Chen Xing-Feng, Gu Xing-Fa, Cheng Tian-Hai, Li Zheng-Qiang, Yu Tao, Xie Dong-Hai
State Key Laboratory of Remote Sensing Science, Institute of Remote Sensing Applications, Chinese Academy of Sciences, Beijing 100101, China.
Guang Pu Xue Yu Guang Pu Fen Xi. 2011 Jun;31(6):1648-53.
The sea surface sunglint is caused by specular reflectance. Water is a kind of dark target with a very low reflectance, so sunglint becomes a big noise in the aerial or aerospace remote sensing images; sunglint is strongly polarized, and can be a natural standard light source for polarized sensor in-flight calibration; sunglint also can be utilized to retrieve gaseous constituents and aerosol properties. For both de-noising and being standard light source, the radiative physic parameters should be calculated accurately. First, A 3-D sea surface model was constituted according to the Cox & Munk model; Second, the polarized radiative model of sunglint was deduced based on the 3-D sea surface model and polarized Fresnel reflectance law; Third, the sensitivities of solar-viewing relative azimuth, zenith, wind speed and wind direction were analyzed utilizing the polarized radiative model. The polarization characteristics analysis of sunglint provides a theoretical basis for the quantitative remote sensing retrievals which uses sunglint.
海面耀光是由镜面反射引起的。水是一种反射率很低的暗目标,因此在航空或航天遥感图像中,海面耀光成为一种很大的噪声;海面耀光具有很强的偏振性,可作为偏振传感器飞行校准的自然标准光源;海面耀光还可用于反演气态成分和气溶胶特性。为了去噪和作为标准光源,需要准确计算辐射物理参数。首先,根据考克斯-芒克模型构建了三维海面模型;其次,基于三维海面模型和偏振菲涅尔反射定律推导了海面耀光的偏振辐射模型;第三,利用偏振辐射模型分析了太阳观测相对方位角、天顶角、风速和风向的敏感性。海面耀光的偏振特性分析为利用海面耀光进行定量遥感反演提供了理论依据。