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Patterns of Skylight Polarization at Different Atmospheric Conditions

机译:不同大气条件下的天光偏振模式

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A skylight polarization measurement system has been designed,and the measurements of skylight polarized radiance distribution have been performed at different atmospheric conditions. The patterns of skylight polarization measured at four kinds of atmospheric conditions at the spectral range 450~475 nm are presented. It is obvious that qualitatively the patterns of skylight polarization in sunny skies are in agreement with Rayleigh model. The stronger atmospheric turbidity, the greater disturbance to the patterns of skylight polarization appears in the atmosphere. The degree of the skylight polarization P and the angle of the skylight polarization χ are the greatest in the clear sky. However, some meteorologic factors disturb the patterns of skylight polarization more or less. Cloud layer, dust, etc decrease the greatest P and corresponding χ of skylight polarization at different atmospheric conditions. In addition, the cloudy sky has terrible patterns of skylight polarization because it is overclouded and the sunlight is occluded completely.
机译:设计了天光偏振测量系统,并在不同的大气条件下进行了天光偏振辐射分布的测量。给出了在450〜475 nm光谱范围内四种大气条件下测得的天光偏振方向图。很明显,在晴朗的天空上,天窗偏振的定性与瑞利模型一致。大气浊度越强,对大气中天光偏振模式的干扰越大。在晴朗的天空中,天光偏振度P和天光偏振角χ最大。但是,一些气象因素或多或少地干扰了天窗偏振的模式。在不同的大气条件下,云层,尘埃等会降低最大P和相应的天窗偏振χ。此外,多云的天空有阴天的偏振模式,因为它被阴云密布,并且阳光被完全遮挡。

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