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Measurement of atmospheric coherence length with differential movement of the image sensor

机译:利用图像传感器的差分运动测量大气相干长度

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This paper gives the introduction about a new measuring device which is to measure th e atmospheric coherence length by using the differential movement principle.The system can observe the edge of the sun in the day time, and also observe planets at night. This system can measure the atmospheric coherence length in both horizontal and slant directions. The measurement in the day time requests the assistance of the attenuator and beacon beam of the atmospheric coherence length in the direction of the slant path.The working principle is the laser beam scattered by atmospheric turbulence through into the receiving optical system. Because the receiving system which is consists of two completely symmetrical telephoto optical system. Therefore, two optical channels in turbulence device are completely identical. After passing through the optical channels, the beam focusing is finished. By adjusting the optical system manually or automatically, two light point images can be formed on the photosensitive element of the CCD. Atmospheric turbulence can cause phase fluctuation of wave front. After aggregation by the receiving lens, The photosensitive element of CCD can collect the relative jitter of the two imaging optical centroid positions we require, and researchers can obtain relative changes from the two centroid positions by the calculations of computer software, as the result, the atmospheric coherence length is obtained. By means of the simulation of the optical system and the imaging quality optimization by Code V, researchers can rather achieve transfer function diagram, the circle of confusion value in different views and energy distribution. From above, researchers can examine whether the optical system is being qualified, or the method is leading to a better observation effect. At end of this dissertation, the limitations of this system will be analyzed, and the improvement methods and suggestions will be provided.
机译:本文介绍了一种新的测量装置,该装置利用微分运动原理测量大气的相干长度。该系统可以在白天观测太阳边缘,在夜晚观测行星。该系统可以测量水平方向和倾斜方向上的大气相干长度。白天的测量需要倾斜方向的大气相干长度的衰减器和信标束的辅助。工作原理是由大气湍流散射的激光束进入接收光学系统。因为接收系统是由两个完全对称的远摄光学系统组成的。因此,湍流装置中的两个光通道是完全相同的。通过光通道后,光束聚焦完成。通过手动或自动调节光学系统,可以在CCD的感光元件上形成两个光点图像。大气湍流会引起波前的相位波动。通过接收透镜聚集后,CCD的感光元件可以收集我们需要的两个成像光学质心位置的相对抖动,研究人员可以通过计算机软件的计算从两个质心位置获得相对变化,结果是获得了大气相干长度。通过光学系统的仿真和Code V的成像质量优化,研究人员可以更好地实现传递函数图,不同视图中的混淆值圈和能量分布。从上面,研究人员可以检查光学系统是否合格,或者该方法是否可以带来更好的观察效果。最后,分析了该系统的局限性,并提出了改进的方法和建议。

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