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Aircraft measurements of the solar and infrared radiative properties of cirrus and their dependence on ice crystal shape

机译:飞机对卷云的太阳和红外辐射特性及其对冰晶形状的依赖性的测量

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摘要

We present aircraft measurements of the radiative transfer properties of thin cirrus cloud sampled off the east coast of Scotland on November 9, 1995. Downwelling radiances were measured from below the cirrus at 0.87, 1.61, 3.7, 8.55, and 11.0 #mu#m, thereby covering a large range of size parameter and ice refractive index and enabling information on cirrus optical thickness, effective crystal size, and scattering phase function to be deduced. The sensitivity of these quantities to the ice crystal shape assumed in the calculations is examined, and the results are compared with in situ data. We find that a randomized polycrystal shape produces effective sizes that are consistent with the in situ data across all wavelengths considered and performs better in this respect than the other crystal shapes analyzed. However, the optical thicknesses retrieved from the 0.87 #mu#m radiances for this shape are considerably less than those derived from the 11.0 #mu#m data, implying that the phase function at solar wavelengths is in error for this shape over a significant portion of the full scattering angle range. An empirical phase function derived from laboratory measurements produces optical thicknesses which are more consistent with the 11.0 #mu#m and in situ data and matches the angular distribution of scattered radiance more accurately than that calculated using any of the model crystal shapes. The anomalous diffraction approximation is found to produce good agreement with the measurements at 8.55 and 11.0 #mu#m for the crystal sizes relevant to the present case study.
机译:我们提供了1995年11月9日从苏格兰东海岸采样的薄卷云的辐射传递特性的飞机测量值。从卷云下方测量了下行流辐射,分别为0.87、1.61、3.7、8.55和11.0#mu#m,从而涵盖了较大范围的尺寸参数和冰折射率,并能够推断出卷云光学厚度,有效晶体尺寸和散射相位函数的信息。检查了这些量对计算中假定的冰晶形状的敏感性,并将结果与​​现场数据进行了比较。我们发现随机多晶形状产生的有效尺寸与所考虑的所有波长上的原位数据一致,并且在这方面比其他分析的晶体形状更好。但是,从该形状的0.87#mu#m辐射率中检索到的光学厚度比从11.0#μ#m数据得出的光学厚度小得多,这意味着该形状在相当大部分的太阳波长下的相位函数都存在误差整个散射角范围。从实验室测量中得出的经验相位函数产生的光学厚度与11.0#μ#m和原位数据更一致,并且比使用任何模型晶体形状计算出的光学厚度更精确地匹配散射辐射的角度分布。对于与本案例研究有关的晶体尺寸,发现异常衍射近似值与在8.55和11.0#mu#m处的测量值产生了良好的一致性。

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