首页> 外文会议>Atmospheric Optics: Models, Measurements, and Target-in-the-Loop Propagation; Proceedings of SPIE-The International Society for Optical Engineering; vol.6708 >Intensity and polarization characteristics of the light scattered by the ice crystals of cirrus clouds with preferred orientations
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Intensity and polarization characteristics of the light scattered by the ice crystals of cirrus clouds with preferred orientations

机译:卷云冰晶散射光的强度和偏振特性

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Knowledge of optical properties of ice crystal particles of cirrus clouds is a challenging problem of atmospheric optics. Cirrus clouds cover, in average, 20%-30% of Earth's surface that leads to their essential impact of climate. Therefore these optical properties are needed for incorporation in up-to-date models of Earth's radiation budget and, consequently, they should be used in numerical models of climate prediction or climate change. The optical properties of ice crystal particles have been calculated for recent 20-30 years by a lot of authors under an assumption of 3-D orientation. However, the crystals often reveal a tendency to be oriented in the horizontal plane because of aerodynamic laws. Phase functions for light scattering by horizontally and preferably oriented hexagonal ice plates and columns are numerically calculated within the framework of geometric optics. The main quantitative properties of the halos (sundog, parhelion 120°, suncave Parry arc, sunvex Parry arc, and others) are obtained for a number of both incident light directions and aspect ratios of the plates arid columns respectively. A parameterization of the phase functions in the parhelic, subparhelic and circumzenithal (circumhorizonthal) circles for the plates and all scattered energy for the columns are proposed based on the integral contributions of the narrow angular peaks (halos) that are tabulated as the weight coefficients. Our results can be used for atmospheric lidarobservation for determining of size, shape distributions of the ice crystals particles in cirrus clouds. A method for retrieving aspect ratios of the plates by means of polarization measurements is discussed.
机译:卷云冰晶颗粒的光学特性的知识是大气光学的一个难题。卷云平均覆盖地球表面的20%-30%,这导致了它们对气候的本质影响。因此,将这些光学特性整合到地球辐射预算的最新模型中是必需的,因此,应将它们用于气候预测或气候变化的数值模型中。许多作者在3-D取向的假设下,最近20-30年已计算出冰晶颗粒的光学性质。然而,由于空气动力学定律,晶体常常显示出在水平面中取向的趋势。在几何光学的框架内,通过数值计算水平和优选定向的六边形冰盘和圆柱体进行光散射的相位函数。分别从多个入射光方向和板和柱的长宽比获得光环的主要定量特性(sundog,parhelion 120°,suncave Parry弧,sunvex Parry弧等)。根据窄角峰(光晕)的积分贡献,提出了板的平行,副平行和周向(周向)圆中的相函数的参数化,以及列的所有散射能量的表述,这些积分被作为权重系数制成表格。我们的结果可用于大气盖层观测,以确定卷云中冰晶颗粒的大小,形状分布。讨论了一种通过偏振测量来获取板的纵横比的方法。

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