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- W2012950131 endingPage "17344" @default.
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- W2012950131 abstract "Analytical formula is derived for the M(2)-factor of coherent and partially coherent dark hollow beams (DHB) in turbulent atmosphere based on the extended Huygens-Fresnel integral and the second-order moments of the Wigner distribution function. Our numerical results show that the M(2)- factor of a DHB in turbulent atmosphere increases on propagation, which is much different from its invariant properties in free-space, and is mainly determined by the parameters of the beam and the atmosphere. The relative M(2)-factor of a DHB increases slower than that of Gaussian and flat-topped beams on propagation, which means a DHB is less affected by the atmospheric turbulence than Gaussian and flat-topped beams. Furthermore, the relative M(2)-factor of a DHB with lower coherence, longer wavelength and larger dark size is less affected by the atmospheric turbulence. Our results will be useful in long-distance free-space optical communications." @default.
- W2012950131 created "2016-06-24" @default.
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- W2012950131 date "2009-09-14" @default.
- W2012950131 modified "2023-09-27" @default.
- W2012950131 title "M^2-factor of coherent and partially coherent dark hollow beams propagating in turbulent atmosphere" @default.
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- W2012950131 doi "https://doi.org/10.1364/oe.17.017344" @default.
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