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On simulation and verification of the atmospheric turbulent phase screen with Zernike polynomials

机译:Zernike多项式仿真与验证大气湍流相屏的仿真与验证

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Atmospheric turbulence is one of the main factors that influence the spread of laser communication in the atmosphere affect, which will change the random distribution of the refractive index of air, and affect the image quality of the beam through the atmosphere seriously. To study atmospheric turbulence in order to grasp changes in atmospheric turbulence, by taking the appropriate methods to control and reduce the effects of atmospheric turbulence on the beam quality. In addition to studying atmospheric turbulence using experimental methods and theoretical analysis. Numerical simulation is an effective means to study the problem of turbulence. Zernike polynomials were used to produce atmospheric turbulence phase screen in this article. The phase structure function and the atmospheric coherence length were used to check whether the atmospheric turbulence phase screen is right or not. Simulation results were studied show that, the atmospheric turbulence phase screen generated with Zernike polynomial method was consistent with the theoretical values in the low spatial frequency components, but, the simulation results had big difference with the theoretical values in the high spatial frequency components. The reason is that Zernike polynomials method has some limitations. In addition, the distribution of turbulence in the atmospheric turbulence phase screen can be changed by increasing the Zernike polynomials of orders or changing the receiving apertures, but which involves great and complex calculation. Therefore, in the specific application of the laser communication system, the best experimental program should be considered. Statistical properties of atmospheric turbulence phase can be described by the phase structure function. Therefore, the structure of the function will be used to determine the phase screen simulation phase screen is accurate. To give a better understanding of both methods the difference between simulation results, the simulation results of Zernike polynomials and power spectral inversion simulation results were compared. At last to give the corresponding power spectrum inversion method to simulate atmospheric turbulence phase screen simulation results and shows that the theory without making the introduction.
机译:大气湍流是影响大气中激光通信扩散影响的主要因素之一,这将改变空气折射率的随机分布,并严重地影响梁的图像质量。为了掌握大气湍流,以通过采用适当的方法来掌握大气湍流的变化,以控制和减少大气湍流对光束质量的影响。除了使用实验方法和理论分析研究大气湍流之外。数值模拟是研究湍流问题的有效手段。 Zernike多项式用于在本文中生产大气湍流相筛网。相位结构功能和大气相干长度用于检查大气湍流相屏是否是右或不正确的。研究了仿真结果表明,用Zernike多项式方法产生的大气湍流相屏与低空间频率分量中的理论值一致,但是,模拟结果与高空间频率分量中的理论值具有很大差异。原因是Zernike多项式方法具有一些限制。另外,可以通过增加Zernike多项式的订单或改变接收孔的Zernike多项式来改变大气湍流相屏幕的湍流分布,但是涉及巨大和复杂的计算。因此,在激光通信系统的具体应用中,应考虑最佳实验程序。可以通过相位结构功能描述大气湍流阶段的统计性质。因此,该功能的结构将用于确定相屏仿真相位屏幕是准确的。为了更好地了解两种方法模拟结果之间的差异,比较了Zernike多项式和功率谱反转模拟结果的仿真结果。最后给出相应的功率谱反转方法来模拟大气湍流相屏仿真结果,并显示理论而不进行介绍。

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