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Analysis of a satellite communication channel: optical scintillations and fade statistics

机译:卫星通信信道分析:光学闪烁和衰落统计

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Abstract: Estimates of the fractional fade time, expected number of fades, and mean duration of fade time associated with a transmitted Gaussian-beam wave are developed for uplink laser satellite-communication channels and compared with similar results based on a spherical wave model. Weak fluctuation theory using the lognormal model is applicable for zenith angles less than 60 degrees. Because spot size and off-axis scintillations are significant in the Gaussian- beam wave model but not for the spherical wave model, pointing errors become an important consideration in a reliable laser communication link. Off-axis scintillations increase even more rapidly for large diameter beams and can in some cases lead to a scintillation saturation for pointing errors greater than 1 $mu@rad off the optical beam axis. !8
机译:摘要:针对上行激光卫星通信信道,开发了与发射的高斯光束相关的衰落时间分数,预期衰落次数以及衰落时间平均持续时间的估计,并与基于球面波模型的相似结果进行了比较。使用对数正态模型的微弱波动理论适用于小于60度的天顶角。由于光斑尺寸和离轴闪烁在高斯光束波模型中很重要,而在球面波模型中却不重要,因此指向误差已成为可靠激光通信链路中的重要考虑因素。对于大直径光束,轴外闪烁的增加甚至更快,并且在某些情况下,由于指向误差会比光束轴大1muμrad,会导致闪烁饱和。 !8

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