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On-orbit calibration performance of MODIS TDI bands

机译:MODIS TDI频段的在轨校准性能

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摘要

Bands 13 (667 run) and 14 (678 run) of the Moderate Resolution Imaging Spectroradiometer (MODIS) onboard the Terra and Aqua satellites are built with a time delay and integration (TDI) circuit and a high-low dual-gain setting intended for the monitoring of the ocean environment. An important on-orbit performance issue for the high-gain output of Terra Band 14 and Aqua Band 13 and 14 is that these three bands saturate during standard on-orbit calibrations using the onboard solar diffuser (SD). Consequently, their calibration procedure requires a derivation different from other reflective solar bands (RSB). A high-low scaling-ratio approach is employed for these bands to obtain the high-gain coefficients via the low-gain output 13L and 14L through a calculated constant ratio derived from other sources. Currently, earth view (EV) scenes over the North Atlantic Ocean are used as the primary sources. As it also has been observed that the response versus scan-angle (RVS) exhibits noticeable changes with time for RSB, a time-dependent RVS calibration algorithm has been implemented based on the SD and lunar calibration results. This paper reviews the electronic design and operation of Band 13 and 14, discusses the SD calibration and the saturation issue of the high-gain output, and the time-dependent RVS algorithms. Long-term performance of the calibration coefficient and RVS are presented. The long-term trend shows that the gain-change for Terra MODIS Band 13 and 14, for both high- and low-gain bands, is significant at 6% and 23%, but is more modest for Aqua MODIS Band 13 and 14 at 6% and 2%. The gain ratios 13H/13L and 14H/14L are very stable at the level of 0.01% for both MODIS instruments. The long-term gain difference due to RVS effect is up to 3% for Terra MODIS and about 2% and below for Aqua MODIS.
机译:Terra和Aqua卫星上的中分辨率成像光谱仪(MODIS)的13(667频段)和14(678频段)频段具有时延和积分(TDI)电路以及旨在用于以下用途的高/低双增益设置:海洋环境的监测。 Terra Band 14,Aqua Band 13和14的高增益输出的一个重要的在轨性能问题是,在使用机载太阳能扩散器(SD)进行标准在轨校准期间,这三个频带会饱和。因此,它们的校准过程需要与其他反射太阳波段(RSB)不同的推导。对这些频带采用高/低比例缩放方法,以通过低增益输出13L和14L通过从其他来源得出的计算出的恒定比率获得高增益系数。当前,北大西洋上空的地球(EV)场景被用作主要来源。由于还观察到响应与扫描角度(RVS)的关系随RSB的变化而显着变化,因此已根据SD和月球校准结果实现了随时间变化的RVS校准算法。本文回顾了频段13和14的电子设计和操作,讨论了SD校准和高增益输出的饱和问题,以及与时间有关的RVS算法。介绍了校准系数和RVS的长期性能。长期趋势表明,Terra MODIS频段13和14在高增益和低增益频段上的增益变化显着,分别为6%和23%,但对于Aqua MODIS频段13和14而言,增益变化较小。分别为6%和2%。两种MODIS仪器的增益比13H / 13L和14H / 14L都非常稳定在0.01%的水平。由于RVS效应引起的长期增益差异,Terra MODIS高达3%,Aqua MODIS约为2%甚至更低。

著录项

  • 来源
    《Earth observing systems XVIII》|2013年|886605.1-886605.10|共10页
  • 会议地点 San Diego CA(US)
  • 作者单位

    Sigma Space Corp., 4600 Forbes Blvd, Lanham, Maryland 20706;

    Sigma Space Corp., 4600 Forbes Blvd, Lanham, Maryland 20706;

    Science Systems and Applications, Inc., 10210 Greenbelt Road, Lanham, MD 20706;

    Sigma Space Corp., 4600 Forbes Blvd, Lanham, Maryland 20706;

    Sigma Space Corp., 4600 Forbes Blvd, Lanham, Maryland 20706;

    Sigma Space Corp., 4600 Forbes Blvd, Lanham, Maryland 20706;

    Sciences and Exploration Directorate, NASA/GSFC, Greenbelt, MD 20771;

  • 会议组织
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    MODIS; RSB; TDI; Calibration;

    机译:MODIS; RSB; TDI;校准;

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