2011
DOI: 10.1364/oe.20.000452
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Aberration corrections for free-space optical communications in atmosphere turbulence using orbital angular momentum states

Abstract: The effect of atmosphere turbulence on light's spatial structure compromises the information capacity of photons carrying the Orbital Angular Momentum (OAM) in free-space optical (FSO) communications. In this paper, we study two aberration correction methods to mitigate this effect. The first one is the Shack-Hartmann wavefront correction method, which is based on the Zernike polynomials, and the second is a phase correction method specific to OAM states. Our numerical results show that the phase correction me… Show more

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Cited by 175 publications
(77 citation statements)
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“…There have also been theoretical suggestions to recover lost entanglement 18 ; however, it is yet to be demonstrated experimentally. In the context of OAM modes, the decay of entanglement has been both predicted 19 and measured 20 for atmospheric turbulence as an environment, with some success in diminishing these effects [21][22][23] .…”
mentioning
confidence: 99%
“…There have also been theoretical suggestions to recover lost entanglement 18 ; however, it is yet to be demonstrated experimentally. In the context of OAM modes, the decay of entanglement has been both predicted 19 and measured 20 for atmospheric turbulence as an environment, with some success in diminishing these effects [21][22][23] .…”
mentioning
confidence: 99%
“…4 shows how the PSNR values of the reconstructed image with and without RS error correction codes vary with the strength of atmosphere turbulence for four-level grayscale, eight-level grayscale and sixteen-level grayscale objects. According to the atmosphere turbulence model [22], the random phase screen caused by atmosphere turbulence is mainly determined by the constant of the index of refraction. Hence, we calculate the PSNR for various strength of the turbulent aberration.…”
Section: Numerical Resultsmentioning
confidence: 99%
“…As a beam propagates through AT, the beam will be scattered by refractive index inhomogeneities. We use the thin sheet phase screens model [22] to simulate the turbulence aberration. For convenience, we denote the phase aberration of AT by , where , and .…”
Section: A the Theoretical Analysis Of The Turbulence Influence On Hmentioning
confidence: 99%
“…Such robustness appears at first glance counterintuitive, because the encoding involves the use of OAM, which is quite sensitive to all the above-mentioned spatial perturbations 37,38 (although significant progresses in pure OAMbased classical and quantum communication through the atmosphere have been recently reported [39][40][41] ). The main reason for such robustness is that the OAM spread induced by spatial-mode perturbations is neutralized by the polarization degree of freedom, which is in contrast very robust against those spatial-mode perturbations.…”
Section: Robustness Of Rotational-invariant Hybrid Qubitsmentioning
confidence: 99%