Acta Optica Sinica, Volume. 40, Issue 18, 1808001(2020)

Effect and Prediction Method of Specular Dust Based on Trough Solar System

Zhimin Wang1,2、*, Wenwu Chan1, Chang Yang1, Rui Tian1,2, Xiaofei Han1, Li Song1,2, and Chonggang Gao3
Author Affiliations
  • 1College of Energy and Power Engineering, Inner Mongolia University of Technology, Hohhot, Inner Mongolia 0 10051, China
  • 2Inner Mongolia Renewable Energy Key Laboratories, Hohhot, Inner Mongolia 0 10051, China
  • 3Inner Mongolia Peak Technology Limited Company, Hohhot, Inner Mongolia 0 10051, China
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    Figures & Tables(15)
    Effect of dust of concentrator surface on ray propagation path
    Effect of surface corrosion of concentrator on ray propagation path
    Layouts of dust samples. (a) Test device; (b) design diagram
    Comparison test platform of dual-axis tracking trough solar system
    Flow chart of thermodynamic performance test based on trough solar system
    Profile of cavity receiver
    Pictures of concentrators with dust under different working conditions. (a) Working condition 1; (b) working condition 2; (c) working condition 3
    Effect of environmental temperature on photothermal coupling factor of trough solar system
    Relative reflectance varies with wavelength at each measurement point. (a) Working condition 1; (b) working condition 2; (c) working condition 3
    Focal plane energy flux density on dusty mirror and clean mirror. (a) Working condition 1; (b) working condition 2; (c) working condition 3
    Acquisition factor varies with aperture width under different working conditions. (a) Working condition 1; (b) working condition 2; (c) working condition 3
    Change of acquisition factor correction coefficient caused by dust reflection factor
    Experimental and predicted values of thermal efficiency under different dust conditions
    • Table 1. Structural parameters of cavity receiver

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      Table 1. Structural parameters of cavity receiver

      TypeParameterValue
      Aperture widthWc /mm50
      Cavity width B /mm120
      CavityreceiverCavity height H /mm100
      Cavity length Lc /mm1500
      Diameter of tube d /mm10
      Number of tubes n7
    • Table 2. Main instruments

      View table

      Table 2. Main instruments

      Name of instrumentTypeAccuracy
      Float flowmeterLZB-2520 L/h
      Magnetic circulating pumpMP-100R
      ThermocoupleK0.75%
      Data interceptorTP7000.2%
      Radiation observation systemBSRN5 W/m2
      Energy flow densitometerGardon Gage3%
      Ultraviolet spectrophotometerUV-3600
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    Zhimin Wang, Wenwu Chan, Chang Yang, Rui Tian, Xiaofei Han, Li Song, Chonggang Gao. Effect and Prediction Method of Specular Dust Based on Trough Solar System[J]. Acta Optica Sinica, 2020, 40(18): 1808001

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    Paper Information

    Category: Geometric Optics

    Received: Mar. 23, 2020

    Accepted: Jun. 3, 2020

    Published Online: Aug. 28, 2020

    The Author Email: Wang Zhimin (wzm.imut@163.com)

    DOI:10.3788/AOS202040.1808001

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