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Optical properties of pristine ice crystals in mid-latitude cirrus clouds: a case study during CIRCLE-2 experiment

机译:中纬卷云中原始冰晶的光学性质:以CIRCLE-2实验为例

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摘要

In this paper, we describe in situ observations of mid-latitude cirrus cloud band carried out on 16 May 2007 during the CIRCLE-2 experiment. The Polar Nephelometer and the Cloud Particle Imager (CPI) instruments with PMS FSSP-300 and 2D-C probes were used for the description of the optical and microphysical cloud properties. Two selected cloud regions are compared and discussed in detail. Significant differences in optical properties are evidenced in terms of 22�° halo occurrences even though prevalent planar-plate ice crystals are observed in both cloud regions. Featureless scattering phase functions are measured in the first cloud region located near the trailing edge of the cirrus-band at about 11 800 m/â��57 �°C. In contrast, well pronounced 22�° halo peaks are observed with predominant similar-shaped ice crystals near the cirrus-band leading edge at 7100 m/â��27 �°C. CPI ice crystal images with Polar Nephelometer observations are carefully analysed and interpreted from a theoretical light scattering model in order to explain occurrence and non-occurrence of the 22�° halo feature. The results highlight that the halo peaks are inherent only in perfect plate ice crystals (or pristine crystals). On the basis of previous datasets in mid-latitude cirrus, it is found that simple pristine crystals are uncommon whereas particles with imperfect or complex shapes are prevalent. As a result, phase functions that are smooth and featureless best represent cirrus scattering properties.
机译:在本文中,我们描述了在2007年5月16日CIRCLE-2实验期间对中纬度卷云带进行的原位观测。极性浊度仪和带有PMS FSSP-300和2D-C探针的云粒子成像仪(CPI)仪器用于描述云和微物理性质。比较并讨论了两个选定的云区域。即使在两个云区域都观察到普遍的平板冰晶,光学性质的显着差异也被证明是在22°光晕发生方面。无特征散射相位函数在卷云带后缘附近的第一个云区域中以大约11 800 m /°C-57°C进行测量。相比之下,在7100 m /°C-27°C处,卷云带前缘附近的主要相似形状的冰晶中,观察到了明显的22°晕峰。极地浊度计观测到的CPI冰晶图像经过仔细分析并从理论上的光散射模型进行了解释,以解释22°光晕特征的发生和不发生。结果突出表明,仅在完美的板状冰晶(或原始晶体)中固有有晕圈峰。根据中纬度卷云的先前数据集,发现简单的原始晶体并不常见,而具有不完善或复杂形状的颗粒则很普遍。结果,光滑且无特征的相位函数最能代表卷云散射特性。

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