Properties of a random electromagnetic multi-Gaussian Schell-model vortex beam in oceanic turbulence

2018 ◽  
Vol 124 (9) ◽  
Author(s):  
Dajun Liu ◽  
Yaochuan Wang
2021 ◽  
Vol 9 (10) ◽  
pp. 1139
Author(s):  
Xinguang Wang ◽  
Le Wang ◽  
Shengmei Zhao

Based on the extended Huygens–Fresnel principle and the power spectrum of anisotropic oceanic turbulence, the analytical expressions of the average intensity and coherence properties of an off-axis hollow Gaussian-Schell model (OAHGSM) vortex beam propagating through anisotropic oceanic turbulence were derived. The effects of turbulent ocean and beam characteristic parameters on the evolution properties of the OAHGSM vortex beam were analyzed in detail. Our numerical simulation results showed that the OAHGSM vortex beam with a larger position factor is more focusable. Meanwhile, the OAHGSM vortex beam eventually evolves into a Gaussian-like beam after propagating through the anisotropic oceanic turbulent channel. The speed of this process can be accelerated by the decrease of the hollow order, topological charge, beam width, and transverse coherence width of the beam. The results also indicated that the normalized average intensity spreads more greatly and the spectral degree of coherence decays more rapidly for the smaller dissipation rate of the kinetic energy per unit mass of fluid, the smaller anisotropic coefficient, the smaller inner scale factor, the larger dissipation rate of the mean-squared temperature, and the higher temperature–salinity contribution ratio.


Author(s):  
Wei Wang ◽  
Ping Wang ◽  
Weina Pang ◽  
Yuting Pan ◽  
Yuanhao Nie ◽  
...  

2020 ◽  
Vol 59 (32) ◽  
pp. 9956
Author(s):  
Zonghua Hu ◽  
Huilong Liu ◽  
Jing Xia ◽  
Aga He ◽  
Hongbo Li ◽  
...  

2017 ◽  
Vol 56 (31) ◽  
pp. 8785 ◽  
Author(s):  
Dajun Liu ◽  
Hongming Yin ◽  
Guiqiu Wang ◽  
Yaochuan Wang

2021 ◽  
Vol 9 (4) ◽  
pp. 442
Author(s):  
Xinguang Wang ◽  
Le Wang ◽  
Shengmei Zhao

In this paper, we use two methods to research the propagation characteristics of a Hypergeometric-Gaussian (HyGG) vortex beam under oceanic turbulence. One is numerical calculation based on the Rytov approximation theory, where the theoretical detection probability equation of the HyGG vortex beam propagating through oceanic turbulence is derived. The other is numerical simulation based on random phase screens model of oceanic turbulence, where the influences generated by oceanic turbulence on the phase and intensity of the propagation beam as well as the propagation of the beam through several independent phase screens, kept at the same distance, have the same effect. The effects of oceanic turbulence parameters and initial beam parameters on the detection probability of the HyGG vortex beam at the receiver are discussed. The results of theoretical derivation are well in agreement with those of numerical simulation, which demonstrated that the numerical simulation method could effectively simulate the complex theoretical derivation. Both results show that with higher dissipation rate of kinetic energy per unit mass of fluid, smaller dissipation rate of mean-squared temperature and lower temperature-salinity contribution ratio comes the better detection probability. Meanwhile, a HyGG vortex beam with smaller topological charge and longer wavelength has a superior turbulent resistance property. It provides a promising way to estimate the propagation characteristics of the optical beams in an underwater environment.


2018 ◽  
Vol 426 ◽  
pp. 456-462 ◽  
Author(s):  
Feng Ye ◽  
Jianbin Zhang ◽  
Jintao Xie ◽  
Dongmei Deng

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