compensation in digital holographic imaging of the retina Julie - - PowerPoint PPT Presentation

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compensation in digital holographic imaging of the retina Julie - - PowerPoint PPT Presentation

Deep neural networks for aberration compensation in digital holographic imaging of the retina Julie Rivet 12 , G. Tochon 2 , S. Meimon 3 , M. Paques 4 , T. Graud 2 , M. Atlan 1 , Institut Langevin 1 , ESPCI Paris LRDE 2 , EPITA ONERA 3 Ctr.


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SLIDE 1

Deep neural networks for aberration compensation in digital holographic imaging of the retina

Julie Rivet12, G. Tochon2, S. Meimon3, M. Paques4, T. Géraud2, M. Atlan1,

Institut Langevin1, ESPCI Paris LRDE2, EPITA ONERA3

  • Ctr. Hospitalier d’Ophtalmologie des Quinze-Vingts4
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SLIDE 2

Introduction

  • Project: holographic imaging of the retina in real-time
  • Problem: aberrations created by cornea disturb holographic imaging
  • Fast estimation and correction of aberrations are necessary
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SLIDE 3

Outline I. Digital holographic imaging

  • II. Aberration estimation
  • III. Prospects

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I. Digital holographic imaging

  • II. Aberration estimation
  • III. Prospects
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SLIDE 4

Setup and image formation

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Angular spectrum propagation

Block of interferograms

𝑢 𝑨 = 0 𝑢

Block of holograms

𝝃 𝑦 𝑧 𝑨

Block of spectrograms

Sensor plane Image plane Image plane

Time Fourier transform

Real-time processing with Holovibes

𝑨 = 0 𝑧 𝑧 𝑦 𝑦

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SLIDE 5

5 Fluctuation spectrum calculation

Doppler images

𝝃 𝑦 𝑧

Block of spectrograms

Image plane Holography Doppler images taken and processed by Léo Puyo from Institut Langevin 𝑨 = 0

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SLIDE 6

Impact of aberrations from cornea

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Goal: aberration correction in real-time

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SLIDE 7

Outline

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I. Digital holographic imaging

  • II. Aberration estimation
  • III. Prospects
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SLIDE 8

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Astigmatism estimation by image-based optimization

Astigmatism 0°, 45° and 90°

Minimization of

Aberrated image Corrected image Aberrated wavefront

Holography Doppler images taken and processed by Léo Puyo

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SLIDE 9

Aberration measurement with digital wavefront sensor

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Principle of Shack-Hartmann wavefront sensor Simulations

Tests on real data in progress…

  • Each aberration corresponds to one degree of Zernike

polynomial (one mode).

  • M reference matrix of size nsubapertures x nmodes
  • Y = MA, where Y is observation vector (nsubapertures x 1)

and A is amplitude vector (nmodes x 1)

  • Then M is reversed to find A.
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SLIDE 10

Aberration compensation with deep neural network

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U-Net

input : image

  • utput : image

Ronneberger, et al. "U-net: Convolutional networks for biomedical image segmentation." International Conference on Medical image computing and computer- assisted intervention. Springer, Cham, 2015.

Interferograms Hologram reconstruction Processings & corrections Images of the retina Deep neural network

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SLIDE 11

Hologram rendering with a U-Net

11 Training: one defocus Reconstruction: the same amount of defocus Results: good correction

Input: aberrated hologram Ground truth Reconstructed image Training on 28 000 Input/output image couples

UNet

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SLIDE 12

Hologram rendering with a U-Net

12 Training: one average aberration Reconstruction: variety of aberrations close to the avg. Results: U-Net not suitable as is to learn a diversity of aberrators

Aberrated image Aberration compensation through deep learning Ground truth

Time sequence of aberrations taken from real eyes with 30 different types of aberrations

N=30

Jessica Jarosz, Pedro Mecê, Jean-Marc Conan, Cyril Petit, Michel Paques, and Serge Meimon, "High temporal resolution aberrometry in a 50-eye population and implications for adaptive

  • ptics error budget," Biomed. Opt. Express 8, 2088-2105 (2017)
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SLIDE 13

Outline

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I. Digital holographic imaging

  • II. Aberration estimation
  • III. Prospects
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SLIDE 14

Prospects

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What if the aberrator has a large number of degrees of freedom?

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SLIDE 15

Cataracts compensation using deep neural networks

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N=30 N=1 N=100000

Training : one random phase screen filtered by gaussian filter (σ=0,4) Reconstruction : variety of phase screens « close » to the one used for training Issue : UNET not suitable « as is » to learn a diversity of « aberrators »

Aberrated image Aberration compensation through deep learning Ground truth

Increase of # of degrees of freedom

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SLIDE 16

To go further Work on the training database:

  • With a large amount of images with several types of complex objects,

increasing the degrees of freedom to correct more and more aberrations.

  • What if the object is the simplest one ?

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SLIDE 17

Digital Gabor hologram rendering with deep learning

17 Collection of random points Synthetic interferogram Angular spectrum propagation Synthetic magnitude hologram For training database

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SLIDE 18

Digital Gabor hologram rendering with deep learning

18 With simulated images

Synthetic interferogram Synthetic magnitude hologram Reconstructed hologram with neural networks

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SLIDE 19

Digital Gabor hologram rendering with deep learning

19 With real data (worms)

Experimental interferogram Magnitude hologram Reconstructed hologram with neural networks

Data courtesy of Stéphanie Rind from Institut Langevin

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SLIDE 20

Thank you !

Funding: European Research Council (ERC Helmholtz, grant agreement #610110)

Contact: julie.rivet@espci.fr

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SLIDE 21

Digital Gabor hologram rendering with deep learning

21 With real data (worms)

Experimental interferogram Magnitude hologram Reconstructed hologram with neural networks

Data courtesy of Stéphanie Rind from Institut Langevin

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SLIDE 22

Aberrations

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