Laser & Optoelectronics Progress, Volume. 61, Issue 13, 1312003(2024)

Extraction of Laser Spot Centroid of Turbulent Disturbance Based on Ellipse Fitting Method

Jianbing Wang1, Haifeng Yao2、**, Zhi Liu3、*, Keyan Dong3, and Shutong Liu1
Author Affiliations
  • 1School of Electronic and Information Engineering, Changchun University of Science and Technology, Changchun 130022, Jilin , China
  • 2School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China
  • 3National and Local Joint Engineering Research Center of Space and Optoelectronics Technology, Changchun University of Science and Technology, Changchun 130022, Jilin , China
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    Figures & Tables(16)
    Free space laser communication diagram
    Flow chart of proposed algorithm
    Weight coefficient selection process
    Comparison between the phase structure function and the theoretical structure function of different phase screen generation methods
    Spot distortion under different turbulence intensities. (a) Cn2=3×10-17 m-2/3; (b) Cn2=4.5×10-15 m-2/3;(c) Cn2=6×10-14 m-2/3; (d) Cn2=3.5×10-13 m-2/3
    Mean gray intensity within the mask under different turbulence intensities. (a) Cn2=4.5×10-16 m-2/3; (b) Cn2=2.5×10-13 m-2/3
    Simulation system
    Centroid extraction by different algorithms under weak turbulence. (a) Segmentation results of OTSU; (b) variable threshold segmentation; (c) edge of spot;(d) different algorithms for centroid extraction
    Mean gray intensity change curve of different spot centroid extraction methods with the change of mask radius R under different turbulence. (a) Weak turbulence; (b) moderate turbulence; (c) strong turbulence
    Real scene communication link
    Laser spot for real scene communication. (a) Original image; (b) segmented image; (c) centroid extraction
    Mean gray intensity with the change of mask radius
    • Table 1. Turbulent phase screen simulation parameters

      View table

      Table 1. Turbulent phase screen simulation parameters

      ParameterNumerical value
      Wavelength λ /nm1550
      Coherence length r00.1
      Internal scale l0 /m0.0001
      Outer scale L0 /m100
      Phase screen size L /m1
      Complex matrix dimension N512
    • Table 2. Main simulation parameters

      View table

      Table 2. Main simulation parameters

      ParameterWeak turbulenceStrong turbulence
      Wavelength λ /nm1064
      Cn2 /m-2/34.5×10-162.5×10-13
      Facula gridle ω0 /m0.02
      Phase screen size L /m1
      Transmission distance2000
      Number of phase screens10
      Weight coefficient ω1,ω25,2.41.8,1.42
    • Table 3. Centroid shift under different atmospheric turbulence

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      Table 3. Centroid shift under different atmospheric turbulence

      MethodWeak turbulenceModerate turbulenceStrong turbulence
      σΔx /pixelσΔy /pixelσΔx /pixelσΔy /pixelσΔx /pixelσΔy /pixel
      Proposed method6.957.2712.2710.5113.1212.64
      Ellipse fitting7.218.5113.6512.5417.7116.95
      Gray centroid method8.719.6525.8231.1437.7329.74
      Gravity center method7.607.3823.4127.1633.3125.08
    • Table 4. Centroid shift under different centroid extraction algorithms

      View table

      Table 4. Centroid shift under different centroid extraction algorithms

      MethodσΔx /pixelσΔy /pixel
      Proposed method4.3019.15
      Ellipse fitting4.4519.17
      Gray centroid method4.6919.18
      Gravity center method4.5719.16
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    Jianbing Wang, Haifeng Yao, Zhi Liu, Keyan Dong, Shutong Liu. Extraction of Laser Spot Centroid of Turbulent Disturbance Based on Ellipse Fitting Method[J]. Laser & Optoelectronics Progress, 2024, 61(13): 1312003

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    Paper Information

    Category: Instrumentation, Measurement and Metrology

    Received: Aug. 28, 2023

    Accepted: Oct. 19, 2023

    Published Online: Jul. 17, 2024

    The Author Email: Haifeng Yao (custfeng@outlook.com), Zhi Liu (liuzhi@cust.edu.cn)

    DOI:10.3788/LOP231987

    CSTR:32186.14.LOP231987

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