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

机译:使用Klett方法得出倾斜的可见性,并在机场直观显示倾斜的可见性

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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.
机译:大气能见度是民航领域最重要的气象量之一。实际上,对于飞行员来说,倾斜的可见性比水平的可见性更为重要。借助已知的Klett方法,可以使用激光雷达确定大气消光系数曲线。因此,可以获得倾斜的可见性。但是,必须首先确定大气消光系数和大气反向散射系数之间的关系中的大气消光系数和k因子的边界值。在本工作中,我们构造了大气消光系数和k因子必须满足的非线性方程。作为方程式的解,首次同时获得了大气消光系数和k因子。最后,获得了大气的消光系数和倾斜的可见性。使用真实的激光雷达数据和已安装的太阳光度计观察到的气溶胶光学深度进行了数值模拟。使用流行的飞行模拟器Prepar3D在不同的可见性下演示了这些飞行。

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