Polarization sensitivity calibration of the non-polarization channel of polarization multiangle imager onboard Fengyun satellite

Haofei Wang, P. Zhang, Dekui Yin, Jian Shang, Xiuqing Hu, Zhengqiang Li
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Abstract

The polarization instrument of Fengyun-3 precipitation satellite is the first Polarization and Multi-Angle Imager (PMAI) with short-wave infrared channel in China, aiming to accurately measure the radiation characteristics of clouds and aerosols in the atmosphere. The accuracy of radiometric measurement is an important technical index of instrument performance, which is of great significance for the inversion of high-precision quantitative parameters of satellite remote sensing. For the non-polarization channel of a polarization imager, polarization is a kind of interference information, and the polarization sensitivity of the instrument needs to be inverted and quantitatively removed to improve the accuracy of radiation calibration. A method of least squares fitting response value of complete linear polarization incident light based on different polarization angles is proposed to measure the polarization sensitivity of the non-polarization channel full field of view. According to the measured polarization rate of each channel and the polarization characteristics of the incident light, the polarization sensitivity of each channel is calibrated based on the polarization calibration model. The results show that the polarization sensitivity of the non-polarization channel shows obvious edge effect, gradually increasing from the center of the focal plane to the edge, and has obvious spectral differences, the smaller the wavelength having the higher the polarization sensitivity. The maximum polarization sensitivity occurs in the edge field of view of the non-polarization channel in the 1030nm band, close to 1.6%, which has a great impact on the accuracy of radiometric calibration. After polarization sensitivity calibration, the polarization sensitivity of the edge field of view is within 0.5%. The results show that by calibrating the polarization sensitivity of the full field of view of the non-polarization channel, the radiometric calibration can be effectively improved, which provides strong support for high-precision quantitative remote sensing.
风云星偏振多角度成像仪非极化通道偏振灵敏度定标
风云三号降水卫星极化仪是国内首台短波红外偏振多角度成像仪,旨在精确测量大气中云和气溶胶的辐射特性。辐射测量精度是衡量仪器性能的一项重要技术指标,对卫星遥感高精度定量参数的反演具有重要意义。对于偏振成像仪的非偏振通道,偏振是一种干扰信息,需要对仪器的偏振灵敏度进行反向和定量去除,以提高辐射校准的精度。提出了一种基于不同偏振角的完全线偏振入射光响应值的最小二乘拟合方法,用于测量非偏振通道全视场的偏振灵敏度。根据测量到的各通道的偏振率和入射光的偏振特性,基于偏振校准模型对各通道的偏振灵敏度进行校准。结果表明:非极化通道的偏振灵敏度表现出明显的边缘效应,从焦平面中心到边缘逐渐增大,且具有明显的光谱差异,波长越小的偏振灵敏度越高;最大极化灵敏度出现在1030nm波段非极化通道的边缘视场,接近1.6%,对辐射定标精度影响较大。偏振灵敏度标定后,边缘视场的偏振灵敏度在0.5%以内。结果表明,通过标定非极化通道全视场的偏振灵敏度,可以有效地提高辐射定标精度,为高精度定量遥感提供有力支持。
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