2021
DOI: 10.1088/1367-2630/ac1fca
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The orbital angular momentum of a turbulent atmosphere and its impact on propagating structured light fields

Abstract: When structured light is propagated through the atmosphere, turbulence results in modal scattering and distortions. An extensively studied example is that of light carrying orbital angular momentum (OAM), where the atmosphere is treated as a phase distortion and numerical tools extract the resulting modal cross-talk. This approach focuses on the light itself, perturbed by the atmosphere, yet does not easily lend itself to physical insights, and fails to ask a pertinent question: where did the OAM that the beam… Show more

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Cited by 34 publications
(39 citation statements)
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“…bottom left plots in Fig. 3(a) and (b)], consistent with analytic findings for Kolmogorov turbulence [34]. Furthermore, the numerical results are in agreement with experimental data (circles in Fig.…”
supporting
confidence: 88%
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“…bottom left plots in Fig. 3(a) and (b)], consistent with analytic findings for Kolmogorov turbulence [34]. Furthermore, the numerical results are in agreement with experimental data (circles in Fig.…”
supporting
confidence: 88%
“…Crosstalk among pure OAM modes [top left plots in Fig. 3(a) and (b)] is distributed diagonally, evidence of the absence of coherent coupling between modes with opposite OAM, confirming previous findings [34]. The remaining phase information expressed by the diagonal's broadening is due to the disorder-induced coupling to neighboring modes = ± 1, 2... On the other hand, pure amplitude modes [top right plots in Fig.…”
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confidence: 84%
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“…This means that though it's a good idea to construct high dimensional Hilbert space by increasing the value of topological charge m, it may not be efficient in improving free space optical communication. In addition, it's to be noted that the OAM spectrum becomes asymmetric and shifts towards zero under increasing turbulence, which is due to the beam losing angular momentum to the turbulence [45]. Mathematically, this can be explained from the turbulence correlated coordinates a s and ξ s , as the shifts of the coordinates in x and y directions are asymmetric (see Supplement 1 for more information).…”
Section: Orbital Angular Momentum Spectrummentioning
confidence: 99%
“…Arguments have been put forward for one mode family being more robust than another, with studies covering Bessel-Gaussian [42][43][44][45][46][47][48][49][50][51][52][53], Hermite-Gaussian [54][55][56][57], Laguerre-Gaussian [58][59][60][61][62] and Ince-Gaussian [63] beams, with mixed and contradictory results. In the context of OAM, since the atmosphere itself can be thought of giving or taking OAM from the beam, it has been shown theoretically and experimentally that atmospheric turbulence distortions are independent of the original OAM mode [64], all susceptible to the deleterious effects of atmospheric turbulence, and indeed OAM has been suggested as not the ideal modal carrier through turbulence [65]. Vectorial structured light has been suggested to improve resilience because of the invariance of the polarisation degree of freedom, but numerous studies in turbulence [66][67][68][69][70][71][72][73] have been inconclusive, with some reporting that the vectorial structure is stable [67,68,73], and others not [69][70][71][72]74].…”
Section: Introductionmentioning
confidence: 99%