Optical Spatial Filter to Suppress Beam Wander and Spatial Noise Induced by Atmospheric Turbulence in Free-Space Optical Communications

U. Darusalam, P. Priambodo, E. Rahardjo
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引用次数: 8

Abstract

We propose an optical spatial filter (OSF) method to suppress beam wander and spatial noise effects. Signal from random displacements of the focus spot around the optical axis within the constricted area is collected. This method advantageously suppresses fluctuations in signal intensity. The OSF consists of a pinhole and cone reflector. The pinhole produces Fresnel diffraction on the focus spot. The cone reflector provides directed reflectance onto the pinhole for random focus spot displacements due to beam wander. The calculations of signal power are based on fluctuations of signal intensity that are minimized by the circular aperture function of the pinhole and the cosine of the reflectance angle from the cone reflector. The method is applied to free-space optical communications at a wavelength of 1.55 μm with an atmospheric chamber to provide optical propagation media. Based on calculations, the beam wander angles that can be received by the OSF are from 14.0° to 28.0°. Moreover, based on experiment, the OSF with a pinhole diameter of 20.0 μm and cone reflector diameter of 1.5 mm produces signal power of −15.3 dBm. Both calculations and experiment show that the OSF enhances the received signal power in the presence of turbulence.
光学空间滤波器抑制自由空间光通信中大气湍流引起的光束漂移和空间噪声
提出了一种光学空间滤波(OSF)方法来抑制光束漂移和空间噪声效应。聚焦光斑在收缩区域内围绕光轴的随机位移信号被收集。这种方法有利地抑制了信号强度的波动。OSF由针孔和锥形反射器组成。针孔在焦点上产生菲涅耳衍射。锥形反射器提供了定向反射到针孔上的随机焦点点位移由于光束漫游。信号功率的计算基于信号强度的波动,该波动通过针孔的圆孔径函数和锥反射器反射角的余弦来最小化。将该方法应用于波长为1.55 μm的自由空间光通信中,在大气腔中提供光传播介质。根据计算,OSF能接收到的光束偏角范围为14.0°~ 28.0°。实验结果表明,针孔直径为20.0 μm、锥形反射镜直径为1.5 mm的光场产生的信号功率为−15.3 dBm。计算和实验结果表明,在存在湍流的情况下,OSF增强了接收信号的功率。
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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