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Deep Learning for Solving Optical Inverse Problems: CNN-Based Wavelength Prediction and Phase Retrieval Techniques

This article provides an in-depth analysis of technical solutions for solving optical inverse problems using deep convolutional neural networks, covering the end-to-end implementation of predicting incident light wavelengths from Fraunhofer diffraction patterns.

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Published 2026-06-15 21:45Recent activity 2026-06-15 21:56Estimated read 5 min
Deep Learning for Solving Optical Inverse Problems: CNN-Based Wavelength Prediction and Phase Retrieval Techniques
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Section 01

[Introduction] Deep Learning for Solving Optical Inverse Problems: CNN-Based Wavelength Prediction and Phase Retrieval Techniques

This project was released by sanarhm on GitHub on June 15, 2026. Its core is to use deep convolutional neural networks (CNN) to solve optical inverse problems, enabling end-to-end prediction of incident light wavelengths from Fraunhofer diffraction patterns. The project uses the PyTorch framework and aims to break through the limitations of traditional methods. Original link: https://github.com/sanarhm/Deep-Learning-for-Optical-Pattern-Recognition-and-Phase-Retrieval-in-Engineering-Physics

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Section 02

Research Background: Challenges of Optical Inverse Problems

Optical inverse problems are classic challenges in engineering physics. Inverting wavelengths/phases from Fraunhofer diffraction patterns is an ill-posed problem (multiple solutions). Traditional methods like the Gerchberg-Saxton algorithm have high iteration costs, are prone to local optima, and are sensitive to noise. Deep learning provides a new direction for solving such problems through data-driven end-to-end learning.

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Section 03

Technical Solution: Fraunhofer Theory and CNN Architecture

Based on Fraunhofer diffraction theory (far-field diffraction, where wavelength is inversely proportional to the characteristic scale of the pattern), the project uses PyTorch to build a CNN: input preprocessed diffraction intensity patterns, extract spatial features (edges, textures, frequency distributions) via convolutional layers, output wavelength predictions (regression task), bypassing the complexity of traditional iterations.

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Section 04

Dataset Construction: Synthetic Data and Augmentation Strategies

Due to the difficulty in obtaining real data, synthetic data (labeled diffraction patterns generated based on physical principles) is used, covering various conditions (wavelength ranges, aperture shapes, noise). Data augmentation includes adding Gaussian noise, random rotation and scaling, adjusting contrast and brightness to improve model robustness.

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Section 05

Model Training: Loss Functions and Optimization Strategies

For the regression task, MSE/MAE loss functions are used; the optimizer is Adam (adaptive learning rate); learning rate decay and early stopping mechanisms (monitoring overfitting with the validation set) are adopted, and the dataset is divided into training/validation/test sets.

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Section 06

Technical Advantages: Efficiency, End-to-End, and Noise Resistance

Compared to traditional iterative algorithms, the trained model can predict with a single forward pass (milliseconds vs. seconds/minutes); no explicit physical modeling is needed, reducing reliance on domain knowledge; trained with noisy data, it has stronger noise resistance than traditional methods.

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Section 07

Application Prospects and Technical Limitations

Application scenarios: Real-time spectral analysis (industrial monitoring), phase retrieval imaging (X-ray crystallography, etc.), optical system calibration. Limitations: Generalization ability (accuracy decreases beyond training range), interpretability (black box), insufficient multi-parameter joint estimation. Future directions: Improve extrapolation ability, introduce explainable AI, support multi-task learning.

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Section 08

Conclusion: The Potential of Deep Learning in Optical Inverse Problems

This project demonstrates the potential of deep learning in solving optical inverse problems. CNN end-to-end learning enables wavelength prediction, with significant advantages in efficiency and noise resistance, providing a new research direction for optical inverse problems and promising applications in more engineering physics scenarios.