2023
DOI: 10.1088/1402-4896/acbbfd
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Propagation of hollow higher-order cosh-Gaussian beam in oceanic turbulence

Abstract: The averaged received intensity of hollow higher-order cosh-Gaussian (HHOCG) beam propagating in oceanic turbulence is derived based on extended Huygens–Fresnel integral. In detail, the effect of beam parameters and oceanic turbulence parameters on the received intensity is analyzed. Interestingly, beam has a focusing nature along propagation. Our results indicate that received intensity distribution is not affected from the variation in source field parameters. Beam size at the receiver plane can vary accordi… Show more

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Cited by 16 publications
(8 citation statements)
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References 29 publications
(28 reference statements)
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“…In this context, propagation and evolution of hollow beams in different random media have been studied widely in the literature and their advantages are presented [5,[12][13][14][15][16]. Regarding, cosh-Gaussian beam also has some application areas such as uniaxial crystal [17].…”
Section: Introductionmentioning
confidence: 99%
“…In this context, propagation and evolution of hollow beams in different random media have been studied widely in the literature and their advantages are presented [5,[12][13][14][15][16]. Regarding, cosh-Gaussian beam also has some application areas such as uniaxial crystal [17].…”
Section: Introductionmentioning
confidence: 99%
“…On the other hand, research on the behavior of laser beams propagating through oceanic turbulence has been a focus of attention up until now because underwater laser communications and imaging systems must perform various laser beams like pulsed vortex imaging (Benzehoua and Belafhal 2023a), Gaussian Schell-model Vortex Beam (Huang et al, 2014), hollow higherorder cosh-Gaussian beam (Elmabruk and Bayraktar 2023), cosine-Gaussian-correlated Schellmodel beam (Ding et al 2015), partially Coherent Radially Polarized Doughnut Beam (Fu and Zhang, 2013), vortex cosine hyperbolic-Gaussian beam (Lazrek et al 2022), hollow Gaussian beam (Li et al 2019), partially coherent anomalous hollow vortex beam (Liu et al 2019), partially coherent Lorentz-Gauss vortex beam (Liu et al 2017), radial Gaussian beam (Lu et al 2015), Gaussian array beam (Tang and Zhao 2015), partially coherent Gaussian beam (Yang et al 2017), rotating elliptical chirped Gaussian vortex beam (Ye et al 2018(Ye et al ), quasi-homogeneous beam (wen et al 2022) and hyperbolic sinusoidal Gaussian beam (Bayraktar 2021).…”
Section: Introductionmentioning
confidence: 99%
“…Many studies about the evolution properties of various laser beams propagating in oceanic turbulence have been analyzed (Tang and Zhao, 2013;Fu and Zhang, 2013;Liu et al, 2017a;Liu et al, 2017b;Huang et al, 2014;Xu and Zhao, 2014;Huang et al, 2015;Li et al, 2019;Lu et al, 2015a;Tang and Zhao, 2015;Lu et al, 2015b;Ding et al, 2015;Liu et al, 2015;Liu et al, 2016;Liu et al, 2017c;Liu and Wang, 2018;Liu et al, 2019;Lazrek et al, 2022;Liu et al, 2022;Elmabruk and Bayraktar , 2023;Benzehoua and Belafhal , 2023;Chib et al, 2023).…”
Section: Introductionmentioning
confidence: 99%
“…Since then, radially polarized beams (Tang and Zhao, 2013), partially coherent radially polarized doughnut beam (Fu and Zhang, 2013), four-petal Gaussian beam (Liu et al, 2017a;Liu et al, 2017b). Gaussian Schell-model vortex beam (Huang et al, 2014), stochastic electromagnetic vortex beams (Xu and Zhao, 2014), partially coherent Hermite-Gaussian linear array beam (Huang et al, 2015), hollow Gaussian beams (Li et al, 2019), Gaussian array beam (Lu et al, 2015a;Tang and Zhao, 2015;Lu et al, 2015b), cosine-Gaussian-correlated Schellmodel beams (Ding et al, 2015), flat-topped vortex hollow beam (Liu et al, 2015;Liu et al, 2016), partially coherent Lorentz-Gauss vortex beam (Liu et al, 2017c), random electromagnetic multi-Gaussian Schell-model vortex beam (Liu and Wang, 2018), partially coherent anomalous hollow vortex beam (Liu et al, 2019), vortex Cosine-Hyperbolic-Gaussian beams (Lazrek et al, 2022), multi-sinc Schell-model beams (Liu et al, 2022), hollow higherorder cosh Gaussian beam (Elmabruk and Bayraktar , 2023) pulsed Laguerre higher-order cosh-Gaussian beam (Benzehoua and Belafhal , 2023) and a new power spectrum of the refractive-index fluctuations turbulent oceanic (Chib et al, 2023).…”
Section: Introductionmentioning
confidence: 99%