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Effects of orbital drift on land surface temperature measured by AVHRR thermal sensors

机译:轨道漂移对AVHRR热传感器测量的地表温度的影响

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The NOAA series of meteorological satellites that carry the Advanced Very High Resolution Radiometer (AVURR) suffer from orbital drift so that during each satellite's duty period the overpass time occurs later in the day. Replacement satellites restore the overpass time temporarily, hut then it gradually decays. The goals of this paper are to document the effects of variable observation time owing to orbital drift on brightness temperatures (BT) and land surface temperature (LST) calculated from them in the NOAA/NASA Pathfinder AVHRR Land (PAL) data set and to consider possible corrections for the resulting trends and discontinuities in the PAL BT data. The drift effects were found to be greater for bare ground than for vegetated land cover classes, however significant effects were found for most vegetated classes. The magnitude of the orbital drift effect for most global cover types was at least as large as the other errors that affect LST measurement. A simple empirical correction for observation time based on solar zenith angle (SZA) was used to correct the PAL BT time series following Gutman [Int. J. Remote Sens. 20 (1999a) 3407]. The correction from this method was compared with that predicted by a physically based model and was found to differ in the early part of each satellite's duty cycle. Finally, the impacts of correction on the effective observation time were analyzed and the simple statistical correction was found to suffer from greater variability than has hitherto been recognized. A modification to the statistical correction to adjust the effective observation time is described.
机译:携带高级超高分辨率辐射计(AVURR)的NOAA系列气象卫星遭受轨道漂移,因此在每个卫星的工作期间,越过时间会在当天晚些时候发生。替换卫星暂时恢复了立交时间,但随后逐渐衰减。本文的目的是在NOAA / NASA探路者AVHRR土地(PAL)数据集中记录因轨道漂移而导致的观测时间变化对它们所计算出的亮度温度(BT)和地表温度(LST)的影响,并考虑对PAL BT数据中的趋势和不连续性进行可能的校正。发现裸露地面的漂移影响要大于植被覆盖率的漂移影响,但是对于大多数植被覆盖类型,漂移影响却显着。大多数全球覆盖类型的轨道漂移效应的大小至少与影响LST测量的其他误差一样大。基于太阳天顶角(SZA)的观测时间的简单经验校正用于校正遵循Gutman [Int。 J. Remote Sens。20(1999a)3407]。将该方法的校正结果与基于物理模型的预测结果进行了比较,发现在每个卫星工作周期的早期都有所不同。最后,分析了校正对有效观测时间的影响,发现简单的统计校正比迄今为止公认的具有更大的可变性。描述了对统计校正的修改以调整有效观察时间。

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