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Proceedings Paper

Statistics of the turbulent phase in strong scintillation conditions
Author(s): Mikhail Charnotskii
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Paper Abstract

Under strong scintillation condition the phase of the optical field propagating through turbulence contains phase singularities. Commonly used statistical description of phase in terms of phase structure function is based on smooth perturbation (Rytov) theory, and does not account for singularities. Markov approximation for wave propagation in turbulence predicts asymptotically normal probability distribution with zero mean for the optical field under strong scintillation conditions, and provides an equation for the coherence function. These allow calculation of all statistics of the field including the amplitude and phase. We derive equations for the single and two-point joint and marginal probabilities distributions of the amplitude and phase, and equation for the phase structure function that are valid for the strong scintillation condition when phase singularities are present.

Paper Details

Date Published: 3 October 2014
PDF: 6 pages
Proc. SPIE 9224, Laser Communication and Propagation through the Atmosphere and Oceans III, 922405 (3 October 2014); doi: 10.1117/12.2061396
Show Author Affiliations
Mikhail Charnotskii, Zel Technologies, LLC (United States)
National Oceanic and Atmospheric Administration (United States)


Published in SPIE Proceedings Vol. 9224:
Laser Communication and Propagation through the Atmosphere and Oceans III
Alexander M. J. van Eijk; Christopher C. Davis; Stephen M. Hammel, Editor(s)

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