2016
DOI: 10.1103/physreva.93.033821
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Strong enhancing effect of correlations of photon trajectories on laser beam scintillations

Abstract: A distribution function approach is applied to describe the dynamics of the laser beam in the Earth atmosphere. Using a formal solution of the kinetic equation for the distribution function, we have developed an iterative scheme for calculation of the scintillation index (σ 2 ). The problem reduces to obtaining the photon trajectories and their correlations. Bringing together theoretical calculations and many-fold computer integrations, the value of σ 2 is obtained. It is shown that a considerable growth of σ … Show more

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Cited by 15 publications
(42 citation statements)
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“…(56). Finally, we note that the parameters (60) and (63) still contain the beam wandering variance, and we calculate σ 2 BW by means of Eq. (52).…”
Section: Probability Distribution Of Transmittancementioning
confidence: 99%
“…(56). Finally, we note that the parameters (60) and (63) still contain the beam wandering variance, and we calculate σ 2 BW by means of Eq. (52).…”
Section: Probability Distribution Of Transmittancementioning
confidence: 99%
“…The evolution equation for PDF is derived from Heisenberg's equation. Although in more general case its evolution is gathered by Boltzmann-Langevin equation [29] which takes to account whole range of possible changes in photon momentum due to collisions with atmosphere inhomogeneities, for reasonably long distances (see [30]) description with collisionless Boltzmann equation…”
Section: Photon Distribution Functionmentioning
confidence: 99%
“…where g = |g| and we also used Markov approximation index-of-refraction spectrum is delta-correlated in the direction of propagation, which was rigorously justified in [30]. After integration over direction of g…”
Section: Acknowledgmentsmentioning
confidence: 99%
See 1 more Smart Citation
“…Here k is the optical wave number, C 2 n is the turbulence refractive-index structure constant, L is the propagation length, W 0 is the beam-spot width at the transmitter site, and Ω=kW 2 0 /2L is the Fresnel parameter. In general, the calculation of the correlation functions and their moments requires high-accuracy numerical integrations [42,62,63].…”
Section: Application To Atmospheric Channelsmentioning
confidence: 99%