大气湍流衰落条件下基于apd的星地FSO链路信道仿真

H. Ivanov, Ziad Hatab, E. Leitgeb
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引用次数: 1

摘要

自由空间光学(FSO)是地面空间通信领域新兴的前沿技术,在扩展信息带宽方面具有显著的优势。无线光链路受到大气天气过程,特别是大气湍流的挑战,这在目前的工作中是唯一解决的。考虑到大气通道原型和湍流模拟,进行了FSO馈线链路的实验室表征,从而可以对高端组件和技术进行测试。为了利用最先进的带跨阻抗放大器(TIA)的APD接收机评估卫星到地面的光下行链路,利用自主开发的基于光纤可变衰减器的FSO信道仿真器。此外,输入的闪烁数据基于大量的大气探空观测数据库,并应用对数正态和伽玛-伽玛FSO信道建模。这导致被测APD-TIA光电探测器的精确表征,其性能是用高分辨率示波器和误码率测试仪测量的。因此,通过这种概念验证,可以在不涉及实际近地试验活动的情况下评估大气闪烁及其对卫星对地面激光通信情景的负面影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Channel Emulation of Satellite-to-Ground APD-based FSO Link in the Presence of Atmospheric Turbulence Fading
Free Space Optics (FSO) is emerging frontier technology in the field of ground-space communication that offers significant benefits in direction of expanding the information bandwidth. Wireless optical links are challenged by atmospheric weather processes and especially atmospheric turbulence, which is solely addressed in the current work. Considering atmospheric channel prototyping and turbulence simulations, laboratory characterization of FSO feeder links allowing tests of high-end components and technologies is carried out. In order to evaluate satellite-to-ground optical downlinks using a state-of-the-art APD receiver with Trans-Impedance Amplifier (TIA), self-developed FSO channel emulator implementing optical-fiber-based variable attenuator is utilized. Furthermore, the input scintillation data are modelled based on vast atmospheric radiosonde observation databases together with applying Log-normal and Gamma-Gamma FSO channel modelling. This leads to precise characterization of the used APD-TIA photodetector under test whose performance is measured with a high resolution oscilloscope and a bit error rate tester. Consequently, by means of this proof of concept, atmospheric scintillations and their negative influence over satellite-to-ground laser communication scenarios are evaluated without involving real near-Earth test campaigns.
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