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Correcting NOAA-AVHRR Orbital Drift: a Simple and Automatic Methodology

机译:校正NOAA-AVHRR轨道漂移:一种简单而自动的方法

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NOAA (National Oceanic and Atmosphere Administration) AVHRR (Advanced Very High Resolution Radiometer) data scientific use is hindered by the orbital drift each platform has suffered, which prevents multitemporal analyses. The study presented here provides a new way to correct the data from this orbital drift, using additional information on the data acquisition, such as solar zenithal angle and acquisition day information. This information is used to estimate at each date and for each pixel a theoretical solar zenithal angle, which difference to the actual one is fitted against each channel data anomaly. This fit is then used to calculate a correcting factor which is applied to the whole time series for each channel data. This procedure has been applied to data provided by the GIMMS (Global Imaging Modeling and Mapping Studies) group, namely the African continent from the end of 2000 to the end of 2004, corresponding to NOAA-16 satellite.
机译:每个平台遭受的轨道漂移阻碍了NOAA(国家海洋与大气管理局)AVHRR(高级超高分辨率辐射计)数据的科学使用,从而阻止了多时相分析。本文介绍的研究提供了一种新方法,可以使用有关数据采集的其他信息(例如太阳天顶角和采集日信息)来校正来自此轨道漂移的数据。该信息用于估计每个日期以及每个像素的理论太阳天顶角,该理论天顶角与实际角度的差异将针对每个通道数据异常进行拟合。然后,该拟合用于计算校正因子,该校正因子将应用于每个通道数据的整个时间序列。该程序已应用于GIMMS(全球成像建模和制图研究)小组提供的数据,该小组即2000年底至2004年底的非洲大陆,对应于NOAA-16卫星。

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