Deriving the slant visibility using the Klett method and the visualization of the slant visibility at the airport

Yuzhao Ma, Jiaqi Liu, Xing-long Xiong
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Abstract

Atmosphere visibility is one of the most important meteorological quantities in civil aviation domain. In practice the slant visibility is more important than the horizontal visibility for the pilot. With the help of the known Klett approach, a lidar can be used for determination of atmosphere extinction coefficient profiles. Consequently, the slant visibility can be obtained. However, the boundary value of the atmosphere extinction coefficient and the k factor in the relationship between atmosphere extinction coefficient and the atmosphere backscattering coefficient have to be firstly determined. In the present work we construct the nonlinear equations that the atmosphere extinction coefficient and the k factor must satisfy. As the solutions of the equations the atmosphere extinction coefficient and the k factor are for the first time obtained simultaneously. At the end the atmosphere extinction coefficients and the slant visibilities are obtained. The numerical simulations have been performed using the real lidar data and the aerosol optical depth observed by the installed sun photometer. The flights are demonstrated using the popular flight simulator Prepar3D under different visibilities.
利用Klett方法推导斜面能见度及机场斜面能见度的可视化
大气能见度是民航领域最重要的气象量之一。在实际操作中,对飞行员来说,倾斜能见度比水平能见度更重要。在已知的Klett方法的帮助下,激光雷达可以用于确定大气消光系数剖面。因此,可以获得倾斜能见度。但是,大气消光系数与大气后向散射系数的关系中,必须首先确定大气消光系数的边界值和k因子。本文构造了大气消光系数和k因子必须满足的非线性方程。作为方程的解,大气消光系数和k因子首次同时得到。最后得到了大气消光系数和倾斜能见度。利用实际激光雷达数据和安装的太阳光度计观测到的气溶胶光学深度进行了数值模拟。飞行演示使用流行的飞行模拟器prepare3d在不同的能见度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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