Impact Analysis of the Atmosphere Optical State on Wind Lidar Sounding Range

M. L. Belov, A. A. Samsonova, S. Ivanov, V. Gorodnichev
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Abstract

One of the most important questions for correlation lidars is the sounding range question.Correlation lidar sounding range greatly depends not only on the parameters of the equipment, but also on the optical state of the earth's atmosphere.In addition, there are currently two approaches to the estimation of lidar sounding range. In one approach, an estimate of the sounding range is obtained by equating the detector threshold power to the laser signal power recorded by the detector. In another approach, an estimate of the sounding range is obtained by equating the minimum detectable energy of the detected laser signal energy.This paper is about impact research of the atmosphere optical state on wind correlation lidar sounding range and compare sounding range estimates obtained under the two different approaches to the energy calculation lidar.The analysis is carried out for the surface layer of the atmosphere, the horizontal sounding path and the radiation wavelength of 0.532 μm. In atmospheric haze conditions, an empirical formula is used for the attenuation factor. The signal-to-noise ratio is assumed to be 100.Solid-state Nd:YAG Ekspla lasers NL319 (lamp pumping, pulse energy 5 J) and NL231-100 (diode pumping, pulse energy 90 mJ) were chosen as radiation sources.Hamamatsu photomultiplier tube R5070A with radiant sensitivity ~ 50 mA/W was chosen as a detector.It is shown that in a wide optical state range (meteorological range of visibility from 20 to 2 km) the lamp-pumped laser source sounding range with pulse energy 5 J varies from ~ 3,8 km to ~ 1,2 km and the diode-pumped laser source sounding range with pulse energy 90 mJ varies from ~ 1,1 km to ~ 0,64 km.The approach based on comparison of the detector threshold power with the received laser signal power overestimates the sounding range due to incomplete influencing consideration factors.
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大气光学状态对风激光雷达探测距离的影响分析
相关激光雷达最重要的问题之一是探测距离问题。相关激光雷达探测距离不仅在很大程度上取决于设备参数,而且还取决于地球大气的光学状态。此外,目前激光雷达探测距离的估计有两种方法。在一种方法中,探测距离的估计是通过将探测器的阈值功率与探测器记录的激光信号功率相等来获得的。在另一种方法中,探测距离的估计是通过将探测到的激光信号能量的最小可探测能量相等来获得的。本文研究了大气光学状态对风相关激光雷达探测距离的影响,比较了两种不同的能量计算激光雷达探测距离估算方法。对大气表层、水平探测路径和辐射波长0.532 μm进行了分析。在大气雾霾条件下,衰减系数采用经验公式。信噪比假定为100。选择固态Nd:YAG Ekspla激光器NL319(灯泵浦,脉冲能量5 J)和NL231-100(二极管泵浦,脉冲能量90 mJ)作为辐射源。选用辐射灵敏度为50 mA/W的滨松光电倍增管R5070A作为探测器。结果表明,在较宽的光学状态范围内(气象能见度20 ~ 2 km),脉冲能量为5 J的灯泵浦激光源探测距离在~ 3.8 km ~ ~ 1.2 km之间变化,脉冲能量为90 mJ的二极管泵浦激光源探测距离在~ 1.1 km ~ ~ 0.64 km之间变化。基于探测器阈值功率与接收到的激光信号功率比较的方法由于影响因素不完全,高估了探测距离。
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