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东海海域的天空光偏振及子午线研究 被引量:3

Sky Light Polarization and Meridian in East China Sea
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摘要 基于瑞利散射理论,对天空光偏振分布模式进行了仿真。利用图像式全天空偏振模式测试系统对东海海域的天空光偏振分布模式进行了测试。提出了一种利用偏振方位角信息判断子午线的方法。研究结果表明,当太阳高度角大于85°或低于25°时,可利用偏振方位角定位子午线方向。该子午线方向与理论仿真结果一致。 Based On the Rayleigh scattering theory, the distribution pattern of the sky light polarization is simulated. The distribution pattern of the sky light polarization in the East China Sea is tested by the photographic full-sky polarization pattern testing system. A method for determining the meridian by the polarization azimuthal angle information is proposed. The research results show that, when the solar altitude angle is larger than 85° or less than 25°, the meridian direction can be positioned by means of the polarization azimuthal angle. The meridian direction is consistent with the theoretical simulation result.
作者 崔岩 谢楠 张西光 周鑫昌 褚金奎 关乐 Cui Yan1 Xie Nan1, Zhang Xiguang1, Zhou Xinchang1, Chu Jinkui1, Guan Le2(1 Key Laboratory for Precision & Non-Traditional Machining of Ministry of Education, Dalian University of Technology, Dalian, Liaoning 116024, China; 2Key Laboratory for Micro/Nano Technology and System of Liaoning Province, Dalian University of Technology Dalian, Liaoning 116024, China)
出处 《激光与光电子学进展》 CSCD 北大核心 2018年第10期374-380,共7页 Laser & Optoelectronics Progress
基金 国家自然科学基金(51675076)
关键词 散射 大气光学 偏振模式 海上测试 子午线 太阳高度角 scattering atmospheric optics polarization mode sea test meridian solar altitude angle
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