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Non-Uniformity Correction of Spatial Object Images Using Multi-Scale Residual Cycle Network (CycleMRSNet)
Chunfeng Jiang1,2, Zhengwei Li2, Yubo Wang1,2
1Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China.
Sensors (Basel, Switzerland)
|March 17, 2025
Summary
CycleMRSNet corrects non-uniform telescope image backgrounds using a novel CycleGAN architecture with multi-scale attention. This enhances image quality for better space object tracking and recognition systems.
Area of Science:
- Astronomy
- Computer Vision
- Image Processing
Background:
- Ground-based telescopes face stray light and vignetting, causing non-uniform backgrounds.
- Non-uniform backgrounds degrade signal-to-noise ratio for target tracking and recognition accuracy.
- Existing methods struggle to effectively correct these image artifacts.
Purpose of the Study:
- To propose CycleMRSNet, a novel network architecture for correcting non-uniform backgrounds in astronomical images.
- To enhance image processing capabilities using a multi-scale attention mechanism within a CycleGAN framework.
- To improve the accuracy and robustness of space object tracking and recognition systems.
Main Methods:
- Developed CycleMRSNet based on the CycleGAN framework.
- Integrated a multi-scale feature extraction module (MSFEM) in the generator.
- Embedded efficient multi-scale attention residual blocks (EMA-residual blocks) in the Resnet backbone.
- Trained the model on a small-scale dataset and tested on simulated and real images.
Main Results:
- CycleMRSNet achieved high performance metrics: PSNR 32.7923, SSIM 0.9814, and FID 1.9212 on the test set.
- The model significantly outperformed existing methods in background correction.
- Demonstrated improved focus on multi-scale information in high-dimensional feature maps.
Conclusions:
- CycleMRSNet effectively corrects non-uniform backgrounds in images from ground-based telescopes.
- The proposed architecture enhances feature extraction efficiency and attention to critical image areas.
- The method improves the overall robustness and accuracy of astronomical imaging systems.

