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Constraining mass-diameter relations from hydrometeor images and cloud radar reflectivities in tropical continental and oceanic convective anvils

机译:在热带大陆和海洋对流砧中,从水文气象图和云雷达反射率约束质量直径关系

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In this study the density of ice hydrometeors in tropical clouds is derived from a combined analysis of particle images from 2-D-array probes and associated reflectivities measured with a Doppler cloud radar on the same research aircraft. Usually, the mass-diameter m(D) relationship is formulated as a power law with two unknown coefficients (pre-factor, exponent) that need to be constrained from complementary information on hydrometeors, where absolute ice density measurement methods do not apply. Here, at first an extended theoretical study of numerous hydrometeor shapes simulated in 3-D and arbitrarily projected on a 2-D plan allowed to constrain the exponent beta of the m(D) relationship from the exponent sigma of the surface-diameter S(D) relationship, which is likewise written as a power law. Since S(D) always can be determined for real data from 2-D optical array probes or other particle imagers, the evolution of the m(D) exponent can be calculated. After that, the pre-factor alpha of m(D) is constrained from theoretical simulations of the radar reflectivities matching the measured reflectivities along the aircraft trajectory.
机译:在这项研究中,热带云中冰水凝结物的密度来自对二维阵列探测器的粒子图像和在同一研究飞机上用多普勒云雷达测量的相关反射率的组合分析。通常,质量直径m(D)关系被公式化为幂律,具有两个未知系数(预因子,指数),需要从水凝物的补充信息中加以限制,而绝对冰密度测量方法则不适用。在这里,首先,对在3D模式下模拟并任意投影在2D平面上的多种水凝流星形状进行了扩展的理论研究,从而可以根据表面直径S(s( D)关系,它同样被写为幂律。由于始终可以为来自二维光学阵列探头或其他粒子成像仪的真实数据确定S(D),因此可以计算m(D)指数的演变。此后,m(D)的因数alpha受雷达反射率理论模拟的约束,该理论与沿飞机轨迹测得的反射率匹配。

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