首页> 外文会议>Proceedings of the Tiangong-2 remote sensing application conference: technology, method and application >Cross-Calibration of S-NPP/VIIRS and Tiangong-2/MAI Visible Channels Using the SNO Method
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Cross-Calibration of S-NPP/VIIRS and Tiangong-2/MAI Visible Channels Using the SNO Method

机译:使用SNO方法交叉校准S-NPP / VIIRS和天宫2 / MAI可见通道

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The space laboratory "Tiangong-2" (TG-2) was launched on 15 September 2016. The Multi-Angle Polarization Imager (MAI), onboard TG-2, is the first visible and near-infrared multi-angle polarization imager developed in China. MAI can accomplish polarization observation from up to 14 different viewing angles, which is of great significance for relevant research on the microphysical characteristics of clouds and aerosols. Aimed at the problem of a lack of an onboard calibration device for MAI, to correct TG-2's calibration coefficients in time, the Simultaneous Nadir Overpass (SNO) cross-calibration method is proposed as a reasonable and feasible method for MAI 565- and 670-nm channels. Data from the M4 and M5 channels of the Visible Infrared Imaging Radiometer Suite (VIIRS), with good calibration accuracy, are used as reference data, and a series of matching conditions and a spectral adjustment algorithm are specified. To apply the SNO method, eight groups of examples from December 2016 to February 2017 are selected, and a large number of matching pixel samples covering land, ocean surface, and cloud layers are obtained. The resulting cross-calibration curves between MAI 565-nm and VIIRS M4 channels, and between MAI 670-nm and VIIRS M5 channels, show correlation coefficients of reflectivity of 0.986 and 0.994, mean biases of 2.48% and 5.90%, and RMSEs of 3.56% and 6.95%, respectively. Overall, the cross-calibration method achieved good results, which are of reference significance to correct the laboratory calibration coefficient of MAI. The proposed method effectively solves the problems of MAI's subsequent on-orbit monitoring and vicarious calibration, and also lays a foundation for later applications of MAI data in research on cloud and aerosol microphysical parameters.
机译:航天实验室“天宫二号”(TG-2)于2016年9月15日发射升空。TG-2上的多角度偏振成像仪(MAI)是第一台可见和近红外多角度偏振成像仪。在中国开发。 MAI可以从多达14个不同的视角完成偏振观测,这对云和气溶胶微物理特性的相关研究具有重要意义。针对缺少用于MAI的机载校准装置的问题,以及时校正TG-2的校准系数,提出了同时最低点立交(SNO)交叉校准方法作为MAI 565-和670的一种合理可行的方法。 -nm通道。来自可见红外成像辐射计套件(VIIRS)的M4和M5通道的数据具有良好的校准精度,被用作参考数据,并指定了一系列匹配条件和光谱调整算法。为了应用SNO方法,选择了2016年12月至2017年2月的八组示例,并获得了覆盖陆地,海洋表面和云层的大量匹配像素样本。 MAI 565-nm和VIIRS M4通道之间以及MAI 670-nm和VIIRS M5通道之间的交叉校准曲线显示反射率的相关系数为0.986和0.994,平均偏差为2.48%和5.90%,RMSE为3.56 %和6.95%。总体而言,交叉校正法取得了良好的效果,对校正MAI的实验室校正系数具有参考意义。该方法有效地解决了MAI的后续在轨监测和替代定标问题,为以后MAI数据在云和气溶胶微物理参数研究中的应用奠定了基础。

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