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Published on: January 14, 2020
Wide viewing angle dynamic holographic stereogram with a curved array of spatial light modulators
Joonku Hahn1, Hwi Kim, Yongjun Lim
1School of Electrical Engineering, Seoul National University, Gwanak-Gu Sillim-Dong, Seoul 151-744, Korea.
Optics Express
|August 6, 2008
Summary
A novel curved array of spatial light modulators (SLMs) enables wider viewing angles for dynamic holographic stereograms. This design overcomes limitations of planar displays, significantly reducing light loss and improving scalability for digital holographic systems.
Area of Science:
- Optics and Photonics
- Display Technology
- Holography
Background:
- Achieving wide viewing angles in digital holographic displays is challenging.
- Previous methods required extremely large planar spatial light modulators (SLMs), where paraxial approximations fail.
- Existing systems struggle to balance viewing angle width with display capabilities.
Purpose of the Study:
- To propose a novel dynamic holographic stereogram design using a curved array of SLMs.
- To overcome the limitations of planar SLMs in achieving wide viewing angles.
- To simplify optical structure and reduce light power loss in holographic displays.
Main Methods:
- A curved array of SLMs is employed to increase data points and reduce spatial bandwidth per SLM.
- Each SLM displays local angular spectra of the object wave, based on holographic stereogram principles.
- SLMs are reformed to simplify optics and minimize light power loss, effectively acting as sub-SLMs.
Main Results:
- The proposed design achieves a 22.8-degree viewing angle for digital holographic displays.
- Scalability in viewing angle is significantly improved.
- Light power loss is substantially reduced compared to conventional methods.
Conclusions:
- The curved SLM array offers a scalable solution for wide-angle holographic displays.
- This novel design enhances dynamic holographic stereogram performance.
- The system provides a practical approach to high-quality digital holographic imaging.

