Journal of the European Optical Society-Rapid Publications, Volume. 19, Issue 1, 2023015(2023)

Convolutional neural network optimisation to enhance ESPI fringe visibility

José Manuel Crespo* and Vicente Moreno*
Author Affiliations
  • QMatterPhotonics Research Group, Optics Area, Department of Applied Physics, Faculty of Physics / Faculty of Optics and Optometry, University of Santiago de Compostela, 15782 Santiago de Compostela, Galicia, Spain
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    Figures & Tables(6)
    Example setup for speckle pattern interferometry.
    Example U-NET network with an input image of 256 × 256 and 1 channel (B/N) and 32 × 32 resolution after the full encoder path. The decoder path reverses the encoding operations and uses inputs from the corresponding encoder layer (skip connections) to end with a cleaned output image.
    Generated image samples. (A) Computed ESPI image using only the n = 3, 8 and 14 first Zernike polynomials to simulate the complexity of specimen displacement. (B) Clean image or ground true, the sin(φ/2) component used to generate image (A).
    U-NET network finally used concatenating blocks consisting of two 5 × 5 convolutions (each one followed by a ReLU activation unit) and a 2 × 2 maxpooling operation with stride = 2 for downsampling along the encoding path, reversing the operations along the decoder path using blocks composed of upsampling operations followed by a 2 × 2 convolution (up-conv), concatenated with the corresponding output of the encoding part and followed by two 5 × 5 convolutions (each one followed by a ReLU activation unit).
    Samples of cleaned images using the selected hyperparameters. (A) Input image. (B) Expected output (Ground true). (C) Processed image by the U-NET. The SSMI index is computed using expected and processed image (columns B and C).
    • Table 1. Average SMMI value for the checked combinations of levels in the encoder path and kernel size.

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      Table 1. Average SMMI value for the checked combinations of levels in the encoder path and kernel size.

      Kernel size
      3 × 35 × 57 × 7
      Depth40.8960.9000.801
      50.7980.7600.728
      60.8800.8590.760
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    José Manuel Crespo, Vicente Moreno. Convolutional neural network optimisation to enhance ESPI fringe visibility[J]. Journal of the European Optical Society-Rapid Publications, 2023, 19(1): 2023015

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    Paper Information

    Category: Research Articles

    Received: Jan. 31, 2023

    Accepted: Mar. 23, 2023

    Published Online: Aug. 31, 2023

    The Author Email: Crespo José Manuel (josemanuel.crespo.continas@rai.usc.es), Moreno Vicente (josemanuel.crespo.continas@rai.usc.es)

    DOI:10.1051/jeos/2023015

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