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<journal-id journal-id-type="publisher-id">Front. Phys.</journal-id>
<journal-title>Frontiers in Physics</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Phys.</abbrev-journal-title>
<issn pub-type="epub">2296-424X</issn>
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<publisher-name>Frontiers Media S.A.</publisher-name>
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<article-meta>
<article-id pub-id-type="publisher-id">1488578</article-id>
<article-id pub-id-type="doi">10.3389/fphy.2024.1488578</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Physics</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>A wide-range temperature sensor with a single diode laser based on H<sub>2</sub>O absorption spectra near 1850.5 nm</article-title>
<alt-title alt-title-type="left-running-head">Ai et al.</alt-title>
<alt-title alt-title-type="right-running-head">
<ext-link ext-link-type="uri" xlink:href="https://doi.org/10.3389/fphy.2024.1488578">10.3389/fphy.2024.1488578</ext-link>
</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Ai</surname>
<given-names>Suman</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/2829282/overview"/>
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<role content-type="https://credit.niso.org/contributor-roles/software/"/>
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<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Xu</surname>
<given-names>Zhenyu</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1878982/overview"/>
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</contrib>
<contrib contrib-type="author">
<name>
<surname>Huang</surname>
<given-names>An</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/2406325/overview"/>
<role content-type="https://credit.niso.org/contributor-roles/conceptualization/"/>
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</contrib>
<contrib contrib-type="author">
<name>
<surname>Deng</surname>
<given-names>Hao</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/2713910/overview"/>
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<contrib contrib-type="author">
<name>
<surname>Niu</surname>
<given-names>Rantong</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
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<contrib contrib-type="author">
<name>
<surname>Kan</surname>
<given-names>Ruifeng</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
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<aff id="aff1">
<sup>1</sup>
<institution>Department of Environmental Science and Optoelectronic Technology</institution>, <institution>University of Science and Technology of China</institution>, <addr-line>Hefei</addr-line>, <country>China</country>
</aff>
<aff id="aff2">
<sup>2</sup>
<institution>Anhui Institute of Optics and Fine Mechanics</institution>, <institution>Hefei Institutes of Physical Science</institution>, <institution>Chinese Academy of Sciences</institution>, <addr-line>Hefei</addr-line>, <country>China</country>
</aff>
<author-notes>
<fn fn-type="edited-by">
<p>
<bold>Edited by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/765483/overview">Yufei Ma</ext-link>, Harbin Institute of Technology, China</p>
</fn>
<fn fn-type="edited-by">
<p>
<bold>Reviewed by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1899099/overview">Wei Ren</ext-link>, Xi&#x2019;an University of Posts and Telecommunications, China</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/998080/overview">Zongliang Wang</ext-link>, Liaocheng University, China</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/2039087/overview">Fupeng Wang</ext-link>, Ocean University of China, China</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Zhenyu Xu, <email>zyxu@aiofm.ac.cn</email>
</corresp>
</author-notes>
<pub-date pub-type="epub">
<day>05</day>
<month>12</month>
<year>2024</year>
</pub-date>
<pub-date pub-type="collection">
<year>2024</year>
</pub-date>
<volume>12</volume>
<elocation-id>1488578</elocation-id>
<history>
<date date-type="received">
<day>30</day>
<month>08</month>
<year>2024</year>
</date>
<date date-type="accepted">
<day>15</day>
<month>11</month>
<year>2024</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2024 Ai, Xu, Huang, Deng, Niu and Kan.</copyright-statement>
<copyright-year>2024</copyright-year>
<copyright-holder>Ai, Xu, Huang, Deng, Niu and Kan</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/">
<p>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.</p>
</license>
</permissions>
<abstract>
<p>We have developed a compact sensor utilizing a tunable diode laser near 1850.5 nm to measure H&#x2082;O absorption for wide-range temperature diagnostics. The sensor&#x2019;s performance was experimentally evaluated in a tube furnace at temperatures ranging from 600 to 1800 K and pressures from 3.5 to 103 kPa, showing a relative error between the measured and set temperatures of &#x2212;2%&#x2013;3.5%. The numerical simulations confirmed the sensor&#x2019;s suitability for temperature measurements between 500 and 2500 K, with the accuracy of absorbance extraction being a critical factor. The above results suggest that the sensor is highly effective for temperature measurement across a broad range and holds potential for applications in aerospace and industrial combustion diagnostics.</p>
</abstract>
<kwd-group>
<kwd>temperature sensor</kwd>
<kwd>1850.5 nm diode laser</kwd>
<kwd>tunable diode laser absorption spectroscopy</kwd>
<kwd>wide-range temperature measurement</kwd>
<kwd>good sensing performance</kwd>
</kwd-group>
<contract-sponsor id="cn001">National Science and Technology Major Project<named-content content-type="fundref-id">10.13039/501100018537</named-content>
</contract-sponsor>
<custom-meta-wrap>
<custom-meta>
<meta-name>section-at-acceptance</meta-name>
<meta-value>Optics and Photonics</meta-value>
</custom-meta>
</custom-meta-wrap>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>Highly accurate and fast-response measurements of temperature and species concentration are critical in assessing combustion efficiency, which directly influences thermal performance in various combustion systems, such as gas turbines, scramjets, wind tunnels, shock tubes, laboratory flames, and industrial-scale combustors [<xref ref-type="bibr" rid="B1">1</xref>&#x2013;<xref ref-type="bibr" rid="B3">3</xref>]. Among the available diagnostic techniques, tunable diode laser absorption spectroscopy (TDLAS) is widely adopted for retrieving combustion temperature and species concentration due to its robustness, high sensitivity, fast response, and non-intrusive measurement capabilities [<xref ref-type="bibr" rid="B4">4</xref>&#x2013;<xref ref-type="bibr" rid="B8">8</xref>]. This technique detects specific absorption features of target gases, such as water vapor (H&#x2082;O), which is a major product in combustion and has been frequently used as a target gas in TDLAS-based diagnostics [<xref ref-type="bibr" rid="B9">9</xref>, <xref ref-type="bibr" rid="B10">10</xref>]. H&#x2082;O exhibits several strong absorption bands in the infrared region [<xref ref-type="bibr" rid="B11">11</xref>], as illustrated in <xref ref-type="fig" rid="F1">Figure 1</xref>.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Absorption line strength of H<sub>2</sub>O at 1600 K in infrared spectral region.</p>
</caption>
<graphic xlink:href="fphy-12-1488578-g001.tif"/>
</fig>
<p>At a typical combustion temperature of 1,600 K, the line strengths are plotted across a wavelength range from 1 to 10 &#x3bc;m. These absorption bands occur at 1.4 &#x3bc;m (<italic>v</italic>
<sub>1</sub>&#x2b;<italic>v</italic>
<sub>3</sub>), 1.8 &#x3bc;m (<italic>v</italic>
<sub>1</sub>&#x2b;<italic>v</italic>
<sub>2</sub>&#x2b;<italic>v</italic>
<sub>3</sub>), 2.7 &#x3bc;m (<italic>v</italic>
<sub>1</sub>&#x2b;<italic>v</italic>
<sub>2</sub>&#x2b;<italic>v</italic>
<sub>3</sub>), 5.5 &#x3bc;m (<italic>v</italic>
<sub>2</sub>), and 6.5 &#x3bc;m (<italic>v</italic>
<sub>1</sub>&#x2b;<italic>v</italic>
<sub>2</sub>), with the line strengths at 2.7 &#x3bc;m, 5.5 &#x3bc;m, and 6.5 &#x3bc;m being approximately 10 times stronger than those at 1.4 &#x3bc;m and 1.8 &#x3bc;m. Although these stronger absorption bands in the mid-infrared region provide higher precision for temperature sensing and trace H&#x2082;O detection, they require more expensive laser sources, such as quantum cascade lasers (QCLs) [<xref ref-type="bibr" rid="B12">12</xref>, <xref ref-type="bibr" rid="B13">13</xref>] and interband cascade lasers (ICLs) [<xref ref-type="bibr" rid="B14">14</xref>, <xref ref-type="bibr" rid="B15">15</xref>]. In contrast, the near-infrared absorption bands around 1.4 &#x3bc;m and 1.8 &#x3bc;m can be accessed using fiber-optic diode lasers, offering advantages such as compact size, lower cost, high spectral quality, and room-temperature operation [<xref ref-type="bibr" rid="B16">16</xref>&#x2013;<xref ref-type="bibr" rid="B18">18</xref>], and the signals from these lasers can be directly acquired using either a photodetector or a quartz tuning fork detector, which has the merits of wide response range, low cost and tiny size [<xref ref-type="bibr" rid="B19">19</xref>&#x2013;<xref ref-type="bibr" rid="B21">21</xref>], making these lasers more attractive for temperature and H&#x2082;O concentration measurements in various combustion systems.</p>
<p>Most previous studies have focused on the 1.4 &#x3bc;m region for high-temperature sensing due to the availability of telecommunication-type lasers. For instance, Qu et al. [<xref ref-type="bibr" rid="B22">22</xref>] and Liu et al. [<xref ref-type="bibr" rid="B23">23</xref>] designed a temperature sensor capable of measuring temperatures using a distributed feedback (DFB) laser with a center wavelength of 1397.8 nm to detect two H&#x2082;O absorption lines at 7153.7484 cm&#x207b;<sup>1</sup> and 7154.3534 cm&#x207b;<sup>1</sup>. Similarly, Shao et al. [<xref ref-type="bibr" rid="B24">24</xref>] developed a gas sensor based on a 1.56 &#x3bc;m laser using wavelength modulation and two-line temperature retrieval to measure temperatures ranging from 200&#xb0;C to 1000&#xb0;C. However, these methods are prone to calculation errors due to uncertainties in the HITRAN or HITEMP databases. Increasing the number of H&#x2082;O absorption lines can enhance temperature measurement precision. Recent studies by Liu et al. [<xref ref-type="bibr" rid="B25">25</xref>] and Li et al. [<xref ref-type="bibr" rid="B26">26</xref>] employed three H&#x2082;O absorption lines at 7185.597 cm&#x207b;<sup>1</sup>, 7444.350 cm&#x207b;<sup>1</sup>, and 7444.37 cm&#x207b;<sup>1</sup>, respectively, to achieve high-precision temperature measurements in a flat-flame furnace and scramjet engine. Zhang et al. [<xref ref-type="bibr" rid="B27">27</xref>] used three DFB lasers operating near 1,343 nm, 1,392 nm, and 1,469 nm to accurately measure engine nozzle temperatures. In our previous work [<xref ref-type="bibr" rid="B28">28</xref>], five DFB lasers were employed near 1,392 nm, 1,393 nm, 1,339 nm, 1,343 nm, and 1,469 nm to improve temperature measurement precision in the expansion section of a scramjet engine.</p>
<p>Despite the stronger absorption at high temperatures in the 1.8 &#x3bc;m band compared to the 1.4 &#x3bc;m band [<xref ref-type="bibr" rid="B11">11</xref>], TDLAS measurements near 1.8 &#x3bc;m have been rarely reported. The 1.8 &#x3bc;m band holds promise for more sensitive H&#x2082;O detection and higher-precision temperature measurements. Therefore, in this study, we employed a single DFB laser operating near 1.85 &#x3bc;m as a TDLAS sensor to scan multiple H&#x2082;O absorption lines, with the lower-state energy levels ranging from 70 to 6,581 cm&#x207b;<sup>1</sup>. This sensor, featuring a high signal-to-noise ratio and strong line strength over a wide temperature range, enables high-precision temperature measurements across a broad temperature range.</p>
</sec>
<sec id="s2">
<title>2 Measurement basis of the sensor</title>
<sec id="s2-1">
<title>2.1 Selection of H<sub>2</sub>O absorption lines</title>
<p>The precision of laser-based sensors largely depends on the absorption strength of the selected target lines, which directly influences measurement accuracy. Therefore, selecting optimized absorption lines is critical. In this study, I will elaborate on the specific line selection criteria: 1) Target Molecule Selection: H&#x2082;O was chosen as the target molecule for TDLAS-based temperature measurement, with a designated temperature range of 500&#x2013;2500 K. This range not only covers the operational temperatures of our laboratory tube furnace for experimental validation but also extends to meet the requirements of future combustion flow field studies in aerospace engines. 2) Band Selection: The chosen spectral band lacks interference from major combustion products such as CO and CO&#x2082;, and features uniformly distributed lower-state energy levels, enabling measurements across a wide temperature span. 3) Laser Selection and Initial Line Database: Based on the above analysis of <xref ref-type="fig" rid="F1">Figure 1</xref> and selection criteria (1) and (2), a DFB laser operating near 1,850 nm (1.8&#x2013;2 &#x3bc;m) was selected, covering the 5,400&#x2013;5,409 cm&#x207b;<sup>1</sup> range. Absorption lines were initially chosen from HITEMP2010 with line strengths at 296 K meeting a threshold of S (T<sub>0</sub>)&#x2265;1.0 &#xd7; 10<sup>&#x2212;35</sup> cm<sup>-2</sup> <inline-formula id="inf1">
<mml:math id="m1">
<mml:mrow>
<mml:mo>&#x2219;</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> atm<sup>&#x2212;1</sup>. (4) Temperature-Based Line Screening: Within this initial database, line strengths were calculated at 100 K intervals, and line strengths meeting S(T)&#x2265;1.0 &#xd7; 10<sup>&#x2212;6</sup> cm<sup>&#x2212;2</sup> <inline-formula id="inf2">
<mml:math id="m2">
<mml:mrow>
<mml:mo>&#x2219;</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> atm<sup>&#x2212;1</sup> were selected to create temperature-specific databases from 500 to 2,500 K. (5) Signal-to-Noise Ratio (SNR) Optimization: For each temperature interval, lines with peak absorbance values yielding signal-to-noise ratios above 10 were further selected and consolidated to form an optimized absorption line database for temperature calculations over the 500&#x2013;2,500 K range. Based on the criteria, H&#x2082;O absorption lines between 5,400.5 cm&#x207b;<sup>1</sup> and 5,405.7 cm&#x207b;<sup>1</sup> were selected. Because the line selection incorporated the temperature dependence of line strengths, each line in the final combined database exhibits varying intensities across temperatures, enabling accurate measurements from low to high temperatures.</p>
<p>Based on the line selection criteria, the simulated H&#x2082;O absorption spectra at 1,600 K (in blue) are shown in <xref ref-type="fig" rid="F2">Figure 2A</xref>. Additionally, in combustion flow environments, such as aerospace engines and gas turbines, hydrocarbon-based fuels are commonly used, resulting in maximum potential interference concentrations of approximately 20% CO&#x2082;, 10% CO, and 10% CH&#x2084;. Hence, potential interference from carbon dioxide (CO&#x2082;), carbon monoxide (CO), and methane (CH&#x2084;) was considered, with their simulated absorption spectra displayed in black, red, and green, respectively. The H&#x2082;O absorption is significantly stronger than that of other gases, indicating that spectral interference from these gases can be ignored. <xref ref-type="fig" rid="F2">Figure 2B</xref> further illustrates the normalized line strength distribution of the selected absorption lines for temperatures ranging from 500 to 2500 K. The variation in line strengths for each absorption line at different temperatures is distinguished by the color gradient in the heatmap, clearly indicating the applicable temperature calculation range for each line and demonstrating how the line strengths and detectable absorption lines vary with temperature, enabling temperature measurement over a wide range.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>
<bold>(A)</bold> Simulated absorption of H<sub>2</sub>O(in blue curve) at the temperature of 1600 K, the concentration of 50%, the pressure of 0.1 atm, and the pathlength of 23 cm. The absorption interferences of 20% CO<sub>2</sub>(in black curve), 10% CO (in red curve) and 10% CH<sub>4</sub>(in green curve) are also displayed in this figure; <bold>(B)</bold> Distribution of the normalized line strength of the selected absorption lines in the temperature range of 500&#x2013;2500 K.</p>
</caption>
<graphic xlink:href="fphy-12-1488578-g002.tif"/>
</fig>
</sec>
<sec id="s2-2">
<title>2.2 Temperature retrieval method</title>
<p>The most common methods for retrieving temperature in TDLAS combustion diagnostics are two-line thermometry [<xref ref-type="bibr" rid="B29">29</xref>, <xref ref-type="bibr" rid="B30">30</xref>] and the Boltzmann Plot method [<xref ref-type="bibr" rid="B31">31</xref>&#x2013;<xref ref-type="bibr" rid="B33">33</xref>]. However, these approaches involve computing the integrated absorbance over a wide spectral range, which can be computationally intensive. In this study, we developed a broadband spectral fitting model based on the univariate search method [<xref ref-type="bibr" rid="B34">34</xref>, <xref ref-type="bibr" rid="B35">35</xref>] to determine temperature and H&#x2082;O concentration. This model fits multiple H&#x2082;O absorption lines across the absorption spectrum and continuous spectral bands, which has been reported in our previous work [<xref ref-type="bibr" rid="B36">36</xref>].</p>
<p>The flowchart for the broadband spectral fitting model is shown in <xref ref-type="fig" rid="F3">Figure 3</xref>. First, a measured broadband spectral absorbance (denoted as Abs_mea) is recorded, and a model-based spectral absorbance (denoted as Abs_model), using Voigt profile, is simulated based on input fitting parameters such as H&#x2082;O line parameters from HITEMP2010 and experimental conditions (e.g., pressure, optical path length). A nonlinear univariate method (using the <italic>fminbnd</italic> function in MATLAB) is then employed to search for the optimal temperature (denoted as T<sub>opt</sub>) under an initial concentration (denoted as X&#x2080;) and initial temperature (denoted as T<sub>initial</sub>). A linear fitting between Abs_mea and Abs_model is performed to obtain the slope (<inline-formula id="inf3">
<mml:math id="m3">
<mml:mrow>
<mml:mi mathvariant="bold-italic">f</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>) and intercept (<inline-formula id="inf4">
<mml:math id="m4">
<mml:mrow>
<mml:mi mathvariant="bold-italic">b</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>) of the linear fit according to the relationship of <inline-formula id="inf5">
<mml:math id="m5">
<mml:mrow>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>mea</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> &#x3d; <inline-formula id="inf6">
<mml:math id="m6">
<mml:mrow>
<mml:mi mathvariant="bold-italic">f</mml:mi>
<mml:mo>&#x2219;</mml:mo>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>model</mml:mtext>
<mml:mo>&#x2b;</mml:mo>
<mml:mi mathvariant="bold-italic">b</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>. The concentration is then updated as <inline-formula id="inf7">
<mml:math id="m7">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">X</mml:mi>
<mml:mtext>opt</mml:mtext>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> &#x3d; <inline-formula id="inf8">
<mml:math id="m8">
<mml:mrow>
<mml:msub>
<mml:mi>X</mml:mi>
<mml:mn>0</mml:mn>
</mml:msub>
<mml:mo>&#x2219;</mml:mo>
<mml:mi mathvariant="bold-italic">f</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>. After <italic>jth</italic> iterations, the second norm of the fitting residuals (<italic>r</italic>
<sub>
<italic>normr</italic>
</sub>) is minimized and the convergence condition (&#x7c; <inline-formula id="inf9">
<mml:math id="m9">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">T</mml:mi>
<mml:mrow>
<mml:mtext mathvariant="bold">opt</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi mathvariant="bold">j</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:mn mathvariant="bold">1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>-<inline-formula id="inf10">
<mml:math id="m10">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">T</mml:mi>
<mml:mrow>
<mml:mtext mathvariant="bold">opt</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi mathvariant="bold">j</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> &#x7c;&#x3c;1&#x3001;&#x7c; <inline-formula id="inf11">
<mml:math id="m11">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">X</mml:mi>
<mml:mrow>
<mml:mtext mathvariant="bold">opt</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi mathvariant="bold">j</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:mn mathvariant="bold">1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>-<inline-formula id="inf12">
<mml:math id="m12">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">X</mml:mi>
<mml:mrow>
<mml:mtext mathvariant="bold">opt</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi mathvariant="bold">j</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> &#x7c;&#x3c;1 &#xd7; 10<sup>&#x2212;3</sup>) is satisfied, yielding the optimal temperature and concentration. Here, the <italic>r</italic>
<sub>
<italic>normr</italic>
</sub> value represents the second norm of the spectral fitting residuals, which is the square root of the sum of squared residuals. The <italic>r</italic>
<sub>
<italic>normr</italic>
</sub> is shown in <xref ref-type="disp-formula" rid="e1">Equation 1</xref>:<disp-formula id="e1">
<mml:math id="m13">
<mml:mrow>
<mml:msub>
<mml:mi>r</mml:mi>
<mml:mrow>
<mml:mi>n</mml:mi>
<mml:mi>o</mml:mi>
<mml:mi>r</mml:mi>
<mml:mi>m</mml:mi>
<mml:mi>r</mml:mi>
<mml:mo>&#x3d;</mml:mo>
</mml:mrow>
</mml:msub>
<mml:mtext>&#x2009;</mml:mtext>
<mml:msqrt>
<mml:mrow>
<mml:mstyle displaystyle="true">
<mml:munderover>
<mml:mo>&#x2211;</mml:mo>
<mml:mrow>
<mml:mi mathvariant="bold-italic">j</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn mathvariant="bold">1</mml:mn>
</mml:mrow>
<mml:mi mathvariant="bold-italic">N</mml:mi>
</mml:munderover>
</mml:mstyle>
<mml:msup>
<mml:mrow>
<mml:mfenced open="[" close="]" separators="|">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>mea</mml:mtext>
</mml:mrow>
<mml:mi mathvariant="bold-italic">j</mml:mi>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>mea</mml:mtext>
</mml:mrow>
<mml:mrow>
<mml:mi mathvariant="bold-italic">j</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi mathvariant="bold-italic">f</mml:mi>
<mml:mi mathvariant="bold-italic">i</mml:mi>
<mml:mi mathvariant="bold-italic">t</mml:mi>
<mml:mi mathvariant="bold-italic">t</mml:mi>
<mml:mi mathvariant="bold-italic">e</mml:mi>
<mml:mi mathvariant="bold-italic">d</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mn mathvariant="bold">2</mml:mn>
</mml:msup>
</mml:mrow>
</mml:msqrt>
</mml:mrow>
</mml:math>
<label>(1)</label>
</disp-formula>Where <inline-formula id="inf13">
<mml:math id="m14">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>mea</mml:mtext>
</mml:mrow>
<mml:mi>j</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> is Abs_mea during the <italic>j</italic>th iteration, <inline-formula id="inf14">
<mml:math id="m15">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>mea</mml:mtext>
</mml:mrow>
<mml:mrow>
<mml:mi>j</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>f</mml:mi>
<mml:mi>i</mml:mi>
<mml:mi>t</mml:mi>
<mml:mi>t</mml:mi>
<mml:mi>e</mml:mi>
<mml:mi>d</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> is the fitting result <inline-formula id="inf15">
<mml:math id="m16">
<mml:mrow>
<mml:mtext>according&#x2009;to&#x2009;Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>mea</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> &#x3d; <inline-formula id="inf16">
<mml:math id="m17">
<mml:mrow>
<mml:mi mathvariant="bold-italic">f</mml:mi>
<mml:mo>&#x2219;</mml:mo>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>model</mml:mtext>
<mml:mo>&#x2b;</mml:mo>
<mml:mi mathvariant="bold-italic">b</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>.</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>Flowchart of temperature retrieval method.</p>
</caption>
<graphic xlink:href="fphy-12-1488578-g003.tif"/>
</fig>
<p>
<inline-formula id="inf17">
<mml:math id="m18">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">T</mml:mi>
<mml:mtext>opt</mml:mtext>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> and <inline-formula id="inf18">
<mml:math id="m19">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">X</mml:mi>
<mml:mtext>opt</mml:mtext>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> are respectively the optimal temperature and concentration, then <italic>r</italic>
<sub>
<italic>normr</italic>
</sub> can be further expressed by <xref ref-type="disp-formula" rid="e2">Equation 2</xref>:<disp-formula id="e2">
<mml:math id="m20">
<mml:mrow>
<mml:mtable columnalign="center">
<mml:mtr>
<mml:mtd>
<mml:mrow>
<mml:mi mathvariant="bold-italic">arg</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi mathvariant="bold-italic">min</mml:mi>
</mml:mrow>
</mml:mtd>
</mml:mtr>
<mml:mtr>
<mml:mtd>
<mml:mi mathvariant="bold-italic">T</mml:mi>
</mml:mtd>
</mml:mtr>
</mml:mtable>
<mml:msqrt>
<mml:mrow>
<mml:mstyle displaystyle="true">
<mml:munderover>
<mml:mo>&#x2211;</mml:mo>
<mml:mrow>
<mml:mi mathvariant="bold-italic">j</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn mathvariant="bold">1</mml:mn>
</mml:mrow>
<mml:mi mathvariant="bold-italic">N</mml:mi>
</mml:munderover>
</mml:mstyle>
<mml:msup>
<mml:mrow>
<mml:mfenced open="[" close="]" separators="|">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>mea</mml:mtext>
</mml:mrow>
<mml:mi mathvariant="bold-italic">j</mml:mi>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:mi mathvariant="bold-italic">f</mml:mi>
<mml:mo>&#x2219;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>model</mml:mtext>
</mml:mrow>
<mml:mrow>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi mathvariant="bold-italic">j</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">T</mml:mi>
<mml:mrow>
<mml:mi mathvariant="bold-italic">o</mml:mi>
<mml:mi mathvariant="bold-italic">p</mml:mi>
<mml:mi mathvariant="bold-italic">t</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi mathvariant="bold-italic">X</mml:mi>
<mml:mrow>
<mml:mi mathvariant="bold-italic">o</mml:mi>
<mml:mi mathvariant="bold-italic">p</mml:mi>
<mml:mi mathvariant="bold-italic">t</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mi mathvariant="bold-italic">b</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mn mathvariant="bold">2</mml:mn>
</mml:msup>
</mml:mrow>
</mml:msqrt>
</mml:mrow>
</mml:math>
<label>(2)</label>
</disp-formula>Where <inline-formula id="inf19">
<mml:math id="m21">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>model</mml:mtext>
</mml:mrow>
<mml:mrow>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi mathvariant="bold-italic">j</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> is <inline-formula id="inf20">
<mml:math id="m22">
<mml:mrow>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>model</mml:mtext>
</mml:mrow>
</mml:math>
</inline-formula> during the <italic>j</italic>th iteration, <inline-formula id="inf21">
<mml:math id="m23">
<mml:mrow>
<mml:mstyle displaystyle="true">
<mml:munderover>
<mml:mo>&#x2211;</mml:mo>
<mml:mrow>
<mml:mi mathvariant="bold-italic">j</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn mathvariant="bold">1</mml:mn>
</mml:mrow>
<mml:mi mathvariant="bold-italic">N</mml:mi>
</mml:munderover>
</mml:mstyle>
<mml:msup>
<mml:mrow>
<mml:mfenced open="[" close="]" separators="|">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>mea</mml:mtext>
</mml:mrow>
<mml:mi mathvariant="bold-italic">j</mml:mi>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:mi mathvariant="bold-italic">f</mml:mi>
<mml:mo>&#x2219;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mtext>Abs</mml:mtext>
<mml:mo>_</mml:mo>
<mml:mtext>model</mml:mtext>
</mml:mrow>
<mml:mrow>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi mathvariant="bold-italic">j</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">T</mml:mi>
<mml:mrow>
<mml:mi mathvariant="bold-italic">o</mml:mi>
<mml:mi mathvariant="bold-italic">p</mml:mi>
<mml:mi mathvariant="bold-italic">t</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi mathvariant="bold-italic">X</mml:mi>
<mml:mrow>
<mml:mi mathvariant="bold-italic">o</mml:mi>
<mml:mi mathvariant="bold-italic">p</mml:mi>
<mml:mi mathvariant="bold-italic">t</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mi mathvariant="bold-italic">b</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mn mathvariant="bold">2</mml:mn>
</mml:msup>
</mml:mrow>
</mml:math>
</inline-formula> represents the objective function dependent on temperature <inline-formula id="inf22">
<mml:math id="m24">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">T</mml:mi>
<mml:mrow>
<mml:mi mathvariant="bold-italic">o</mml:mi>
<mml:mi mathvariant="bold-italic">p</mml:mi>
<mml:mi mathvariant="bold-italic">t</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>. The term <inline-formula id="inf23">
<mml:math id="m25">
<mml:mrow>
<mml:mtable columnalign="center">
<mml:mtr>
<mml:mtd>
<mml:mrow>
<mml:mi mathvariant="bold-italic">arg</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi mathvariant="bold-italic">min</mml:mi>
</mml:mrow>
</mml:mtd>
</mml:mtr>
<mml:mtr>
<mml:mtd>
<mml:mi mathvariant="bold-italic">T</mml:mi>
</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:mrow>
</mml:math>
</inline-formula> indicates the value of <inline-formula id="inf24">
<mml:math id="m26">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">T</mml:mi>
<mml:mrow>
<mml:mi mathvariant="bold-italic">o</mml:mi>
<mml:mi mathvariant="bold-italic">p</mml:mi>
<mml:mi mathvariant="bold-italic">t</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> that minimizes the objective function. Specifically, <inline-formula id="inf25">
<mml:math id="m27">
<mml:mrow>
<mml:mi mathvariant="bold-italic">arg</mml:mi>
<mml:mtext>&#x2009;</mml:mtext>
<mml:mi mathvariant="bold-italic">min</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> is an operator that finds the variable value at which the function reaches its minimum, and <inline-formula id="inf26">
<mml:math id="m28">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">T</mml:mi>
<mml:mrow>
<mml:mi mathvariant="bold-italic">o</mml:mi>
<mml:mi mathvariant="bold-italic">p</mml:mi>
<mml:mi mathvariant="bold-italic">t</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> refers to this variable in the context.</p>
<p>The typical example illustrating this method is shown in <xref ref-type="fig" rid="F4">Figures 4</xref>, <xref ref-type="fig" rid="F5">5</xref>. To fit the actual experimental conditions, an H&#x2082;O absorbance spectrum was simulated under the conditions of <italic>Pressure</italic> &#x3d; 1 atm, <italic>X</italic>
<sub>
<italic>H2O</italic>
</sub> &#x3d; 0.06, <italic>L</italic> &#x3d; 23 cm and <italic>T</italic> &#x3d; 1200 K. Gaussian noise with an amplitude of &#xb1;0.005 and a 20% error in H&#x2082;O absorption line parameters were added in the H&#x2082;O absorbance spectrum regarded as measured spectrum. Then it was input into the broadband spectral fitting model to obtain the trends for temperature, concentration, and <italic>r</italic>
<sub>
<italic>normr</italic>
</sub> during each iteration, as shown in <xref ref-type="fig" rid="F4">Figure 4</xref>.</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>
<bold>(A)</bold> Temperature and concentration of each iteration; <bold>(B)</bold> <italic>rnormr</italic> of each iteration.</p>
</caption>
<graphic xlink:href="fphy-12-1488578-g004.tif"/>
</fig>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>
<bold>(A)</bold> Absorption spectra (Abs_mea in blue curve&#x26;Abs_model in red curve) for the first iteration; <bold>(B)</bold> Spectral linear fitting result for the first iteration; <bold>(C)</bold> Absorption spectra (Abs_mea in blue curve&#x26;Abs_model in red curve) for the 11th iteration; <bold>(D)</bold> Spectral linear fitting result for the 11th iteration.</p>
</caption>
<graphic xlink:href="fphy-12-1488578-g005.tif"/>
</fig>
<p>In the first iteration (blue curve in <xref ref-type="fig" rid="F4">Figure 4A</xref>), the optimal temperature differs significantly from the true value of 1200 K, and the corresponding <italic>r</italic>
<sub>
<italic>normr</italic>
</sub> (green curve in <xref ref-type="fig" rid="F4">Figure 4B</xref>) is also at its maximum. <xref ref-type="fig" rid="F5">Figure 5A</xref> shows the Abs_mea (blue curve) and Abs_model (red curve) for the first iteration, where a poor fit between the measured and model-based spectrum is evident. Similarly, <xref ref-type="fig" rid="F5">Figure 5B</xref> presents the linear fit of the spectral data for the first iteration, demonstrating a clear deviation between the measured data and the linear fit. These results indicate that the temperature and the concentration are not optimal in the first iteration. After several iterations, the temperature and concentration in the 11th iteration converge closely to the true values of 1200 K and 0.06, respectively. Furthermore, the <italic>r</italic>
<sub>
<italic>normr</italic>
</sub> is minimized. The spectra (<xref ref-type="fig" rid="F5">Figure 5C</xref>) and the linear fit of the spectral data (<xref ref-type="fig" rid="F5">Figure 5D</xref>) confirm a much-improved fit, indicating that the optimal temperature and concentration have been successfully determined.</p>
</sec>
</sec>
<sec id="s3">
<title>3 Experimental setup and discussions</title>
<sec id="s3-1">
<title>3.1 Experimental setup</title>
<p>A DFB laser (Nanoplus, S/N: 2899/03-02) operating near 1850.5 nm was selected as the laser source. A commercial laser controller (LDC501, Stanford Research Systems) was used to regulate the laser operating temperature, and a sawtooth wave signal generated by a commercial function generator (SDG2082X, SIGLENT) was applied to continuously scan the absorption lines of H&#x2082;O. The temperature measurement performance of the sensor was evaluated using a commercial tube furnace platform (GSL-1800X-III-&#x20b5;50). The laser beam was split into two parts using a fiber splitter, as shown in <xref ref-type="fig" rid="F6">Figure 6</xref>. Fifty percent of the beam was collimated by a fiber collimator, transmitted through the temperature test region in the furnace, and then detected by a photodetector (Thorlabs PDA10D-E-C). The other half of the beam passed through a quartz Fabry-P&#xe9;rot etalon for frequency calibration and was detected by another photodetector. The generated photocurrents were converted into voltage signals using a custom-made transimpedance amplifier. The signals were then digitized using a 16-bit data acquisition card (NI PXIe-5172). To ensure a stable temperature region within the furnace, the sapphire tube was inserted into both ends of the furnace tube. Additionally, a pair of structures incorporating internal gas pipes was designed to mount the collimator. The structures allowed for purging the internal air gap with high-purity nitrogen (99.99%) to eliminate absorption interference from residual H&#x2082;O.</p>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>Overall scheme of sensor temperature measurement.</p>
</caption>
<graphic xlink:href="fphy-12-1488578-g006.tif"/>
</fig>
<p>Seven equally spaced temperatures ranging from 600 K to 1800 K were set within the furnace&#x2019;s maximum tolerance temperature of 2000 K. After reaching the preset temperatures, pure water vapor (100% purity) at three different pressures (P1&#x2013;P3: 3.5&#x2013;6.5 KPa) was introduced into the furnace, with the pressures monitored using a manometer (MKS628). For each temperature and pressure, 500 raw spectral signals were recorded once the pressure stabilized. Additional tests were conducted at higher pressures (P4&#x2013;P6: 10&#x2013;103 KPa) using a mixture of pure water vapor and high-purity nitrogen, with 500 spectral signals captured for each set condition. Non-absorbing regions of the raw spectral signals were fitted using a third-order polynomial to extract the H&#x2082;O absorbance. <xref ref-type="fig" rid="F7">Figure 7A</xref> displays the measured raw data and the corresponding extracted H&#x2082;O absorbance. A spectral fitting result using the broadband spectral fitting model is shown in <xref ref-type="fig" rid="F7">Figure 7B</xref>, demonstrating close agreement between the fitted and measured H&#x2082;O absorbance. But there is still a deviation between &#x2212;0.02 and 0.02 as shown in <xref ref-type="fig" rid="F7">Figure 7C</xref>. The reason of this deviation can be concluded as follows. DFB laser&#x2019;s wide scanning range combined with spectral broadening and weak absorption lines, introduces errors in selecting non-absorbing regions, resulting in irregular baseline fluctuations that subsequently cause baseline shifts during spectral fitting, and this effect will be discussed in <xref ref-type="sec" rid="s3-2">Section 3.2</xref>. Moreover, the spectral line parameters in HITEMP2010 have errors ranging from 5% to 20%, or even higher, and unavoidable spectral noise also contributes to the deviation. Calibration of spectral parameters and an increase in the SNR can reduce these errors, but due to the large number of lines involved, this process is still ongoing. However, as illustrated in <xref ref-type="fig" rid="F7">Figure 7D</xref>, even with a deviation between &#x2212;0.02 and 0.02, <italic>r</italic>
<sub>
<italic>normr</italic>
</sub> converges to a minimum after 13 iterations, allowing optimal temperature and concentration values to be obtained.</p>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption>
<p>Processing of experimental measured data: <bold>(A)</bold> Experimental measured H2O absorption signal and extracted spectrum at T &#x3d; 1000 K&#x3001;X<sub>H2O</sub> &#x3d; 0.0578&#x3001;P<sub>H2O-N2</sub> &#x3d; 99.11KPa; <bold>(B)</bold> Spectral fitting result; <bold>(C)</bold> Spectral fitting residual between Abs_mea and Abs_model; <bold>(D)</bold> rnormr of each iteration.</p>
</caption>
<graphic xlink:href="fphy-12-1488578-g007.tif"/>
</fig>
</sec>
<sec id="s3-2">
<title>3.2 Results and discussions</title>
<sec id="s3-2-1">
<title>3.2.1 Analysis of experimental results</title>
<p>To further validate the sensor&#x2019;s performance, temperature measurements were carried out in the furnace across a range of 600&#x2013;1800 K and pressures from 3.5 to 103 KPa. An example of the extracted H&#x2082;O absorption spectrum at temperatures between 600 K and 1800 K (at P3) is shown in <xref ref-type="fig" rid="F8">Figure 8A</xref>. The absorption intensity varies across this temperature range, corresponding to the trend in line strength with temperature, as depicted in <xref ref-type="fig" rid="F2">Figure 2B</xref>.</p>
<fig id="F8" position="float">
<label>FIGURE 8</label>
<caption>
<p>
<bold>(A)</bold> Experimental measured H2O absorption spectrum at 600&#x2013;1800K (@P3); <bold>(B)</bold> Error bar chart (top panel) and relative error (bottom panel) of experimental data at 600&#x2013;1800K and 3.5&#x2013;103 KPa.</p>
</caption>
<graphic xlink:href="fphy-12-1488578-g008.tif"/>
</fig>
<p>The extracted H&#x2082;O absorption spectra were processed using the broadband spectral fitting model to determine the measured temperatures, with error bars and relative errors at different temperatures and pressures shown in <xref ref-type="fig" rid="F8">Figure 8B</xref>. At a constant temperature, the standard deviations at different pressures remain relatively consistent and close to the average values. The relative error fluctuates within 2% for pressures ranging from 3.5 to 6.5 KPa, indicating stable temperature measurement performance. At higher pressures (10&#x2013;103 KPa), the maximum standard deviation is 34.6 K (at 1800 K, 102.9 KPa), and the relative error ranges from &#x2212;1% to 3.5%. The relative error increases significantly at temperatures above 1000 K and pressures exceeding 50 KPa. The wide wavelength scanning range of the laser, combined with weak spectral lines and spectral broadening, complicates the accurate fitting of non-absorbing regions using polynomial methods, leading to errors in absorbance extraction and temperature measurement.</p>
</sec>
<sec id="s3-2-2">
<title>3.2.2 Simulation analysis</title>
<p>To evaluate the impact of absorbance extraction errors on temperature accuracy, the absorption-free laser intensity (<italic>I&#x2080;</italic>) was determined by extracted baselines at different temperatures and pressures in <xref ref-type="sec" rid="s3-2-1">Section 3.2.1</xref>. H&#x2082;O absorption spectra (denoted as <inline-formula id="inf27">
<mml:math id="m29">
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>&#x3c5;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula>) were simulated at seven equal-interval temperatures between 600 and 1800 K and six different pressures (3.5&#x2013;150 KPa), with Gaussian noise (amplitude &#xb1;0.005) and a 20% error in the H&#x2082;O line parameters added to the simulated spectra. The transmitted intensity (<inline-formula id="inf28">
<mml:math id="m30">
<mml:mrow>
<mml:msub>
<mml:mi>I</mml:mi>
<mml:mi>t</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>) is calculated by <xref ref-type="disp-formula" rid="e3">Equation 3</xref>.<disp-formula id="e3">
<mml:math id="m31">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="bold-italic">I</mml:mi>
<mml:mi mathvariant="bold-italic">t</mml:mi>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:msub>
<mml:mi mathvariant="bold-italic">I</mml:mi>
<mml:mn mathvariant="bold">0</mml:mn>
</mml:msub>
<mml:mo>&#xb7;</mml:mo>
<mml:mi mathvariant="bold-italic">exp</mml:mi>
<mml:mrow>
<mml:mfenced open="[" close="]" separators="|">
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi mathvariant="bold-italic">&#x3b1;</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi mathvariant="bold-italic">&#x3c5;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x2b;</mml:mo>
<mml:mi mathvariant="bold-italic">B</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi mathvariant="bold-italic">&#x3c5;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:math>
<label>(3)</label>
</disp-formula>where B(&#x3c5;) represents the added Gaussian noise.</p>
<p>
<xref ref-type="fig" rid="F9">Figure 9A</xref> shows an example of the simulated transmitted intensity at 1000 K and 150 kPa, along with the extracted spectrum. The error bars and relative errors are plotted in <xref ref-type="fig" rid="F9">Figure 9B</xref>, showing a maximum standard deviation of 60.1 K (at 1800 K, 150 KPa). The relative error fluctuates within &#xb1;1% at pressures between 3.5 KPa and 10 kPa, but rises to 3% at pressures between 50 and 150 kPa, which is largely consistent with the experimental results. This indicates that incorrect selection of non-absorbing regions can reduce accuracy of absorbance extraction and temperature measurements.</p>
<fig id="F9" position="float">
<label>FIGURE 9</label>
<caption>
<p>
<bold>(A)</bold> Simulated <inline-formula id="inf29">
<mml:math id="m32">
<mml:mrow>
<mml:msub>
<mml:mi mathvariant="normal">I</mml:mi>
<mml:mi mathvariant="normal">t</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> (@1000K, 150 KPa) and the extracted spectra; <bold>(B)</bold> Error bar chart (top panel) and relative error (bottom panel) of simulation data at 600&#x2013;1800K and 3.5&#x2013;150 KPa.</p>
</caption>
<graphic xlink:href="fphy-12-1488578-g009.tif"/>
</fig>
<p>To further verify the impact of these factors and evaluate the sensor&#x2019;s performance at temperatures above 1800 K, H&#x2082;O absorption spectra were simulated for ten equal-interval temperatures between 500 and 2500 K at six different pressures (3.5&#x2013;150 KPa). Gaussian noise (amplitude &#xb1;0.005) and a 20% error in spectral parameters were added to the H&#x2082;O absorbance, where the process assumes accurate absorbance extraction. <xref ref-type="fig" rid="F10">Figure 10A</xref> shows an example of the simulated spectra, while <xref ref-type="fig" rid="F10">Figure 10B</xref> presents the corresponding error bars and relative errors. The maximum standard deviation of temperature is 105.14 K (at 2500 K, 150 KPa), and the relative error fluctuates between 1.5% and 2%, which is lower than the error shown in <xref ref-type="fig" rid="F9">Figure 9B</xref> for the same conditions. These results demonstrate that the sensor performs effectively over the 500&#x2013;2500 K range, and that improper selection of non-absorbing regions directly reduces the accuracy of absorbance extraction and temperature measurements, which will be addressed in future work by developing a broadband baseline fitting model to enhance temperature measurement accuracy.</p>
<fig id="F10" position="float">
<label>FIGURE 10</label>
<caption>
<p>
<bold>(A)</bold> Simulated absorption spectrum (@500&#x2013;2500K, 150 KPa); <bold>(B)</bold> Error bar chart (top panel) and relative error (bottom panel) of simulation data at 500&#x2013;2500K and 3.5&#x2013;150 KPa.</p>
</caption>
<graphic xlink:href="fphy-12-1488578-g010.tif"/>
</fig>
</sec>
</sec>
</sec>
<sec sec-type="conclusion" id="s4">
<title>4 Conclusion</title>
<p>In this study, we developed a TDLAS sensor operating near 1850.5 nm to scan multiple H&#x2082;O absorption lines within the 5,400&#x2013;5,406 cm&#x207b;<sup>1</sup> range for wide-range temperature measurement. The sensor&#x2019;s performance was experimentally validated in a tube furnace at temperatures ranging from 600 to 1800 K and pressures from 3.5 to 103 kPa, where the relative error of temperature is within 3.5%. Additionally, numerical simulations demonstrated that the sensor is capable of accurate temperature measurements from 500 to 2500 K. The accuracy of the extracted absorbance plays a crucial role in the overall measurement precision, and factors such as the wide scanning range, weak spectral lines, and spectral line broadening can influence the selection of non-absorbing regions and the quality of absorbance extraction. Future work will focus on the development of a broadband baseline fitting model to mitigate the effects of spectral interference and further improve temperature measurement accuracy. Overall, the sensor exhibits high measurement accuracy over a wide temperature range and is well-suited for applications in combustion environments with large temperature gradients, such as the isolation and expansion sections of scramjet engines. Additionally, this sensor provides a promising solution for multiline temperature distribution measurements in future diagnostics.</p>
</sec>
</body>
<back>
<sec sec-type="data-availability" id="s5">
<title>Data availability statement</title>
<p>The original contributions presented in the study are included in the article/supplementary material, further inquiries can be directed to the corresponding author.</p>
</sec>
<sec sec-type="author-contributions" id="s6">
<title>Author contributions</title>
<p>SA: Conceptualization, Data curation, Formal Analysis, Investigation, Methodology, Software, Validation, Visualization, Writing&#x2013;original draft, Writing&#x2013;review and editing. ZX: Formal Analysis, Funding acquisition, Methodology, Project administration, Supervision, Writing&#x2013;review and editing. AH: Conceptualization, Investigation, Writing&#x2013;review and editing. HD: Validation, Visualization, Writing&#x2013;review and editing. RN: Resources, Writing&#x2013;review and editing. RK: Funding acquisition, Project administration, Writing&#x2013;review and editing.</p>
</sec>
<sec sec-type="funding-information" id="s7">
<title>Funding</title>
<p>The author(s) declare that financial support was received for the research, authorship, and/or publication of this article. This research was funded by National Key R&#x26;D Program of China (Grant No. 2023YFF0716400), National Science and Technology Major Project (Grant No. J2019-V-0005-0096) and Foundational Military Research Institute Stability Support Project.</p>
</sec>
<sec sec-type="COI-statement" id="s8">
<title>Conflict of interest</title>
<p>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.</p>
</sec>
<sec sec-type="disclaimer" id="s9">
<title>Publisher&#x2019;s note</title>
<p>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.</p>
</sec>
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