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SeaWiFS Long-Term Solar Diffuser Reflectance Trend Analysis

机译:SeaWiFS长期太阳漫射器反射率趋势分析

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The NASA Ocean Biology Processing Group's Calibration and Validation (Cal/Val) Team implemented daily solar calibrations of SeaWiFS to look for step-function changes in the instrument response and has used these calibrations to supplement the monthly lunar calibrations in monitoring the radiometric stability of SeaWiFS during its first year of on-orbit operations. The Team has undertaken an analysis of the mission-long solar calibration time series, with the lunar-derived radiometric corrections over time applied, to assess the long-term degradation of the solar diffuser reflectance over nine years on orbit. The SeaWiFS diffuser is an aluminum plate coated with YB71 paint. The bidirectional reflectance distribution function of the diffuser was not fully characterized before launch, so the Cal/Val Team has implemented a regression of the solar incidence angles and the drift in the node of the satellite's orbit against the diffuser time series to correct for solar incidence angle effects. An exponential function with a time constant of 200 days yields the best fit to the diffuser time series. The decrease in diffuser reflectance over the mission is wavelength-dependent, ranging from 9% in the blue (412 nm) to 5% in the red and near infrared (670-865 nm). The degradation of diffuser reflectance is similar to that observed for SeaWiFS radiometric response itself from lunar calibration time series for bands 1-5 (412-555 nm), though the magnitude of the change is four times larger for the diffuser. Evidently, the same optical degradation process has affected both the telescope optics and the solar diffuser in the blue and green. The Cal/Val Team has developed a methodology for computing the signal-to-noise ratio (SNR) for SeaWiFS on orbit from the diffuser time series. The on-orbit change in the SNR for each band over the nine-year mission is less than 7%. The on-orbit performance of the SeaWiFS solar diffuser should offer insight into the long-term on-orbit performance of solar diffusers on other instruments, such as MODIS, VIIRS, and ABI.
机译:NASA海洋生物处理小组的校准和验证(Cal / Val)团队实施了SeaWiFS的日照校准,以寻找仪器响应中的阶跃函数变化,并使用这些校准来补充每月的月度校准,以监控SeaWiFS的辐射稳定性在运行的第一年。该小组对整个任务的太阳校准时间序列进行了分析,并应用了随着时间变化的月球辐射校正,以评估太阳漫射器反射率在轨道上九年的长期退化。 SeaWiFS扩散器是涂有YB71油漆的铝板。扩散器的双向反射分布函数在发射前尚未完全表征,因此,Cal / Val团队已对太阳入射角和卫星轨道节点相对于扩散器时间序列的漂移进行了回归,以校正太阳入射角度效应。时间常数为200天的指数函数最适合于扩散器时间序列。整个任务中漫反射器反射率的降低取决于波长,范围从蓝色(412 nm)的9%到红色和近红外(670-865 nm)的5%。散射器反射率的下降与从1-5波段(412-555 nm)的月球校准时间序列观察到的SeaWiFS辐射响应本身相似,尽管该变化的幅度是散射器的四倍。显然,相同的光学降解过程已经影响了望远镜光学器件和蓝色和绿色的太阳漫射器。 Cal / Val团队开发了一种方法,用于根据扩散器时间序列计算SeaWiFS在轨道上的信噪比(SNR)。在为期9年的任务中,每个频段的SNR的在轨变化小于7%。 SeaWiFS太阳扩散器的在轨性能应该可以洞察其他仪器(例如MODIS,VIIRS和ABI)上太阳扩散器的长期在轨性能。

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