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A Variational Method to Retrieve the Extinction Profile in Liquid Clouds Using Multiple-Field-of-View Lidar

机译:使用多视场激光雷达检索液体云中消光剖面的一种变分方法

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Liquid clouds play a profound role in the global radiation budget, but it is difficult to retrieve their vertical profile remotely. Ordinary narrow-field-of-view (FOV) lidars receive a strong return from such clouds, but the information is limited to the first few optical depths. Wide-angle multiple-FOV lidars can isolate radiation that is scattered multiple times before returning to the instrument, often penetrating much deeper into the cloud than does the single-scattered signal. These returns potentially contain information on the vertical profile of the extinction coefficient but are challenging to interpret because of the lack of a fast radiative transfer model for simulating them. This paper describes a variational algorithm that incorporates a fast forward model that is based on the time-dependent two-stream approximation, and its adjoint. Application of the algorithm to simulated data from a hypothetical airborne three-FOV lidar with a maximum footprint width of 600 m suggests that this approach should be able to retrieve the extinction structure down to an optical depth of around 6 and a total optical depth up to at least 35, depending on the maximum lidar FOV. The convergence behavior of Gauss-Newton and quasi-Newton optimization schemes are compared. Results are then presented from an application of the algorithm to observations of stratocumulus by the eight-FOV airborne Cloud Thickness from Off-Beam Lidar Returns (THOR) lidar. It is demonstrated how the averaging kernel can be used to diagnose the effective vertical resolution of the retrieved profile and, therefore, the depth to which information on the vertical structure can be recovered. This work enables more rigorous exploitation of returns from spaceborne lidar and radar that are subject to multiple scattering than was previously possible.
机译:液态云在全球辐射预算中发挥着重要作用,但很难远程获取其垂直剖面。普通的窄视场(FOV)激光雷达会从此类云层获得强劲的回报,但信息仅限于前几个光学深度。广角多FOV激光雷达可以隔离多次散射的辐射,然后再返回仪器,该辐射通常比单散射信号更深地渗透到云中。这些回波可能包含有关消光系数垂直剖面的信息,但由于缺乏用于模拟消光系数的快速辐射传输模型,因此难以解释。本文介绍了一种变分算法,该算法结合了基于与时间相关的两流逼近的快速前进模型及其伴随算法。将算法应用于假设的机载三FOV激光雷达(最大覆盖区宽度为600 m)的模拟数据表明,该方法应能够将消光结构的光学深度降低至大约6,总光学深度可达至少35,取决于最大激光雷达视场。比较了高斯-牛顿和拟牛顿优化方案的收敛性。然后将结果应用该算法应用于平流积云的观测,该观测结果是通过近束激光雷达回波(THOR)激光雷达的8 FOV机载云厚度测得的。演示了如何使用平均内核来诊断检索到的轮廓的有效垂直分辨率,从而诊断垂直结构信息的深度。这项工作可以比以前更严格地利用星际激光雷达和雷达的回波,这些回波会受到多重散射。

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