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偏振光大气传输的前向散射新模型

马丽珍 史鹏 张闻钊 顾永建

马丽珍, 史鹏, 张闻钊, 顾永建. 偏振光大气传输的前向散射新模型[J]. 应用光学, 2010, 31(3): 503-507.
引用本文: 马丽珍, 史鹏, 张闻钊, 顾永建. 偏振光大气传输的前向散射新模型[J]. 应用光学, 2010, 31(3): 503-507.
MA Li-zhen, SHI Peng, ZHANG Wen-zhao, GU Yong-jian. New forward scattering model for polarized light propagating in atmosphere[J]. Journal of Applied Optics, 2010, 31(3): 503-507.
Citation: MA Li-zhen, SHI Peng, ZHANG Wen-zhao, GU Yong-jian. New forward scattering model for polarized light propagating in atmosphere[J]. Journal of Applied Optics, 2010, 31(3): 503-507.

偏振光大气传输的前向散射新模型

详细信息
    通讯作者:

    马丽珍(1973-),女,甘肃定西人,博士研究生,讲师,主要从事空间光学方面的研究工作。

  • 中图分类号: TN926;O436

New forward scattering model for polarized light propagating in atmosphere

  • 摘要: 建立了偏振光空间传输前向散射的物理模型。对各向同性散射介质,在非相干性假设条件下,导出了偏振光双散射和多散射前向散射的有效Mueller矩阵,给出了偏振光Mie散射前向有效Mueller矩阵各矩阵元之间的对称性关系,即Mueller矩阵的16个矩阵元中只有7个是独立的,其他9个矩阵元通过组合及一定角度的旋转即可得到。利用Monte Carol方法模拟了偏振光在空间传输10 km的前向散射的有效Mueller矩阵,模拟结果表明各矩阵元存在一定的对称性关系,与基于本模型导出的偏振光前向散射的有效Mueller矩阵元具有较好的一致性。
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  • 刊出日期:  2010-05-15

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