SNPP virs在轨三年后的热辐射波段性能

E. Haas, D. Moyer, G. Moy, F. D. Luccia, D. Kunkee
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引用次数: 2

摘要

Suomi国家极轨伙伴关系(SNPP)航天器的主要传感器是于2011年10月28日发射的可见光-红外成像辐射计套件(VIIRS)。它共有22个波段,其中7个热发射波段(TEBs),一个高动态范围单色昼夜波段(DNB)和14个反射太阳波段(RSBs)。利用机载校准黑体(OBCBB)作为热源在轨道上跟踪TEB增益和噪声性能。teb查看OBCBB每次扫描允许增益校正大约每1.7秒。F因子(与增益成反比)和噪声等效δ温度(NEdT)的长期趋势可以评估TEB热模型的稳定性和不确定性。本文将讨论热模式不确定性对红外热像仪校准的影响,以及这些不确定性如何影响红外热像仪的长期性能。它还将显示teb在轨道上运行3年以上的稳定性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
SNPP VIIRS thermal emissive band performance after three years on-orbit
The Suomi National Polar-orbiting Partnership (SNPP) spacecraft's primary sensor is the Visible-Infrared Imaging Radiometer Suite (VIIRS) which launched on October 28, 2011. It has 22 total bands with 7 thermal emissive bands (TEBs), a high dynamic range monochromatic Day Night Band (DNB) and 14 reflective solar bands (RSBs). The TEB gain and noise performance is tracked on-orbit using an On-Board Calibrator BlackBody (OBCBB) as a thermal source. The TEBs view the OBCBB every scan allowing gain correction roughly every 1.7 seconds. Long term trending of the F factor (inversely proportional to gain) and Noise Equivalent delta Temperature (NEdT) allows the stability and uncertainty in the TEB thermal model to be evaluated. This paper will discuss the impacts of the thermal model uncertainties on the VIIRS calibration and how those impact the long term performance of VIIRS. It will also show the stability of the TEBs over 3 years on-orbit.
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