三波长偏振激光雷达系统的改进校准方法和探测误差模拟

Laibin Wang, Dong Liu
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引用次数: 0

摘要

偏振激光雷达在探测大气中非球形气溶胶粒子的微物理特性以及气溶胶与云之间的间接相互作用方面发挥着重要作用。然而,偏振激光雷达系统中存在各种复杂的光电元件,这些元件的不完善往往给系统准确接收数据带来困难。为了确保多波长偏振激光雷达系统探测数据的准确性,对系统进行精确校准是至关重要的一步。本文基于三波长(355nm、532nm、1064nm)偏振激光雷达系统。在 Freudenthaler 等人提出的 ± 45 ° 偏振激光雷达系统校准方法的基础上,设计了一种改进的校准方法,用于校准不同波长的探测通道。新的校准方法纠正了± 45 °方法的一些问题,并提出了一种计算方法,以减少级联多个二向反射镜对接收信号的影响。 仿真结果表明,使用平均偏振误差角成功地减少了级联多个二向反射镜对信号的影响。文章最后,我们通过仿真计算验证了所提方法在不同探测波长下的误差分析。结果表明,在探测大气分子等极小大气颗粒时,探测误差约为 6%。在探测去极化比大于 0.1 的非球形粒子时,每个探测通道的误差可降至 3% 以下。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
An improved calibration method and detection error simulation for three-wavelength polarization lidar systems
Polarization lidar plays an important role in detecting the microphysical properties of non spherical aerosol particles in the atmosphere and the indirect interaction between aerosols and clouds. However, there are various complex optoelectronic components in polarization lidar systems, and the imperfect nature of these components often poses difficulties for the system to accurately receive data. To ensure the accuracy of the detection data of a multi wavelength polarization lidar system, precise calibration of the system is a crucial step. This article is based on a three wavelength (355nm, 532nm, 1064nm) polarization lidar system. Based on the ± 45 ° polarization lidar system calibration method proposed by Freudenthaler et al, an improved calibration method is designed to calibrate different wavelength detection channels. The new calibration method corrects some issues with the ± 45 ° method and proposes a calculation method to reduce the impact of cascading multiple dichroic mirrors on the received Signal The simulation results show that the use of the average polarization error angle successfully reduces the impact of cascading multiple dichroic mirrors on the signal. At the end of the article, we validated the error analysis of the proposed method under different detection wavelengths through simulation calculations. The results show that when detecting extremely small atmospheric particles such as atmospheric molecules, the detection error is around 6%. When detecting non spherical particles with a depolarization ratio greater than 0.1, the error of each detection channel can be reduced to less than 3%.
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