| 太阳天顶角对反演高光谱地表反射率影响分析 |
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| 引用本文： | 杜沈达,张运杰,韦玮,黄冬,李新,郑小兵.太阳天顶角对反演高光谱地表反射率影响分析[J].光学学报,2021,41(2):182-188. |
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| 作者姓名： | 杜沈达 张运杰 韦玮 黄冬 李新 郑小兵 |
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| 作者单位： | 中国科学院合肥物质科学研究院安徽光学精密机械研究所,安徽合肥230031;中国科学技术大学,安徽合肥230026;中国科学院通用光学定标与表征技术重点实验室,安徽合肥230031;中国科学院合肥物质科学研究院安徽光学精密机械研究所,安徽合肥230031;中国科学院通用光学定标与表征技术重点实验室,安徽合肥230031 |
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| 基金项目： | 国家重点研发计划(2018YFB0504900,2018YFB0504905);中国科学院合肥物质科学研究院院长基金(YZJJ2019QN5);安徽省自然科学基金青年项目(1908085QD158)。 |
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| 摘 要： | 为了满足星上载荷高频次的在轨定标需求,常使用场地自动化定标技术将多光谱反射率反演为高光谱反射率,所以提升光谱的反演精度对提高自动化定标精度尤为重要。使用布设在敦煌辐射校正场的通道式自动化观测仪器计算从2018年9月至2019年9月的反射率;根据测量过程中太阳天顶角的不同将数据分为6组,并使用双向反射分布函数模型对不同太阳天顶角下的光谱形状进行一致性分析。实验结果表明,双向反射分布函数模型校正不同入射角度是有效的。
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| 关 键 词： | 散射 自动化观测 太阳天顶角 地表反射率 相似度 光谱反演 双向分布函数 |
Analysis of Influence of Solar Zenith Angle on Reconstruction of Hyperspectral Surface Reflectance |
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| Du Shenda,Zhang Yunjie,Wei Wei,Huang Dong,Li Xin,Zheng Xiaobing.Analysis of Influence of Solar Zenith Angle on Reconstruction of Hyperspectral Surface Reflectance[J].Acta Optica Sinica,2021,41(2):182-188. |
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| Authors: | Du Shenda Zhang Yunjie Wei Wei Huang Dong Li Xin Zheng Xiaobing |
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| Institution: | (Anhui Institute of Optics and Fine Mechanics,Hefei Institutes of Physical Science,Chinese Academy of Sciences,Hefei,Anhui 230031,China;University of Science and Technology of China,Hefei,Anhui 230026,China;Key Laboratory of Optical Calibration and Characterization,Chinese Academy of Sciences,Hefei,Anhui 230031,China) |
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| Abstract: | In order to meet the high-frequency on-orbit calibration requirements of the on-board load,the site automatic calibration technology is often used to invert the multi-spectral reflectance into the hyper spectral reflectance,so it is particularly important to improve the precision of automatic calibration to improve the inversion accuracy of spectrum.In this paper,we calculate the reflectance from September 2018 to September 2019 using a channel-type automated observation instrument deployed in the Dunhuang radiometric calibration site.Furthermore,we divide the data into 6 groups according to the difference in the solar zenith angles during the measurement process and employ the model of bidirectional reflectance distribution function(BRDF)for the consistency analysis of spectral shapes at different solar zenith angles.The experimental results show that the BRDF model is effective for correcting the data at different incident angles. |
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| Keywords: | scattering automated observation solar zenith angle surface reflectance similarity spectral reconstruction bidirectional reflectance distribution function |
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