利用RBF神经网络和Kullback-Leibler距离对自由空间光学信道模型进行分类

G. Prakash, M. Kulkarni, U. Sripati
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引用次数: 8

摘要

自由空间光(FSO)通信系统提供免许可证和低成本的访问性能。无线光通信系统提供几乎无限的带宽。由于这些系统中使用的激光束受到空间限制,因此链路非常安全。然而,FSO链路只有在晴朗的天气条件下才能表现良好。云、雾、气溶胶和湍流极大地影响了FSO系统的性能,并导致接收信号的强度和相位波动。FSO链路可能遭受数据包损坏和擦除。人们提出了各种统计模型来描述大气湍流通道。对不同湍流程度的适当模式的选择取决于大气参数。本文采用径向基函数神经网络对通道进行分类,以确定最优拟合。我们还使用Kullback-Leibler距离作为参考分布与观测数据分布之间的度量。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Using RBF Neural Networks and Kullback-Leibler distance to classify channel models in Free Space Optics
Free Space Optical (FSO) communication systems offer a license free and cost effective access performance. FSO systems provide virtually unlimited bandwidth. Since the laser beams used in these systems are spatially confined, the links are very secure. However FSO links perform well only in clear weather conditions. Clouds, fog, aerosols, and turbulence drastically affect the performance of FSO systems and lead to fluctuations in both the intensity and phase of the received signal. FSO links can suffer from data packet corruption and erasure. Various statistical models have been proposed to describe the atmospheric turbulence channels. The choice of the appropriate model for varying level of turbulence is dependent on the atmospheric parameters. In this paper we classify the channels using Radial Basis Function Neural Networks to decide the best fit. We also use Kullback-Leibler distance as a measure between the reference distribution and the distribution of observed data.
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