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Experimental study of laser beam propagation in turbulent atmosphere

机译:激光在湍流中传播的实验研究

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Intensity of atmospheric turbulence may overly affect bit error rate for a ground-based laser wireless communication system, so it is necessary to measure of atmospheric turbulence intensity and fluctuation of image centroid while laser beam propagates in turbulent atmosphere. In this paper, an experiment system is set up based on theory of lighttransmission in turbulent atmosphere. In the system, a laser named Nd : YAG is used horizontally to emit a laser beamwith wavelength 1.06 μm on a platform at the height of 1.5 m. Three infrared CCD cameras are set at 200 m, 300 m(or600 m) and 1000 m far from laser, which are applied to receive laser facula images from Lambertian boards,respectively.A lot of laser facula images are collected within some serial days under different periods of time every day, and hundredsof image frames are gathered at a time by making use of this experiment device. Fluctuation of image centroid iscomputed with these image frames, and the structure constant of atmospheric refractive index (C_n~2 ) is also derived. Finally, a comparison is made between aforementioned C_n~2 and those derived by meteorology factors.
机译:对于基于地面的激光无线通信系统,大气湍流的强度可能会过度影响误码率,因此有必要在激光束在湍流大气中传播时测量大气湍流强度和图像质心的波动。本文建立了基于光理论的实验系统 传播在动荡的气氛中。在该系统中,水平使用名为Nd:YAG的激光发射激光束 在1.5 m高度的平台上的波长为1.06μm。三台红外CCD摄像机分别设置为200 m,300 m(或 距离激光600 m)和1000 m,它们用于接收来自Lambertian板的激光光斑图像, 分别。 每天在不同的时间段内,在连续的几天内收集了大量的激光光斑图像,数百个 利用该实验装置一次收集图像帧。图像质心的波动是 利用这些图像帧进行计算,并且还推导了大气折射率的结构常数(C_n〜2)。最后,对上述C_n〜2与气象因子推导的C_n〜2进行了比较。

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