit a concentration detection limit of 12.5 ppb for NH3 at 1531 nm. Furthermore, this fibered OF-CEAS setup permits easy replacement for the DFB laser operating in the range of cavity mirrors, the multi-component analysis of gas can be accomplished with this OF-CEAS setup. We are looking forward to developing an instrument for breath gas analysis which is suitable for clinical application.

Availability of data and materials

The datasets used and analyzed during the current study are available from the corresponding author on reasonable request.


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This research was funded by the Research Project of National University of Defense Technology (No. ZK16–03-21).

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XL proposed the concept of this study, and was a contributor in review and editing for this manuscript. ZT acquired the funding for this research work. ZL performed the investigation and experimental research, and was the major contributor in writing and editing the manuscript. All authors read and approved the final manuscript.

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Correspondence to Xingwu Long.

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Luo, Z., Tan, Z. & Long, X. Study of a periodic spectral fluctuation existing in a fibered optical feedback cavity-enhanced absorption spectroscopy (OF-CEAS). J. Eur. Opt. Soc.-Rapid Publ. 15, 23 (2019).

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