• Acta Optica Sinica
  • Vol. 37, Issue 9, 0914004 (2017)
Ping Li*, Wei Han, Wei Wang, Huaiting Jia, Wanqing Huang, Fang Wang, Lidan Zhou, Bin Feng, Qihua Zhu, and Wanguo Zheng
Author Affiliations
  • Research Center of Laser Fusion, China Academy of Engineering Physics, Mianyang, Sichuan 621900, China
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    DOI: 10.3788/AOS201737.0914004 Cite this Article Set citation alerts
    Ping Li, Wei Han, Wei Wang, Huaiting Jia, Wanqing Huang, Fang Wang, Lidan Zhou, Bin Feng, Qihua Zhu, Wanguo Zheng. Defect Inspection by Band-Pass Imaging Related to Hot Image Property[J]. Acta Optica Sinica, 2017, 37(9): 0914004 Copy Citation Text show less
    Principle diagram of hot image formation
    Fig. 1. Principle diagram of hot image formation
    Distribution of phase defect
    Fig. 2. Distribution of phase defect
    Spatial distribution of beam with defect point. (a) Intensity on beam propagation axis (b) intensity on hot image screen; (c) intensity on hot image screen with a shadow in nonlinear medium
    Fig. 3. Spatial distribution of beam with defect point. (a) Intensity on beam propagation axis (b) intensity on hot image screen; (c) intensity on hot image screen with a shadow in nonlinear medium
    Optical schematic of band-pass imaging
    Fig. 4. Optical schematic of band-pass imaging
    Spatial frequency spectra of 16 phase defects
    Fig. 5. Spatial frequency spectra of 16 phase defects
    Three optical types applied to calculate the hot image intensity. (a) Optical type 1; (b) optical type 2; (c) optical type 3
    Fig. 6. Three optical types applied to calculate the hot image intensity. (a) Optical type 1; (b) optical type 2; (c) optical type 3
    Linear fitting of hot image relative intensity and relative brightness of defect filtered by band-pass window function in type 1
    Fig. 7. Linear fitting of hot image relative intensity and relative brightness of defect filtered by band-pass window function in type 1
    Linear fitting of hot image relative intensity and relative brightness with the optimal band-pass window for the different optical types. (a) Optical type 1; (b) optical type 2; (c) optical type 3
    Fig. 8. Linear fitting of hot image relative intensity and relative brightness with the optimal band-pass window for the different optical types. (a) Optical type 1; (b) optical type 2; (c) optical type 3
    No.Relative brightness of band-pass image (1~10 mm-1)Relative intensity of hot image
    Optical type 1Optical type 2Optical type 3
    111.01.01.0
    227088.26.31.8
    319247.16.51.9
    430517.04.52.2
    516547.52.41.8
    612516.52.02.0
    7492111.315.04.5
    8584111.621.06.4
    936518.914.05.0
    10700110.027.16.8
    114761.53.01.2
    12251.21.41.5
    1324576.07.01.6
    1414383.26.61.5
    1519944.56.51.5
    164834.81.61.6
    Table 1. Relationship between the band-pass filter parameters and hot image intensity of 16 phase defects
    Optical typeFilter window 1Filter window 2Filter window 3
    Type 10.9550.6930.844
    Type 20.8030.9780.960
    Type 30.8260.8810.922
    Table 2. Correlation coefficients of hot image relative intensity with the band-pass image relative brightness
    Ping Li, Wei Han, Wei Wang, Huaiting Jia, Wanqing Huang, Fang Wang, Lidan Zhou, Bin Feng, Qihua Zhu, Wanguo Zheng. Defect Inspection by Band-Pass Imaging Related to Hot Image Property[J]. Acta Optica Sinica, 2017, 37(9): 0914004
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