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Using radar observations to evaluate 3-D radar echo structure simulated by the Energy Exascale Earth System Model (E3SM) version 1

机译:利用雷达观测评估能量Exascale地球系统模型(E3SM)版本模拟的3-D雷达回波结构

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摘要

The Energy Exascale Earth System Model (E3SM) developedby the Department of Energy has a goal of addressing challenges inunderstanding the global water cycle. Success depends on correct simulationof cloud and precipitation elements. However, lack of appropriate evaluationmetrics has hindered the accurate representation of these elements ingeneral circulation models. We derive metrics from the three-dimensionaldata of the ground-based Next-Generation Radar (NEXRAD) network over theUS to evaluate both horizontal and vertical structures of precipitationelements. We coarsened the resolution of the radar observations to beconsistent with the model resolution and improved the coupling of the CloudFeedback Model Intercomparison Project Observation Simulator Package (COSP)and E3SM Atmospheric Model Version 1 (EAMv1) to obtain the best possiblemodel output for comparison with the observations. Three warm seasons(2014–2016) of EAMv1 simulations of 3-D radar reflectivity features at anhourly scale are evaluated. A general agreement in domain-mean radarreflectivity intensity is found between EAMv1 and NEXRAD below 4 kmaltitude; however, the model underestimates reflectivity over the centralUS, which suggests that the model does not capture the mesoscaleconvective systems that produce much of the precipitation in that region. Theshape of the model-estimated histogram of subgrid-scale reflectivity isimproved by correcting the microphysical assumptions in COSP. Different fromprevious studies that evaluated modeled cloud top height, we find the modelseverely underestimates radar reflectivity at upper levels – the simulatedecho top height is about 5 km lower than in observations – and this resultis not changed by tuning any single physics parameter. For more accuratemodel evaluation, a higher-order consistency between the COSP and the hostmodel is warranted in future studies.
机译:能源部发达的能源EvaStale地球系统模型(E3SM)的目标是解决违反全球水循环的挑战。成功取决于云和降水元素的正确模拟。然而,缺乏适当的评估莫特尔可以阻碍了这些元素含有肉类循环模型的准确表示。我们从基于地面的下一代雷达(NEXRAD)网络的三维DATA从函数中获得指标,以评估沉淀性的水平和垂直结构。我们粗略分辨雷达观测到模型分辨率,并改善了CloudFeedback模型相互比较项目观察模拟器包(COSP)和E3SM大气模型版本1(EADV1)的耦合,以获得与观察结果相比的最佳POSSIBLEMODEL输出。评估了三个温暖的季节(2014-2016)的eamv1模拟3d radar反射率特征,在无氧尺度下进行。在低于4的Eamv1和Nexrad之间发现了域名式radArteflectivity强度的一般协议;然而,该模型低估了中心的反射率,这表明该模型不会捕获在该区域中产生大部分沉淀的MesoscaleConvective系统。通过校正COSP中的微神科假设来实现亚级尺度反射率模型估计直方图的图表。不同于评估所模型的云顶部高度的Pruvious研究,我们发现型号在上层的雷达反射率 - SimulateCho顶部高度约为5km,比观察中的约5公里 - 并且通过调整任何单个物理参数不会改变这一结果。为了更具准确性评估,在未来的研究中有必要在COSP和Hostmodel之间进行更高级的一致性。

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