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Non-Lambertian Photometric Stereo Network based on Inverse Reflectance Model with Collocated Light
This study introduces a novel non-Lambertian photometric stereo network for accurate surface normal estimation using fewer images. The method effectively decouples surface normal from reflectance, improving flexibility and handling shadows.
Area of Science:
- Computer Vision
- Computer Graphics
- Photometry
Background:
- Traditional photometric stereo requires numerous images for accurate surface normal estimation.
- Non-Lambertian reflectance poses challenges for conventional methods.
Purpose of the Study:
- To develop a non-Lambertian photometric stereo network for accurate surface normal recovery with sparse lighting.
- To address limitations of current methods requiring a large number of images.
Main Methods:
- Derived an inverse reflectance model using monotonicity and univariate properties for collocated light.
- Employed supervised deep learning for enhanced shadow rejection and model flexibility.
- Utilized max-pooling for shadow handling and neighborhood image patches for reflectance variation.
Main Results:
- The proposed method achieves state-of-the-art accuracy in surface normal estimation.
- Demonstrated effectiveness on both synthetic and real-world image datasets.
- Successfully decouples surface normal from reflectance, enabling sparse light recovery.
Conclusions:
- The novel network provides a robust solution for non-Lambertian photometric stereo under sparse lighting conditions.
- Deep learning integration significantly enhances shadow rejection and adaptability to diverse reflectances.
- The method offers a more efficient and accurate approach to surface normal estimation.
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