Electronic crosstalk effect in SNPP VIIRS thermal emissive bands (Conference Presentation)

Junqiang Sun, Menghua Wang
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Abstract

The Visible Infrared Imaging Radiometer Suite (VIIRS) onboard the Suomi National Polar-orbiting Partnership (SNPP) spacecraft has been on orbit for more than five years. Pronounced striping in Earth view (EV) images and obvious discontinuity in the EV brightness temperature (BT) of the thermal emissive bands (TEB) during the blackbody (BB) warm-up cool-down (WUCD) calibration have been found since launch but the root-cause of the phenomena has not yet been identified. Meanwhile, recent studies of the MODerate-resolution Imaging Spectroradiometer (MODIS) long-wave infrared (LWIR) photovoltaic (PV) bands demonstrate that crosstalk effect induces the same erroneous features. In this paper, it is shown that there is, indeed, a remarkable crosstalk contamination in SNPP VIIRS TEB. The crosstalk effect is quantitatively characterized by deriving the crosstalk coefficients from the scheduled lunar observations and the established lunar imagery analysis. Among all SNPP VIIRS TEB, band M14 is shown to have the largest crosstalk contamination from Band M15, while bands M13, M15, M16, and I5 have pronounced crosstalk effect as well. The crosstalk effect is distinctively different for the odd and even detectors within each affected band during to the pattern of the placement of the odd and the even detectors of the band on the focal plane assembly (FPA). The crosstalk coefficients are applied to mitigate the crosstalk effect and the improvements to both the BB calibration and EV retrieval are presented and addressed.
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SNPP VIIRS热辐射带中的电子串扰效应(会议报告)
Suomi国家极轨伙伴关系(SNPP)航天器上的可见红外成像辐射计套件(VIIRS)已经在轨道上运行了五年多。自发射以来,在黑体(BB)预热冷却(WUCD)校准过程中,发现了地球视图(EV)图像明显的条纹和热辐射波段(TEB)的亮度温度(BT)明显的不连续,但其根本原因尚未确定。同时,对中分辨率成像光谱仪(MODIS)长波红外(LWIR)光伏(PV)波段的研究表明,串扰效应也会导致相同的错误特征。在本文中,证明了SNPP VIIRS TEB中确实存在显著的串扰污染。从预定的月球观测和已建立的月球图像分析中导出串扰系数,定量表征了串扰效应。在所有SNPP VIIRS TEB中,M14波段受M15波段的串扰污染最大,而M13、M15、M16和I5波段也有明显的串扰效应。在焦平面组件(FPA)上奇数和偶数探测器的放置方式不同的情况下,每个受影响波段内的奇偶探测器串扰效应明显不同。采用串扰系数来减轻串扰效应,并对BB校准和EV检索进行了改进。
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