大气湍流相屏的Zernike多项式模拟与验证

Liming Dai, S. Tong, Lei Zhang, Yinhuan Wang
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引用次数: 4

摘要

大气湍流是影响激光通信在大气中传播的主要因素之一,它会改变空气折射率的随机分布,严重影响光束通过大气后的成像质量。研究大气湍流,掌握大气湍流的变化,采取适当的方法控制和减少大气湍流对光束质量的影响。除了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。本文利用泽尼克多项式制作了大气湍流相屏。利用相位结构函数和大气相干长度来检验大气湍流相位屏是否正确。仿真结果表明,Zernike多项式法生成的大气湍流相位屏在低频分量与理论值一致,但在高频分量与理论值差异较大。原因是Zernike多项式法有一定的局限性。另外,通过增加阶次泽尼克多项式或改变接收孔径可以改变大气湍流相屏的湍流分布,但计算量大且复杂。因此,在激光通信系统的具体应用中,应考虑最佳的实验方案。大气湍流相位的统计性质可以用相结构函数来描述。因此,结构的功能将用于确定相屏仿真相屏是否准确。为了更好地了解两种方法模拟结果的差异,对泽尼克多项式模拟结果和功率谱反演模拟结果进行了比较。最后给出了相应的功率谱反演方法来模拟大气湍流相屏的模拟结果,并说明了该理论无需做介绍。
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On simulation and verification of the atmospheric turbulent phase screen with Zernike polynomials
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.
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