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使用大涡模拟/短波辐射传输模型模拟辐射亮度测试用于校正近云反射率增强的双层模型

Testing the Two-Layer Model for Correcting Near Cloud Reflectance Enhancement Using LES/SHDOM Simulated Radiances.

作者信息

Wen Guoyong, Marshak Alexander, Várnai Tamás, Levy Robert

机构信息

NASA Goddard Space Flight Center, Greenbelt, Maryland.

GESTAR/Morgan State University, Maryland.

出版信息

J Geophys Res Atmos. 2016 Aug 24;121(16):9661-9674. doi: 10.1002/2016JD025021. Epub 2016 Aug 9.

DOI:10.1002/2016JD025021
PMID:32742895
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC7394312/
Abstract

A transition zone exists between cloudy skies and clear sky, such that clouds scatter solar radiation into clear sky regions. From a satellite perspective, it appears that clouds enhance the radiation nearby. We seek a simple method to estimate this enhancement, since it is so computationally expensive to account for all 3-dimensional (3D) scattering processes. In previous studies, we developed a simple two-layer model (2LM) that estimated the radiation scattered via cloud-molecular interactions. Here we have developed a new model to accounts for cloud-surface interaction (CSI). We test the models by comparing to calculations provided by full 3D radiative transfer simulations of realistic cloud scenes. For these scenes, the MODIS-like radiance fields were computed from the Spherical Harmonic Discrete Ordinate Method (SHDOM), based on a large number of cumulus fields simulated by the UCLA Large Eddy Simulation (LES) model. We find that the original 2LM model that estimates cloud-air molecule interactions accounts for 64% of the total reflectance enhancement, and the new model (2LM+CSI) that also includes cloud-surface interactions accounts for nearly 80%. We discuss the possibility of accounting for cloud-aerosol radiative interactions in 3D cloud induced reflectance enhancement, which may explain the remaining 20% of enhancements. Because these are simple models, these corrections can be applied to global satellite observations (e.g. MODIS) and help to reduce biases in aerosol and other clear-sky retrievals.

摘要

多云天空和晴朗天空之间存在一个过渡区域,云层会将太阳辐射散射到晴朗天空区域。从卫星观测的角度来看,云层似乎增强了附近的辐射。由于考虑所有三维(3D)散射过程的计算成本过高,我们寻求一种简单的方法来估算这种增强效应。在之前的研究中,我们开发了一个简单的两层模型(2LM)来估算通过云 - 分子相互作用散射的辐射。在此,我们开发了一个新模型来考虑云 - 表面相互作用(CSI)。我们通过与逼真云场景的全3D辐射传输模拟所提供的计算结果进行比较来测试这些模型。对于这些场景,类似MODIS的辐射场是根据球谐离散坐标法(SHDOM)计算得出的,该方法基于加州大学洛杉矶分校大涡模拟(LES)模型模拟的大量积云场。我们发现,估算云 - 空气分子相互作用的原始2LM模型占总反射率增强的64%,而同时考虑云 - 表面相互作用的新模型(2LM + CSI)占近80%。我们讨论了在3D云诱导反射率增强中考虑云 - 气溶胶辐射相互作用的可能性,这可能解释了其余20%的增强效应。由于这些是简单模型,这些校正可应用于全球卫星观测(例如MODIS),并有助于减少气溶胶和其他晴空反演中的偏差。

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引用本文的文献

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J Geophys Res Atmos. 2019 Feb 27;124(4):2148-2173. doi: 10.1029/2018jd028989. Epub 2019 Jan 28.

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