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Evaluation of gridded scanning ARM cloud radar reflectivity observations and vertical doppler velocity retrievals

机译:网格化扫描ARM云雷达反射率观测和垂直多普勒速度反演的评估

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摘要

The scanning Atmospheric Radiation Measurement (ARM) cloud radars (SACRs)provide continuous atmospheric observations aspiring to capture the 3-Dcloud-scale structure. Sampling clouds in 3-D is challenging due to theirtemporal–spatial scales, the need to sample the sky at high elevations andcloud radar limitations. Thus, a suggested scan strategy is to repetitivelyslice the atmosphere from horizon to horizon as clouds advect over the radar(Cross-Wind Range-Height Indicator – CW-RHI). Here, the processing andgridding of the SACR CW-RHI scans are presented. First, the SACR sampleobservations from the ARM Southern Great Plains and Cape Cod sites arepost-processed (detection mask, gaseous attenuation correction, insectfiltering and velocity de-aliasing). The resulting radial Doppler momentfields are then mapped to Cartesian coordinates with time as one of thedimensions. Next the Cartesian-gridded Doppler velocity fields are decomposedinto the horizontal wind velocity contribution and the vertical Dopplervelocity component. For validation purposes, all gridded and retrieved fieldsare compared to collocated zenith-pointing ARM cloud radar measurements. Weconsider that the SACR sensitivity loss with range, the cloud type observedand the research purpose should be considered in determining the griddeddomain size. Our results also demonstrate that the gridded SACR observationsresolve the main features of low and high stratiform clouds. It isestablished that the CW-RHI observations complemented with processingtechniques could lead to robust 3-D cloud dynamical representations up to25–30 degrees off zenith. The proposed gridded products are expected toadvance our understanding of 3-D cloud morphology, dynamics and anisotropyand lead to more realistic 3-D radiative transfer calculations.
机译:扫描式大气辐射测量(ARM)云雷达(SACR)可提供连续的大气观测,以期捕获3-Dcloud尺度的结构。由于3D云的时空尺度,在高海拔地区对天空进行采样的需求以及云雷达的局限性,因此对3D云进行采样具有挑战性。因此,建议的扫描策略是在云层在雷达上方平移时,将大气层从地平线到地平线重复分割(横风范围高度指示器– CW-RHI)。在此,介绍了SACR CW-RHI扫描的处理和网格化。首先,对来自ARM南部大平原和鳕鱼角站点的SACR样本进行后处理(检测面罩,气体衰减校正,昆虫滤除和速度去混叠)。然后将所得的径向多普勒矩场映射为时间为维度之一的笛卡尔坐标。接下来,将笛卡尔网格多普勒速度场分解为水平风速贡献和垂直多普勒速度分量。为了进行验证,将所有网格化和检索到的场与并置的指向天顶的ARM云雷达测量值进行比较。我们认为,在确定网格化域的大小时,应考虑SACR灵敏度随范围,云类型和研究目的的损失。我们的结果还表明,网格化的SACR观测结果解决了低层和高层云的主要特征。可以确定的是,CW-RHI观测值与处理技术的补充可能会导致在距天顶25-30度的范围内进行可靠的3-D云动力学表示。拟议的网格化产品有望增进我们对3-D云形态,动力学和各向异性的理解,并导致更加逼真的3-D辐射传输计算。

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