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Shallow cumuli cover and its uncertainties from ground-based lidar–radar data and sky images

机译:浅水泵覆盖及其基于地面激光雷达数据和天空图​​像的不确定性

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Cloud cover estimates of single-layer shallow cumuli obtained from narrow field-of-view (FOV) lidar–radar and wide-FOV total sky imager (TSI) data are compared over an extended period (2000–2017 summers) at the established United States Atmospheric Radiation Measurement mid-continental Southern Great Plains site. We quantify the impacts of two factors on hourly and sub-hourly cloud cover estimates: (1)?instrument-dependent cloud detection and data merging criteria and (2)?FOV configuration. Enhanced observations at this site combine the advantages of the ceilometer, micropulse lidar (MPL) and cloud radar in merged data products. Data collected by these three instruments are used to calculate narrow-FOV cloud fraction (CF) as a temporal fraction of cloudy returns within a given period. Sky images provided by TSI are used to calculate the wide-FOV fractional sky cover (FSC) as a fraction of cloudy pixels within a given image. To assess the impact of the first factor on CF obtained from the merged data products, we consider two additional subperiods (2000–2010 and 2011–2017 summers) that mark significant instrumentation and algorithmic advances in the cloud detection and data merging. We demonstrate that CF obtained from ceilometer data alone and FSC obtained from sky images provide the most similar and consistent cloud cover estimates; hourly bias and root-mean-square difference (RMSD) are within 0.04 and 0.12, respectively. However, CF from merged MPL–ceilometer data provides the largest estimates of the multiyear mean cloud cover, about 0.12 (35 %) and 0.08 (24 %) greater than FSC for the first and second subperiods, respectively. CF from merged ceilometer–MPL–radar data has the strongest subperiod dependence with a bias of 0.08 (24 %) compared to FSC for the first subperiod and shows no bias for the second subperiod. The strong period dependence of CF obtained from the combined ceilometer–MPL–radar data is likely results from a change in what sensors are relied on to detect clouds below 3 km. After 2011, the MPL stopped being used for cloud top height detection below 3 km, leaving the radar as the only sensor used in cloud top height retrievals. To quantify the FOV impact, a narrow-FOV FSC is derived from the TSI images. We demonstrate that FOV configuration does not modify the bias but impacts the RMSD (0.1 hourly, 0.15 sub-hourly). In particular, the FOV impact is significant for sub-hourly observations, where 41 % of narrow- and wide-FOV FSC differ by more than 0.1. A new “quick-look” tool is introduced to visualize impacts of these two factors through integration of CF and FSC data with novel TSI-based images of the spatial variability in cloud cover. The influence of cloud field organization, such cloud streets parallel to the wind direction, on narrow- and wide-FOV cloud cover estimates can be visually assessed.
机译:云盖估计从狭窄的视野(FOV)LIDAR-RADAR和WIDE-FOV总天空成像器(TSI)数据的单层浅Cumuli在综合团结的延长期间(2000-2017夏天)比较了各种大气辐射测量中欧南部大平原网站。我们量化每小时和子小时云覆盖估计的两个因素的影响:(1)?仪器依赖性云检测和数据合并标准和(2)?FOV配置。该站点的增强观测结合了CeIlerometer,微透过LIDAR(MPL)和云雷达在合并数据产品中的优点。由这三种仪器收集的数据用于计算窄FOV云分数(CF),因为在给定时期内的阴天返回的时间分数。 TSI提供的天空图像用于计算宽FOV分数天空盖(FSC)作为给定图像内的阴天像素的一部分。为了评估从合并数据产品获得的第一个因素对CF的影响,我们考虑两个额外的子超影(2000-2010和2011-2017夏天),标志着云检测和数据合并中的显着仪器和算法进步。我们证明,从天空图像获得的CeiLeter数据获得的CF和从天空图像获得的FSC提供了最相似和最相一致的云覆盖估计值;每小时偏差和根平均方差(RMSD)分别在0.04和0.12内。然而,来自合并的MPL-CeiLeometer数据的CF为第一和第二子超过度的分别提供了多年子平均云覆盖的最大估计,大约0.12(35%)和0.08(24%)。合并的Ceiletometer-MPL雷达数据的CF具有最强的子超依赖性,与第一个子超的FSC相比,偏差为0.08(24%),并且对于第二个子优势没有显示偏差。 CF从组合的Ceilometer-MPL雷达数据获得的强时级依赖性可能是由于在依赖的传感器依赖的变化来检测3公里的云。 2011年后,MPL停止用于低于3公里的云顶部高度检测,将雷达作为云顶部高度检索中使用的唯一传感器。为了量化FOV的影响,窄-FOV FSC来自TSI图像。我们证明FOV配置不会修改偏置,但会影响RMSD(0.1小时,0.15次小时)。特别是,FOV的影响对于亚小时观察是显着的,其中41%的窄和宽FOV FSC的差异超过0.1。通过CF和FSC数据与云覆盖的空间变异性的新型TSI图像集成,引入了一种新的“快速外观”工具来可视化这两个因素的影响。可以在视觉评估云场组织的影响,平行于风向的云街平行于风向,可以在狭窄和宽云覆盖估计上进行评估。

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