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Published on: August 5, 2009
Statistics of spatially integrated speckle intensity difference.
Steen G Hanson1, Harold T Yura
1DTU-Fotonik, Department of Photonics Engineering, Danish Technical University, Roskilde 4000, Denmark. steen.hanson@risoe.dk
Summary
This study analyzes speckle intensity differences from separated apertures. We derived analytic solutions for probability and distribution functions, offering insights into optical field coherence and speckle statistics.
Area of Science:
- Optics and Photonics
- Statistical Optics
- Electromagnetic Wave Propagation
Background:
- Speckle patterns arise from coherent light scattering.
- Statistical properties of speckle are crucial for applications like imaging and remote sensing.
- Understanding intensity differences between separated apertures is key to characterizing optical fields.
Purpose of the Study:
- To derive closed-form analytic solutions for the statistics of spatially integrated speckle intensity differences.
- To investigate the impact of aperture size and optical field coherence on speckle statistics.
- To provide a theoretical framework for analyzing speckle phenomena in optical systems.
Main Methods:
- Consideration of spatially integrated speckle intensity differences from two separated finite collecting apertures.
- Derivation of probability density function (PDF) and cumulative distribution function (CDF) for fully developed speckle.
- Development of closed-form expressions for the nth statistical moments.
Main Results:
- Closed-form analytic solutions for PDF and CDF were successfully derived.
- Solutions are valid for arbitrary mean number of speckles and degree of coherence.
- Closed-form expressions for nth statistical moments were also obtained.
Conclusions:
- The study provides a comprehensive theoretical treatment of speckle intensity difference statistics.
- The derived solutions offer valuable tools for analyzing optical fields and speckle phenomena.
- This work advances the understanding of speckle statistics in optical systems with finite apertures.

