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SeaWiFS long-term solar diffuser reflectance and sensor noise analyses

机译:SeaWiFS长期太阳漫射器反射率和传感器噪声分析

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The NASA Ocean Biology Processing Group's Calibration and Validation (Cal/Val) team has undertaken an analysis of the mission-long Sea-Viewing Wide Field-of-View Sensor (SeaWiFS) solar calibration time series to assess the long-term degradation of the solar diffuser reflectance over 9 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 9percent in the blue (412 nm) to 5percent in the red and near infrared (670-865 nm). 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 corrected for both the varying solar incidence angles and the diffuser reflectance degradation. A sensor noise model is used to compare on-orbit SNRs computed for radiances reflected from the diffuser with prelaunch SNRs measured at typical radiances specified for the instrument. To within the uncertainties in the measurements, the SNRs for SeaWiFS have not changed over the mission. 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 the Moderate-Resolution Imaging Spectrometer [currently flying on the Earth Observing System (EOS) Terra and Aqua satellites], the Visible and Infrared Radiometer Suite [scheduled to fly on the NASA National Polar-orbiting Operational Environmental Satellite System (NPOESS) and NPOESS Preparatory Project (NPP) satellites] and the Advanced Baseline Imager [scheduled to fly on the National Oceanic and Atmospheric Administration Geostationary Environmental Operational Satellite Series R (GOES-R) satellites].
机译:NASA海洋生物处理小组的校准和验证(Cal / Val)团队已对任务期较长的广视宽视野传感器(SeaWiFS)太阳校准时间序列进行了分析,以评估其长期退化。太阳漫射器在轨道上反射超过9年。 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团队已实现了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的回归,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%。 Cal / Val团队已经开发出一种方法,用于根据针对不断变化的太阳入射角和扩散器反射率退化进行校正的扩散器时间序列,计算轨道上SeaWiFS的信噪比(SNR)。传感器噪声模型用于将针对从扩散器反射的辐射计算出的在轨SNR与在为仪器指定的典型辐射率下测量的发射前SNR进行比较。在测量的不确定性范围内,SeaWiFS的SNR在整个任务中没有改变。 SeaWiFS太阳漫射器的在轨性能应该提供对其他仪器(例如,目前正在对地观测系统(EOS)Terra和上空飞行的中等分辨率成像光谱仪)上太阳漫射器的长期在轨性能的了解。 Aqua卫星],可见和红外辐射计套件[计划在NASA国家极轨运行环境卫星系统(NPOESS)和NPOESS筹备项目(NPP)卫星上飞行]和高级基线成像仪[计划在国家海洋上飞行和大气管理地球静止环境运行卫星系列R(GOES-R)卫星]。

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