New results on turbulence modeling for free-space optical systems

N. Chatzidiamantis, H. Sandalidis, G. Karagiannidis, S. Kotsopoulos, M. Matthaiou
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引用次数: 57

Abstract

In this paper, we propose a statistical channel model, named as Double-Weibull, to describe the irradiance fluctuations in moderate and strong turbulence for free-space optical (FSO) systems. The proposed stochastic model is based on the scintillation theory and derived via the product of two Weibull random variables. Closed-form expressions of probability and cumulative density functions are provided in terms of Meijer's G-function. We also compare the new model with the classical gamma-gamma model and assess their accuracy via a set of simulations when both plane and spherical waves are considered. We finally evaluate the performance of an FSO system over the Double-Weibull turbulence channel and derive closed-form expressions for the bit-error rate, assuming intensity-modulation/direct detection with On-Off keying, and the outage probability.
自由空间光学系统湍流建模的新结果
本文提出了一种双威布尔统计通道模型,用于描述自由空间光学系统在中强湍流中的辐照度波动。该模型基于闪烁理论,由两个威布尔随机变量的乘积推导而成。用Meijer的g函数给出了概率函数和累积密度函数的封闭表达式。我们还将新模型与经典的伽玛-伽玛模型进行了比较,并通过一组考虑平面波和球面波的模拟来评估它们的准确性。我们最后评估了双威布尔湍流信道上的FSO系统的性能,并推导了误码率的封闭表达式,假设强度调制/直接检测与开关键控,以及中断概率。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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