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Pleiades-HR 1A1B Image quality commissioning: innovative radiometric calibration methods and results

机译:Pleiades-HR 1A&1B图像质量调试:创新的辐射校准方法和结果

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Pleiades is an earth observing system conducted by the French National Space Agency, CNES. It consists of two satellites launched on December 2011 (PHR-1A) and December 2012 (PHR-1B), both designed to provide optical push-broom imagery on five spectral bands to civilian and defense users, with ground sample distance up to 70 cm. During inflight image quality commissioning, radiometric activities included inter-detector normalization coefficients computation, refocusing operations, MTF assessment and estimation of signal to noise ratios. This paper presents inflight results for both satellites. It focuses on several innovative methods that were implemented, taking advantage of the satellite platform great agility. These methods are based on processing images obtained through dedicated exotic guidance. In particular, slow-motion steering enables an efficient estimation of the instrumental noise model, since during acquisition each detector has been viewing a stable ground target along different time samples. Conversely, rotated retina guidance is used to guarantee that all different elementary detectors have successively viewed the same set of landscape samples during acquisition. Non-uniformity of detector sensitivities can then be characterized, and on-board coefficients used prior to compression can be calibrated in order to prevent vertical striping effects on operational images. Defocus control and Point Spread Function estimation can be easily obtained through processing acquisitions of stars associated to various spectral characteristics, for different adjustments of the refocusing system. All these methods allow an accurate estimation of radiometric performance on the whole range of specified spectral radiances, while drastically reducing the number of required acquisitions on natural targets.
机译:le宿星是法国国家航天局(CNES)进行的对地观测系统。它由两颗分别于2011年12月(PHR-1A)和2012年12月(PHR-1B)发射的卫星组成,旨在为民用和国防用户提供五个频谱带上的光学扫帚成像,地面采样距离可达70厘米。在机载图像质量调试期间,辐射测量活动包括探测器间归一化系数计算,重新聚焦操作,MTF评估和信噪比估计。本文介绍了这两种卫星的飞行结果。它着重介绍了已实施的几种创新方法,这些方法利用了卫星平台的巨大灵活性。这些方法基于处理通过专用异国向导获得的图像。特别是,由于转向过程中每个检测器一直在沿不同的时间采样观察稳定的地面目标,因此,慢速转向可以有效地估计仪器的噪声模型。相反,旋转的视网膜引导用于确保所有不同的基本检测器在采集过程中已连续观察相同的景观样本集。然后可以表征检测器灵敏度的不均匀性,并且可以对压缩之前使用的车载系数进行校准,以防止对操作图像产生垂直条纹效应。通过对与各种光谱特性相关的恒星进行处理采集,可以轻松获得散焦控制和点扩展函数估计,以实现对重聚焦系统的不同调整。所有这些方法都可以在指定光谱辐射率的整个范围内准确估计辐射性能,同时大大减少了自然目标所需的采集次数。

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