Photon distribution function for long-distance propagation of partially coherent beams through the turbulent atmosphere

G. P. Berman and A. A. Chumak
Phys. Rev. A 74, 013805 – Published 18 July 2006

Abstract

The photon density operator function is used to calculate light beam propagation through turbulent atmosphere. A kinetic equation for the photon distribution function is derived and solved using the method of characteristics. Optical wave correlations are described in terms of photon trajectories that depend on fluctuations of the refractive index. It is shown that both linear and quadratic disturbances produce sizable effects for long-distance propagation. The quadratic terms are shown to suppress the correlation of waves with different wave vectors. We examine the intensity fluctuations of partially coherent beams (beams whose initial spatial coherence is partially destroyed). Our calculations show that it is possible to significantly reduce the intensity fluctuations by using a partially coherent beam. The physical mechanism responsible for this pronounced reduction is similar to that of the Hanbury-Braun–Twiss effect.

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  • Received 24 April 2006

DOI:https://doi.org/10.1103/PhysRevA.74.013805

©2006 American Physical Society

Authors & Affiliations

G. P. Berman1,* and A. A. Chumak1,2

  • 1Theoretical Division and the Center for Nonlinear Studies, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
  • 2Institute of Physics of the National Academy of Sciences, prospect Nauki 46, Kiev-28, MSP 03028, Ukraine

  • *Email address: gpb@lanl.gov

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Vol. 74, Iss. 1 — July 2006

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