首页> 外文期刊>Journal of Applied Meteorology and Climatology >The Microwave Radiative Properties of Falling Snow Derived from Nonspherical Ice Particle Models. Part II: Initial Testing Using Radar, Radiometer and In Situ Observations
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The Microwave Radiative Properties of Falling Snow Derived from Nonspherical Ice Particle Models. Part II: Initial Testing Using Radar, Radiometer and In Situ Observations

机译:非球形冰粒模型推导的落雪的微波辐射特性。第二部分:使用雷达,辐射计和原位观测的初始测试

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In this study, two different particle models describing the structure and electromagnetic properties of snow are developed and evaluated for potential use in satellite combined radar-radiometer precipitation estimation algorithms. In the first model, snow particles are assumed to be homogeneous ice-air spheres with single scattering properties derived from Mie theory. In the second model, snow particles are created by simulating the self-collection of pristine ice crystals into aggregate particles of different sizes, using different numbers and habits of the collected component crystals. Single-scattering properties of the resulting nonspherical snow particles are determined using the discrete dipole approximation. The size-distribution-integrated scattering properties of the spherical and nonspherical snow particles are incorporated into a dual-wavelength radar profiling algorithm that is applied to 14- and 34-GHz observations of stratiform precipitation from the ER-2 aircraftborne High-Altitude Imaging Wind and Rain Airborne Profiler (HIWRAP) radar. The retrieved ice precipitation profiles are then input to a forward radiative transfer calculation in an attempt to simulate coincident radiance observations from the Conical Scanning Millimeter-Wave Imaging Radiometer (CoSMIR). Much greater consistency between the simulated and observed CoSMIR radiances is obtained using estimated profiles that are based upon the nonspherical crystal/aggregate snow particle model. Despite this greater consistency, there remain some discrepancies between the higher moments of the HIWRAP-retrieved precipitation size distributions and in situ distributions derived from microphysics probe observations obtained from Citation aircraft underflights of the ER-2. These discrepancies can only be eliminated if a subset of lower-density crystal/aggregate snow particles is assumed in the radar algorithm and in the interpretation of the in situ data.
机译:在这项研究中,开发了两种不同的描述雪结构和电磁特性的粒子模型,并对其进行了评估,可用于卫星组合雷达-辐射仪降水估算算法。在第一个模型中,假定雪粒子是具有均一散射特性的均质冰空气球,该散射特性是根据Mie理论得出的。在第二个模型中,通过使用不同数量和习性收集的成分晶体,将原始冰晶的自我收集模拟为不同大小的聚集颗粒,从而创建了雪粒。使用离散偶极近似法确定所得非球形雪粒的单散射特性。球形和非球形雪粒的尺寸分布积分散射特性被合并到双波长雷达轮廓分析算法中,该算法应用于ER-2机载高空成像风的层状降水的14和34 GHz观测和Rain Airborne Profiler(HIWRAP)雷达。然后,将检索到的冰降水廓线输入到正向辐射传递计算中,以尝试模拟来自圆锥形扫描毫米波成像辐射计(CoSMIR)的一致辐射观测。使用基于非球面晶体/聚集雪粒模型的估计剖面,可以得到模拟的CoSMIR辐射与观察到的CoSMIR辐射之间更大的一致性。尽管具有更大的一致性,但从HI-2获得的HIWRAP降水量大小分布的较高矩与从ER-2的Citation飞机飞行中获得的微观物理探针观测结果得出的原位分布之间仍存在一些差异。仅当在雷达算法和原位数据解释中假设使用低密度晶体/聚集雪粒子集时,才能消除这些差异。

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