Abstract

In the paper, we propose a novel prediction technique to predict Zernike coefficients from interference fringes based on Generative Adversarial Network (GAN). In general, the task of GAN is image-to-image translation, but we design GAN for image-to-number translation. In the GAN model, the Generator’s input is the interference fringe image, and its output is a mosaic image. Moreover, each piece of the mosaic image links to the number of Zernike coefficients. Root Mean Square Error (RMSE) is our criterion for quantifying the ground truth and prediction coefficients. After training the GAN model, we use two different methods: the formula (ideal images) and optics simulation (simulated images) to estimate the GAN model. As a result, the RMSE is about 0.0182 ± 0.0035λ with the ideal image case and the RMSE is about 0.101 ± 0.0263λ with the simulated image case. Since the outcome in the simulated image case is poor, we use the transfer learning method to improve the RMSE to about 0.0586 ± 0.0035λ. The prediction technique applies not only to the ideal case but also to the actual interferometer. In addition, the novel prediction technique makes predicting Zernike coefficients more accurate than our previous research.

Highlights

  • Aberration is the difference between an actual image and an ideal image in the optical system

  • According to the Testing_1 process, the Generator predicts 1000 fake images using the ideal image of interference fringe and obtains 1000 Root Mean Square Error (RMSE)

  • Summary We proposed a prediction technique to predict Zernike coefficients based on GoogLeNet with an interference fringe in a previous paper [25]

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Summary

Introduction

Aberration is the difference between an actual image and an ideal image in the optical system. Aberration is one of the essential reference indicators when designing an optical system. One method to measure aberration is an interferometer. The aberration information is recorded on the interference fringe image. Zernike coefficients could be calculated using traditional optical equations, such as the interference phase shift method, the Fourier transform method, and the phase-shift method. The conventional conversion methods convert interference fringe images to Zernike coefficients and require two steps, which are complex mathematical calculations. The interference fringe image is converted into the wavefront difference or phase difference. Zernike coefficients are calculated using the surface fitting method with Zernike polynomials [4]

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