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超几何高斯光束在吸收型各向异性海洋湍流中的平均信道容量

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超几何高斯(HyGG)光束具有近似无衍射、自聚焦和自重构特性,有望用于提升基于轨道角动量(OAM)的水下光通信系统的信道容量.基于Rytov近似及广义惠更斯菲涅耳原理推导了HyGG光束在吸收型各向异性海水信道下的OAM探测概率及平均信道容量的解析表达式.分析了HyGG光束在无湍流衰减信道下的光强分布,并详细探究了光源参数、信道环境参数及通信系统参数对HyGG光束传输及通信质量的影响.结果表明,HyGG光束的自聚焦能力随空心度参数的增大而增强.光束的波长、OAM模式数、束腰半径、空心度参数以及发射功率、接收孔径尺寸、OAM信道数、传输距离、湍流的强度、各向异性程度、内外尺度均会对通信系统的平均信道容量产生影响.通信系统误码率与平均信道容量变化趋势相反.此外,空心度参数大于0的HyGG光束在远距离传输下的传输及通信特性优于拉盖尔高斯(LG)光束及高斯涡旋(GV)光束.这些结果对基于HyGG光束的水下光通信链路的搭建具有重要指导意义.
Average Channel Capacity of Hypergeometric Gaussian Beams in Absorbing Anisotropic Ocean Turbulence
Objective We aim to investigate the transmission and communication characteristics of the Hypergeometric-Gaussian(HyGG)beam,which exhibits pseudo-nondiffraction,self-focusing,and self-reconstruction characteristics.These properties are expected to enhance the channel capacity of underwater optical communication(UWOC)systems based on orbital angular momentum(OAM).While there is growing interest in the transmission of the HyGG beam through turbulent media,recent research on its performance in underwater channels remains limited.The team led by Shengmei Zhao explores the spiral phase spectrum evolution of the HyGG beam based on the Nikishov oceanic turbulence power spectrum.However,the Nikishov spectrum exhibits a singularity at zero spatial wave number,and the absorption effects of seawater and anisotropic impacts on the transmission of HyGG beam OAM modes have not been adequately addressed.Furthermore,the existing study investigates the OAM detection probability evolution of the HyGG beam only within less than 0.1 times the Rayleigh distance,failing to fully demonstrate its transmission advantages.Thus,it is essential to introduce a new oceanic turbulence power spectrum and conduct theoretical research on the long-distance transmission and communication performance of the HyGG beam in an absorbent and anisotropic oceanic turbulence channel.This research provides a vital reference for designing and improving practical underwater wireless optical communication systems.Methods To further investigate the transmission and communication characteristics of the HyGG beam in underwater channels,we introduce a newly proposed oceanic turbulence power spectrum.We comprehensively consider the effects of seawater absorption and anisotropy.Based on the Rytov turbulence approximation theory and the new oceanic turbulence power spectrum,we derive the analytical expression of the OAM spiral phase spectrum for the HyGG beam under absorptive and anisotropic oceanic turbulence.Subsequently,using the established average channel capacity model,we analyze in detail the influence of the HyGG beam parameters,seawater channel parameters,and communication system parameters on the average channel capacity during long-distance transmission.Results and Discussions The influence of oceanic turbulence leads to an increase in spiral wavefront distortion with increasing transmission distance.The vortex beam with OAM mode number gradually disperses its energy into neighboring OAM modes.After transmitting 200 m,the OAM detection probability of the HyGG beam is approximately 20%higher than that of the Gaussian vortex(GV)beam and 10%higher than that of the Laguerre-Gaussian(LG)beam.This is due to the stronger self-focusing ability of the HyGG beam,which results in smaller beam broadening in oceanic channels and fewer turbulent cells with varying refractive indices.Consequently,the HyGG beam exhibits reduced wavefront distortion and higher purity of OAM signal modes during transmission in oceanic channels(Fig.3).For practical applications,selecting the appropriate p value of the HyGG beam according to different communication distances effectively enhances system performance(Fig.4).The average channel capacity of the HyGG beam decreases with increasing l0,favoring larger p values for higher average channel capacity due to faster divergence of the HyGG beam with larger l0 values(Fig.5).To mitigate the effects of seawater absorption in long-distance UWOC,we recommend the HyGG beam in the 410-490 nm range.Additionally,selecting the appropriate initial waist radius of the HyGG beam according to actual underwater communication distance requirements maximizes average channel capacity(Fig.6).The average channel capacity of the HyGG beam increases with increasing turbulence scale and decreases with increasing outer scale.Furthermore,the channel capacity increases with the anisotropy parameter,benefiting transmission and communication in seawater(Fig.7).The average channel capacity decreases with increasing root mean square temperature dissipation rate xT and temperature-salinity gradient ratio w,and increases with the kinetic energy dissipation rate ε.Higher values of w,Xt,or lower values ofε,increase oceanic turbulence intensity,exacerbating wavefront distortion and deteriorating transmission and communication performance of the HyGG beam in oceanic channels(Fig.8).At 50 m,the average channel capacity of the HyGG beam is nearly independent of the size of the receiving aperture.With increasing transmission distance,the average channel capacity initially increases and then decreases with larger receiving aperture size,stabilizing at Ra=3 mm with a peak value.These phenomena can be explained as follows:1)at shorter transmission distances,optical signal energy attenuation and inter-mode crosstalk are minimal,and the received optical power significantly exceeds system noise power N0,thus channel capacity is primarily determined by OAM signal mode power and crosstalk power,with little influence from varying the receiving aperture size;2)Although reducing the receiving aperture size can enhance OAM detection probability,longer distances and smaller receiving apertures also result in greater power loss.When received optical power approaches N0,average channel capacity is primarily influenced by received optical power(Fig.10).Conclusions We derive analytical expressions for the OAM detection probability and average channel capacity of the HyGG beam in absorptive anisotropic oceanic channels based on the Rytov approximation and generalized Huygens-Fresnel principle.Our analysis covers the intensity distribution of the HyGG beam in turbulence-free channels and extensively studies the influence of source parameters,channel environmental parameters,and communication system parameters on the transmission and communication quality of the HyGG beam.The results indicate that the self-focusing ability of the HyGG beam increases with the hollowness parameter.The influence of oceanic turbulence on the HyGG beam increases with transmission distance,temperature variance dissipation rate,turbulence inner scale,and OAM mode number,while it decreases with kinetic energy dissipation rate,turbulence outer scale,and anisotropy parameter.The system's average channel capacity increases with higher transmit power and OAM channel number.The trend of the communication system error rate is opposite that of average channel capacity.For different communication link lengths,optimal values for HyGG beam wavelength,waist radius,hollowness parameter,and receiving aperture values exist to maximize the system's average channel capacity.Additionally,due to its self-focusing characteristics,the HyGG beam with hollowness parameter p>0 demonstrates superior transmission and communication performance over LG and GV beams in long-distance transmission.Therefore,The HyGG beam exhibits strong resistance to turbulence and attenuation.

hypergeometric Gaussian beamsocean turbulenceorbital angular momentumbit error rateaverage channel capacity

常帅、陈航、张鹏、何爽、王圆鑫、于浩、徐进、南航、佟首峰

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长春理工大学光电工程学院,吉林长春 130022

中国科学院长春光学精密机械与物理研究所,吉林 长春 130033

珩辉光电测量技术(吉林)有限公司,吉林长春 130117

吉林大学通信工程学院,吉林长春 130012

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超几何高斯光束 海洋湍流 轨道角动量 误码率 平均信道容量

2024

光学学报
中国光学学会 中国科学院上海光学精密机械研究所

光学学报

CSTPCD北大核心
影响因子:1.931
ISSN:0253-2239
年,卷(期):2024.44(23)