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Far-field focusing of laser beam based on digital image processing techniques

机译:基于数字图像处理技术的激光束远场聚焦

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摘要

In order to lead the laser beam transmit in the atmosphere convergently, an experiment of laser focus at the distance of 450m and 300m has been operated in the outdoor place. The actual manipulations are as follows: Firstly, the laser was collimated by a beam expander, then the near-parallel laser beam was transmitted with a Galileo telescope system, and the distance between the concave lens and the convex lens can be tuned through a precise displacement platform, so the focus of the system changed due to the tiny displacement of the concave lens. Secondly, the average power of the laser spot can be measured using power meter, the power is 47.67mW and the standard deviation is 0.67mW while the focal length is 450m. Thirdly, the energy distribution was found through the laser beam analyzer. The spot images were saved using the beam analyzer, then the saved image can be processed with Matlab software afterwards. The function named EDGE and Sobel operator was used in the pre-processing of the saved image, then method of median filter was used in the course of image de-noising and 53H filter was adopted in the signal analysis. The diameter of laser spot was obtained by the method above, the diameter is 5.56mm and the standard deviation is 0.24mm. The spot center excursion is 0.56mm, it is 10.43% of the total diameter of the laser spot. At last, the key factors of the energy dissipation in the focusing system can be summarized as follows: restriction of the diffraction limit, attenuation in the atmosphere, geometrical aberration of optical system, and the diffraction limit and the geometrical aberration are significant in the three factors above, so we can reduce the impact of the both factors during the design of optical system. The reliable referenced data of the system design can be acquired through the primary experiment research.
机译:为了使激光束汇聚到大气中,在室外进行了450m和300m距离的激光聚焦实验。实际的操作如下:首先,通过扩束器对激光进行准直,然后使用伽利略望远镜系统传输近乎平行的激光束,然后可以通过精确地调整凹透镜和凸透镜之间的距离。位移平台,因此系统的焦点由于凹透镜的微小位移而改变。其次,可以使用功率计测量激光光斑的平均功率,功率为47.67mW,标准偏差为0.67mW,焦距为450m。第三,通过激光束分析仪发现能量分布。使用光束分析仪保存斑点图像,然后可以使用Matlab软件处理保存的图像。在保存图像的预处理中使用了EDGE和Sobel运算符功能,然后在图像去噪过程中使用了中值滤波方法,在信号分析中采用了53H滤波。通过上述方法得到激光光斑的直径,直径为5.56mm,标准偏差为0.24mm。光斑中心偏移为0.56mm,是激光光斑总直径的10.43%。最后,聚焦系统能量耗散的关键因素可归纳为:衍射极限的限制,大气衰减,光学系统的几何像差,衍射极限和几何像差在这三个方面都很重要。以上因素,因此我们可以在设计光学系统时减少这两个因素的影响。系统设计的可靠参考数据可以通过初步的实验研究获得。

著录项

  • 来源
    《Optoelectronic imaging and multimedia technology》|2010年|p.78502N.1-78502N.9|共9页
  • 会议地点 Beijing(CN)
  • 作者单位

    Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences,State Key Laboratory of Laser Interaction with Matter, Changchun, 130033 , China;

    Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences,State Key Laboratory of Laser Interaction with Matter, Changchun, 130033 , China;

    Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences,State Key Laboratory of Laser Interaction with Matter, Changchun, 130033 , China;

    Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences,State Key Laboratory of Laser Interaction with Matter, Changchun, 130033 , China;

    Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences,State Key Laboratory of Laser Interaction with Matter, Changchun, 130033 , China;

  • 会议组织
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 多媒体技术与多媒体计算机;光电子技术、激光技术;
  • 关键词

    image processing; far-field focusing; Sobel operator; 53H filter; centroid drift;

    机译:图像处理;远场聚焦; Sobel运算符; 53H过滤器;重心漂移;

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