Hegedüs Ramón, Akesson Susanne, Horváth Gábor
Biooptics Laboratory, Department Of Biological Physics, Physical Institute, Eötvös University, Budapest, Hungary.
J Opt Soc Am A Opt Image Sci Vis. 2007 Aug;24(8):2347-56. doi: 10.1364/josaa.24.002347.
The distribution of polarization in the overcast sky has been practically unknown. Earlier the polarization of light from heavily overcast skies (when the Sun's disc was invisible) has been measured only sporadically in some celestial points by point-source polarimetry. What kind of patterns of the degree p and angle alpha of linear polarization of light could develop after transmission through a thick layer of ice or water clouds? To answer this question, we measured the p and alpha patterns of numerous totally overcast skies on the Arctic Ocean and in Hungary by full-sky imaging polarimetry. We present here our finding that depending on the optical thickness of the cloud layer, the pattern of alpha of light transmitted through the ice or water clouds of totally overcast skies is qualitatively the same as the alpha pattern of the clear sky. Under overcast conditions the value of alpha is determined predominantly by scattering on cloud particles themselves. Nevertheless, the degrees of linear polarization of light from overcast skies were rather low (p<or=16%). Our results obtained under overcast conditions complete the earlier findings that the alpha pattern of the clear sky also appears in partly cloudy, foggy, and smoky skies. Our results show that the celestial distribution of the direction of polarization is a very robust pattern being qualitatively always the same under all possible sky conditions. This is of great importance for the orientation of polarization-sensitive animals based on sky polarization under conditions when the Sun is not visible.
阴天天空中偏振的分布实际上一直不为人知。早些时候,对于浓云密布的天空(太阳圆盘不可见时)的光偏振,仅通过点源偏振测量法在一些天体点进行过零星测量。光通过厚厚的冰层或水云层后,线性偏振的程度p和角度α会呈现出什么样的模式呢?为了回答这个问题,我们通过全天空成像偏振测量法,在北冰洋和匈牙利测量了众多完全阴天天空的p和α模式。我们在此展示我们的发现:取决于云层的光学厚度,完全阴天天空的光透过冰层或水云层后的α模式,在定性上与晴朗天空的α模式相同。在阴天条件下,α值主要由云层粒子本身的散射决定。然而,阴天天空的光的线性偏振程度相当低(p≤16%)。我们在阴天条件下获得的结果完善了早期的发现,即晴朗天空的α模式也出现在部分多云、有雾和有烟雾的天空中。我们的结果表明,偏振方向的天体分布是一种非常稳定的模式,在所有可能的天空条件下,定性上总是相同的。这对于在太阳不可见的条件下基于天空偏振的偏振敏感动物的定向非常重要。