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Results and Lessons Learned from MODIS Polarization Sensitivity Characterization

机译:从MODIS极化灵敏度表征中学到的结果和经验教训

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In addition to radiometric, spatial, and spectral calibration requirements, MODIS design specifications include polarization sensitivity requirements of less than 2% for all Reflective Solar Bands (RSB) except for the band centered at 412nm. To the best of our knowledge, MODIS was the first imaging radiometer that went through comprehensive system level (end-to-end) polarization characterization. MODIS polarization sensitivity was measured pre-launch at a number of sensor view angles using a laboratory Polarization Source Assembly (PSA) that consists of a rotatable source, a polarizer (Ahrens prism design), and a collimator. This paper describes MODIS polarization characterization approaches used by MODIS Characterization Support Team (MCST) at NASA/GSFC and addresses issues and concerns in the measurements. Results (polarization factor and phase angle) using different analyzing methods are discussed. Also included in this paper is a polarization characterization comparison between Terra and Aqua MODIS. Our previous and recent analysis of MODIS RSB polarization sensitivity could provide useful information for future Earth-observing sensor design, development, and characterization.
机译:除了辐射,空间和光谱校准要求外,MODIS设计规范还要求所有反射性太阳波段(RSB)的偏振敏感度要求均低于2%,但以412nm为中心的波段除外。据我们所知,MODIS是第一台通过全面的系统级(端到端)偏振特性表征的成像辐射仪。使用由可旋转光源,偏振器(Ahrens棱镜设计)和准直仪组成的实验室偏振源组件(PSA),在多个传感器视角启动前测量MODIS偏振灵敏度。本文介绍了NASA / GSFC的MODIS特征支持小组(MCST)使用的MODIS偏振特征描述方法,并解决了测量中的问题和关注。讨论了使用不同分析方法得出的结果(极化因子和相角)。本文还包括Terra与Aqua MODIS之间的极化特性比较。我们之前和最近对MODIS RSB极化灵敏度的分析可以为将来的地球观测传感器设计,开发和表征提供有用的信息。

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