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Comparing airborne and satellite retrievals of cloud optical thickness and particle effective radius using a spectral radiance ratio technique: two case studies for cirrus and deep convective clouds

机译:使用光谱辐射比技术比较云光学厚度和颗粒有效半径的空气和卫星检索:两种卷曲和深对流云的案例研究

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Solar radiation reflected by cirrus and deep convective clouds (DCCs) was measured by the Spectral Modular Airborne Radiation Measurement System (SMART) installed on the German High Altitude and Long Range Research Aircraft (HALO) during the Mid-Latitude Cirrus (ML-CIRRUS) and the Aerosol, Cloud, Precipitation, and Radiation Interaction and Dynamic of Convective Clouds System – Cloud Processes of the Main Precipitation Systems in Brazil: A Contribution to Cloud Resolving Modelling and to the Global Precipitation Measurement (ACRIDICON-CHUVA) campaigns. On particular flights, HALO performed measurements closely collocated with overpasses of the Moderate Resolution Imaging Spectroradiometer (MODIS) aboard the Aqua satellite. A cirrus cloud located above liquid water clouds and a DCC topped by an anvil cirrus are analyzed in this paper. Based on the nadir spectral upward radiance measured above the two clouds, the optical thickness τ and particle effective radius reff of the cirrus and DCC are retrieved using a radiance ratio technique, which considers the cloud thermodynamic phase, the vertical profile of cloud microphysical properties, the presence of multilayer clouds, and the heterogeneity of the surface albedo. For the cirrus case, the comparison of τ and reff retrieved on the basis of SMART and MODIS measurements yields a normalized mean absolute deviation of up to 1.2% for τ and 2.1% for reff. For the DCC case, deviations of up to 3.6% for τ and 6.2% for reff are obtained. The larger deviations in the DCC case are mainly attributed to the fast cloud evolution and three-dimensional (3-D) radiative effects. Measurements of spectral upward radiance at near-infrared wavelengths are employed to investigate the vertical profile of reff in the cirrus. The retrieved values of reff are compared with corresponding in situ measurements using a vertical weighting method. Compared to the MODIS observations, measurements of SMART provide more information on the vertical distribution of particle sizes, which allow reconstructing the profile of reff close to the cloud top. The comparison between retrieved and in situ reff yields a normalized mean absolute deviation, which ranges between 1.5 and 10.3%, and a robust correlation coefficient of 0.82.
机译:由Cirrus和深对流云(的DCC)反射的太阳辐射被安装在德国的高海拔和中纬度卷云(ML-CIRRUS)中长距离研究飞机(HALO)的光谱模块化空中辐射测量系统(SMART)测量和气溶胶,云,降水和辐射相互作用和动态流云系统 - 的主要降水系统在巴西的云流程:促进云计算解决建模和全球降水测量(ACRIDICON-CHUVA)活动。在特定的航班,HALO执行与中分辨率成像光谱仪(MODIS)乘坐水上卫星的立交桥密切置测量。位于上述液态水云和一个DCC甲卷云淋上通过砧座Cirrus在本文进行了分析。基于这两个云上述测得的最低点的光谱向上辐射中,Cirrus和DCC的光学厚度τ和颗粒有效半径REFF使用的是辐射率的技术,它参考云热力学相,云微特性的垂直轮廓检索多层云的存在,而表面反射率的异质性。对于卷云情况下,τ和REFF的SMART和MODIS测量的基础上检索到的比较产生高达1.2%为τ和2.1%为REFF的归一化平均绝对偏差。对于DCC情况下,获得了3.6%为τ和6.2%为REFF的偏差。在DCC的情况下较大的偏差主要归因于快速云进化和三维(3-d)的辐射效应。在近红外波长的光谱辐射率向上的测量被用于研究REFF在Cirrus的垂直剖面。 REFF的所检索的值与使用垂直加权方法在原位测量对应比较。相较于MODIS观察,SMART的测量提供了关于颗粒尺寸,其允许重构REFF接近云顶部的轮廓的垂直分布的更多信息。检索之间和原位REFF比较产生一个归一化的平均绝对偏差,其中1.5和10.3%,和0.82稳固的相关性系数之间的范围内。

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