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  <front>
    <journal-meta />
    <article-meta>
      <title-group>
        <article-title>Optical Diagnostics of Temperature and Structural Parameters of an Axisymmetric Flame*</article-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author">
          <string-name>V. Arbuzov</string-name>
          <email>arbuzov@itp.nsc.ru</email>
          <email>arbuzov@math.nsc.ru</email>
          <xref ref-type="aff" rid="aff2">2</xref>
        </contrib>
        <contrib contrib-type="author">
          <string-name>E. Arbuzov</string-name>
        </contrib>
        <contrib contrib-type="author">
          <string-name>Y. Dubnishchev</string-name>
        </contrib>
        <contrib contrib-type="author">
          <string-name>O. Zolotukhina</string-name>
        </contrib>
        <contrib contrib-type="author">
          <string-name>V. Lukashov</string-name>
          <email>luka@itp.nsc.ru</email>
        </contrib>
        <aff id="aff0">
          <label>0</label>
          <institution>Kutateladze Institute of Thermophysics, Siberian Branch of the Russian Academy of Sciences</institution>
          ,
          <addr-line>Novosibirsk 630090</addr-line>
          ,
          <country country="RU">Russia</country>
        </aff>
        <aff id="aff1">
          <label>1</label>
          <institution>Novosibirsk State Technical University</institution>
          ,
          <addr-line>Novosibirsk 630073</addr-line>
          ,
          <country country="RU">Russia</country>
        </aff>
        <aff id="aff2">
          <label>2</label>
          <institution>Sobolev Institute of Mathematics, Siberian Branch of the Russian Academy of Sciences</institution>
          ,
          <addr-line>Novosibirsk 630090</addr-line>
          ,
          <country country="RU">Russia</country>
        </aff>
      </contrib-group>
      <abstract>
        <p>In this paper a method for restoring the parameters of multicomponent media for optical diagnostics of jet using the example of a hydrogen-air flame study is considered. Hilbert visualization and numerical modeling of phase perturbations induced by the studied medium in the probing light field are used. The study of the burning jet was carried out using the methods of Hilbert optics and Abel transformation in the model of axial symmetry of the torch. A software package has been developed that implements a direct solution to the problem: calculation of the spatial optical phase structure of the flame and its corresponding hilbertograms based on the temperature and molar concentrations of the combustion products of the mixture. The reliability of the obtained results is confirmed by comparing the Hilbert structures obtained in the experiment and the reconstructed optical density field of the phase using the Abel transform. The results of the comparison are used as a quality criterion for modeling the phase structure and temperature field in the study of the combustion process. The developed method can be used to solve the inverse problem of restoring the temperature field from the Hilbert image of the phase structure of a hydrogen-air flame in the approximation of axial symmetry. The research is motivated by the scientific and practical significance of the problem, which consists in finding methods for controlling the structural and thermodynamic parameters of reacting jets and flames.</p>
      </abstract>
      <kwd-group>
        <kwd>Optical Diagnostics of Flames</kwd>
        <kwd>Hilbert Optics</kwd>
        <kwd>Optical Information Technology</kwd>
      </kwd-group>
    </article-meta>
  </front>
  <body>
    <sec id="sec-1">
      <title>-</title>
      <p>1</p>
    </sec>
    <sec id="sec-2">
      <title>Introduction</title>
      <p>The optical methods are the most important in unperturbing diagnostics of reacting
jets and flames. They allow one to obtain adequate information about the
thermodynamic and structural parameters of the medium under study without disturbing its
state.</p>
      <p>In [1], a method for estimating the temperature distribution in an asymmetric flame
using high-contrast stereoscopic photography is described. Spectral reconstruction of
temperature fields using color ratio pyrometry and interferometric tomography is
reported [2]. An example adapted to the problems of flame research is optical
diagnostics based on the methods of Hilbert optics and interferometry in combination with
pixel-by-pixel processing of the dynamic structure of visualized phase structures
induced by temperature fields [3]. However, the problem is to diagnose the spatial
optical phase structure of the flame.</p>
      <p>The aim of this work is to adapt the methods of Hilbert optics to the study of
axisymmetric hydrogen-air flame with the reconstruction of the spatial phase and
temperature structure. The research is motivated by the scientific and practical
significance of the problem, which consists in finding methods for controlling the structural
and thermodynamic parameters of the torch [4].
2</p>
    </sec>
    <sec id="sec-3">
      <title>Research method</title>
      <p>The complex of optical diagnostics is based on the IAB–463M device [5] with
modified modules of Hilbert filtration, interferometry, source of probing field, registration
and processing of the optical signal [6]. The probing field is formed by the collimator
system from a slotted source. The investigated hydrogen-air flame is localized in the
vicinity of the front Fourier plane of the lens, which serves as an analyzer of phase
disturbances induced in the probing field by this flame. Visualization of the Fourier
spectrum of phase perturbations is performed by a Hilbert filter placed in the
frequency plane of the Fourier lens. Next, the inverse Fourier transform of the
Hilbertconjugate Fourier spectrum of phase perturbations is performed. The visualized phase
disturbances are registered by the camera's photo matrix. The registered images are
analyzed by a computer connected to the video camera.</p>
      <p>
        In the frequency plane for the Fourier spectrum of the phase optical density of the
light field perturbed by the medium under study (flame), we have immediately after
the filter:
 (  ,   ) (  ,   ) =  (  ,   )cosφ+ ̂ (  ,   )sinφ,
(
        <xref ref-type="bibr" rid="ref1">1</xref>
        )
where  (  ,   ) is the coherent transfer function of the filter performing the
onedimensional Foucault–Hilbert transform,
      </p>
      <p>Optical Diagnostics of Temperature and Structural Parameters of an Axisymmetric Flame 3
 (  ,   ) = cosφ −  sinφ sgn  .</p>
      <p>
        The phase shift φ is a function of the wavelength λ of the probing light field,
φ = φ(λ). At a wavelength satisfying the condition φ(λ0) =  /2, the Hilbert image
of the Fourier spectrum of phase perturbations:
 ̂ (  ,   ) = − sgn   (  ,   ).
(
        <xref ref-type="bibr" rid="ref2">2</xref>
        )
The inverse Fourier transform of the Hilbert-conjugate Fourier spectrum of phase
perturbations (
        <xref ref-type="bibr" rid="ref1">1</xref>
        ) is performed below:
      </p>
      <p>(  ,   )cosφ+ ̂ (  ,   )sinφ ↔  ( ,  )cosφ+ ̂ ( ,  )sinφ.</p>
      <p>
        The intensity of the analytical signal (
        <xref ref-type="bibr" rid="ref3">3</xref>
        ) is recorded by a video camera:
 ( ,  ) = ρ{| ( ,  )|2cos2φ+| ̂ ( ,  )|2sin2φ},
where ρ is a coefficient that takes into account the sensitivity of the photo matrix.
      </p>
      <p>The Hilbert transform has the properties of redistributing energy from the region of
low spatial frequencies to the high-frequency region. Extremes and gradients of the
phase optical density of the medium under study are transformed into visualized
Hilbert-bands structures. The spatial distribution of Hilbert bands provides information
about phase optical density perturbations induced by the temperature field.</p>
      <p>
        An example of the phase structure of a hydrogen-air flame is shown in Fig. 1.a.
The phase structure was visualized using Hilbert optics methods. The experiments
were carried out at atmospheric pressure and initial room temperature.
(
        <xref ref-type="bibr" rid="ref3">3</xref>
        )
(
        <xref ref-type="bibr" rid="ref4">4</xref>
        )
a
b
      </p>
      <p>The burner is shown schematically in Fig. 1.b. It consists of two coaxially and
vertically positioned quartz tubes (dimensions and relative positions are shown in the
figure). Air is supplied through an inner tube. The fuel mixture H2/N2 enters through an
annular channel between the inner and outer pipes (36.51% by volume, 3.95% by
mass). The nitrogen is added to reduce heat transfer to the burner. The diffuse flame
research was performed in sections with axial symmetry. The choice of the area with
axial symmetry is explained by the relatively simple geometry when modeling the
flame.</p>
      <p>Measurements of the radial temperature distribution in three sections of the flame
at distances of 0, 30, and 60 mm from the cut of tubes (Fig. 2) were completed in a
mode corresponding to an average flow rate of air on the axis of 1 m/s and an average
flow rate of fuel of 0.8 m/s, using a platinum thermocouple.</p>
      <p>
        According to the dispersion formula Cauchy [7, 8]
  ( ) − 1 =   (1 +  2 +  4),
(
        <xref ref-type="bibr" rid="ref5">5</xref>
        )
the refractive index of the kth component of the burning mixture   depends on the
wavelength of the radiation source  and the parameters   ,   and   (  and   are
dispersion coefficients for the kth component,   is the relative molar concentration
of the kth component).The refractive index of the entire mixture is defined as
 − 1 =   0   0 ∑   (1 +  2 ) ∙   ,
(
        <xref ref-type="bibr" rid="ref6">6</xref>
        )
where  is the pressure;  0 - pressure (in the room);  is the temperature;  0 - room
temperature.The reconstruction of the values of molar concentrations of fuel
combustion products   and, accordingly, the temperature distribution in the flame is possible
by performing measurements at different wavelengths and using formulas (
        <xref ref-type="bibr" rid="ref5">5</xref>
        ) - (
        <xref ref-type="bibr" rid="ref6">6</xref>
        ).
Hermitian interpolation by the temperature values in sections at heights  = 3, 10, 20,
and 30 mm, is shown in Fig. 4.
      </p>
      <p>
        The phase structure of the probing light field, disturbed by the medium under study
(flame), in a physical experiment is defined as:
 2
 1
∆ψ( ,  ) =  ∫
[ ( ,  ,  ) −  0] ,
(
        <xref ref-type="bibr" rid="ref7">7</xref>
        )
(
        <xref ref-type="bibr" rid="ref8">8</xref>
        )
where  = 2 / is the wave number of the probing field;  ( ,  ,  ) is the refractive
index of the medium in the spatial structure of the flame;  0 is the refractive index of
the medium unperturbing by the flame. The  axis is determined by the direction of
the probe light beam, the flame torch cross section is described in  ,  coordinates.
The choice of the section position is determined by the  coordinate. The coordinates
 1,  2 specify the size of the flame section in the direction of the probe beam.
refractive index  ( ), calculated for  = 0.630 μm ( = 10 mm from the end of the burner tube
cut).
      </p>
      <p>
        Eq. (
        <xref ref-type="bibr" rid="ref7">7</xref>
        ) is turned into the Abel equation in the case of axial flame symmetry (Fig. 5):
where  2 =  2 +  2,  – the radius of the cross section of the considered zone,
 ( ,  ) – refractive index at a distance of  from the axis of the torch. Thus, the value
of the phase function ∆ψ can be restored by formula (
        <xref ref-type="bibr" rid="ref8">8</xref>
        ), knowing  0.
      </p>
      <p>The composition of dry air (relative molar concentrations of dry air components),
as well as the dependence of the saturated vapor pressure on temperature, must be
known to calculate the refractive index of the medium (air)  0 unperturbed by the
flame.</p>
      <p>
        Atmospheric pressure is equal to the sum of the partial pressures of the dry air
components and the partial pressure of water vapor. The partial pressure of water
vapor in the mixture (air) is determined by the formula for the relative humidity of air:
 
=   ∙ 0 ,
100
(
        <xref ref-type="bibr" rid="ref9">9</xref>
        )
where   is the partial pressure of water vapor,  0 is the saturated vapor pressure at
a given temperature,   is the relative air humidity in the room.
equation of state of an ideal gas, knowing the value of   :
where   is the universal gas constant,  0 is the room temperature. Similarly, we
calculate the value of the molar concentration of the entire mixture (air):
where  0 is atmospheric pressure (in the room).
      </p>
      <p>Then the relative molar concentration of water vapor in the air:


=   ,</p>
      <p>∙ 0
 =
 0 ,
  ∙ 0
 
=   .</p>
      <p>
        (10)
(11)
(12)
(13)
The refractive index  0 of the medium unperturbing by the flame, taking into account
(
        <xref ref-type="bibr" rid="ref6">6</xref>
        ) and (
        <xref ref-type="bibr" rid="ref9">9</xref>
        ) - (12), will be determined as
      </p>
      <p>. .  0
 0 = 1 +  0   . . [(∑   (1 +
 2 )) (1 −   ) + (  (1 +
 2
  ))   ],
where   . . - atmospheric pressure under normal conditions (101.325 ∙ 103 Pa);   . .
temperature under normal conditions (0°C);   and   - dispersion coefficients for
the kth component of dry air;</p>
      <p>and  
wavelength of the radiation source.</p>
      <p>- dispersion coefficients for water;  is the</p>
      <p>
        The radial field of the refractive index calculated by formula (
        <xref ref-type="bibr" rid="ref6">6</xref>
        ) is shown in
 =  0 = 101.325 ∙ 103 Pa (normal conditions),   and   are the values taken from
the reference data.
      </p>
      <p>
        The phase function must be reconstructed from the hilbertogram according to the
algorithm proposed in [2], and the refractive index of the medium must be determined
by determing the Abel equation to solve the inverse problem (reconstruction of the
flame temperature from the hilbertograms). The calculated inverse field of the phase
function (for the wavelength  = 0.630 μm), obtained by calculating the Abel integral
(
        <xref ref-type="bibr" rid="ref8">8</xref>
        ), is shown in Fig. 6.b.
      </p>
      <p>
        The refractive index depends on temperature and 4-x values of mole fraction of
combustion products, which follows from formula (
        <xref ref-type="bibr" rid="ref6">6</xref>
        ). Measurements at three
different wavelengths of the probing field are sufficient to determine all unknown
parameters, since the combustion area is divided into zones consisting of 3 components of
combustion products.
      </p>
      <p>The radial profiles of temperature, molar concentrations of combustion products,
refractive index and the corresponding values of the phase function, hilbertogram and
interferogram are shown in Fig. 7 for the section  = 10 mm and  = 0.630 μm.</p>
      <p>The numerically simulated hilbertograms obtained from the calculated phase
function ∆ψ for  = 0.630, 0.520, 0.405 μm, respectively, are shown in Fig. 8. The
dispersion coefficients were taken from the reference data, and the relative air humidity in
the room was taken</p>
      <p>= 60% in the numerical simulation of the hilbertograms.
The results obtained confirm the feasibility of multi-wave optical diagnostics in direct
and inverse problems of studying phase structure and temperature fields in an
axisymmetric flame.</p>
      <p>Optical Diagnostics of Temperature and Structural Parameters of an Axisymmetric Flame 9
The study of a hydrogen-air flame was done in the presented work using the methods
of Hilbert optics and numerical modeling in the approximation of axial symmetry of
the flame using the Abel integral. The reliability of the results is confirmed by
comparing the hilbertograms obtained in the experiment (Fig. 1.a) and reconstructed from
the phase structure according to the Abel equation (Fig. 8). The comparison results
are used as a quality criterion of the modeling the phase structure and temperature
field using the Abel transform in the study of the combustion process. The application
of the developed method for solving the inverse problem - restoration of the
temperature field from the Hilbert image of the phase structure of a hydrogen-air flame will
become the next stage of work.</p>
      <p>The work was done within the framework of the state assignment of IT SB RAS
project III.18.2.5 (state registration No. АААА-А17-117030310010-9, No.
ААААА17-117022850021-3), partial financial support from RFBR (project No.
20-3890195).</p>
    </sec>
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