Investigation of Aerosol Inhomogeneities Parameters in Planetary Boundary Layer in UV-A Spectral Region

P. A. Filimonov, S. Ivanov, V. Gorodnichev, M. L. Belov, Y. Fedotov
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Abstract

For today necessity of atmosphere wind remote sensing for wide pool of applications require development of new measurement methods and improvement of already existing.Currently doppler methods for wind speed measuring have largest sensing range. Correlation-based methods are provide lower sensing range for wind speed measurement. However, doppler-based lidar are expensive in opposite to simply designed correlation lidars that additionally allows to measure wind profile along sensing direction.Development of wind correlation lidars required knowledge of atmosphere aerosol inhomogeneities parameters.The most experimental research till now in this area are related to visible spectral range.One of the perspective eye-safety spectral range for wind lidar is UV spectral region. There not so much experimental research works of aerosol inhomogeneities parameters in UV.This paper is related to field experiments of aerosol inhomogeneities parameters in planetary boundary layer on 0.355 um operating wavelength.Block diagram and parameters of lidar with 0.355 operating wavelength is shown. Process of experiments is described. Typical atmosphere backscattering echo-signal for single laser pulse is demonstrated.Procedures if lidar signals processing are described, example of two-dimensional field of relative fluctuations of volume backscattering coefficient for different atmosphere conditions is shown.Results of measurement data processing shown that in planetary boundary layer average contrast of aerosol inhomogeneities in most cases has values in range 0,4% – 10 % (in case of snow up to 25%), and size in range 1,5 – 20 m. Dependency of observation number of aerosol inhomogeneities by range z from lidar to backscattering volume is descending with 1/z manner that the same for dependency for signal-noise ratio SNR(z).
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紫外- a光谱区行星边界层气溶胶不均匀性参数的研究
由于大气风遥感的广泛应用,需要开发新的测量方法和改进现有的测量方法。目前多普勒风速测量方法的传感范围最大。基于相关的方法为风速测量提供了较低的传感范围。然而,基于多普勒的激光雷达价格昂贵,与简单设计的相关激光雷达相反,后者可以沿着传感方向测量风廓线。发展风相关激光雷达需要了解大气气溶胶不均匀性参数。迄今为止,该领域的实验研究大多与可见光谱范围有关。紫外光谱区是风激光雷达对人眼安全的透视光谱范围之一。紫外辐射下气溶胶非均质性参数的实验研究并不多。本文对行星边界层在0.355 um工作波长上的气溶胶不均匀性参数进行了野外实验研究。给出了工作波长为0.355的激光雷达的框图和参数。描述了实验过程。给出了典型的单激光脉冲大气后向散射回波信号。描述了激光雷达信号的处理过程,给出了不同大气条件下体积后向散射系数相对波动的二维场实例。测量数据处理的结果表明,在大多数情况下,在行星边界层中,气溶胶不均匀性的平均对比值在0.4% - 10%范围内(在积雪高达25%的情况下),大小在1.5 - 20 m范围内。激光雷达波段气溶胶非均匀性观测数与后向散射体积的相关性呈1/z递减,信噪比SNR(z)的相关性也呈1/z递减。
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