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Experimental verification of optical backhaul links for high-altitude platform networks: Atmospheric turbulence and downlink availability

机译:高空平台网络光学回波链路的实验验证:大气湍流和下行链路可用性

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摘要

Optical backhaul downlinks from high-altitude platforms (HAPs) are investigated. An experiment demonstrated the advantages of optical links: a small and lightweight terminal with low power consumption was launched to the stratosphere and data transmitted down to a ground station at a rate of 1.25 Gbit/s: Owing to the chosen system parameters and the high budget margin, disturbing turbulence effects did not decrease the link performance.udThe scientific aspect of the experiment was to study turbulence effects in order to design future systems with higher transmission performance. On the day of the experiment, measured scintillation and wavefront distortions were minimal in the morning. The best atmospheric conditions were observed about 3 h afterudsunrise with a peak of the atmospheric coherence length r0 at 16 cm. An r0 of 4 cm was measured as the worst case before sunrise and later during the day. This trend could also be observed for power- and intensity scintillation index. The latter changed from 0.28 (best case) to 1.12. For small scintillation index audlognormal intensity probability density function was measured. udApart from the robust intensity modulation scheme with direct detection which was used for the trial, future improved systems could benefit from a coherent transmission scheme. According to the r0 measurements and further simulations on heterodyne efficiency it turned out that the aperture size can be decreased from 40 to 10 cm without any significant change in the link margin. udFuture stratospheric optical links between HAPs or links from platforms to satellites will not suffer from cloud blockage but it remains an issue for up/downlinks to a ground station. This can be mitigated by ground-station diversity. Four optical ground stations in the southern part of Europe can lead to an availability of over 98%. The separation distance of the ground stations is about 900 km with a negligible correlation of cloud cover. A change of wavelength from the employed 1.55 to a wavelength around 11 micronsudwith minimum cloud attenuation would increase the link availability for thin clouds.
机译:研究了来自高空平台(HAPS)的光学回程下行链路。实验证明了光学链接的优点:以1.25 Gbit / s的速率向地面电位的流层和数据发射小而轻量级的终端,并以1.25 Gbit / s的速度向地面传输到地面:由于所选择的系统参数和高预算裕度,令人不安的湍流效应没有减少链接性能。 ud实验的科学方面是研究湍流效应,以设计具有更高传输性能的未来系统。在实验的当天,测量的闪烁和波前扭曲在早晨是最小的。在 UDSUNRISE之后,观察到最佳的大气条件约为3小时,大气相干长度R0在16厘米处。在日出之前的最坏情况下,在日出之前和白天后来的案例测量了4厘米的R0。对于功率和强度闪烁指数,也可以观察到这种趋势。后者从0.28(最佳案例)变为1.12。对于小的闪烁指数,测量 UDLognormal强度概率密度函数。 Udapart从具有用于试验的直接检测的强大强度调制方案,未来的改进系统可以从相干传输方案中受益。根据R0测量和进一步模拟外差效率,证明光圈尺寸可以从40到10cm降低,而不会在链接边距发生任何显着变化。 Udfuture哈普斯或来自卫星平台的链路之间的划分光学链路不会遭受云阻塞,但它仍然是向上/下行链路的问题。这可以通过地站多样性来减轻。欧洲南部的四个光学地段可能导致可用性超过98%。地面站的分离距离约为900 km,云盖相关不计。从所采用的1.55到波长的波长的变化为大约11微米 Udwith最小云衰减将增加薄云的链接可用性。

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