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On-orbit Performance and Calibration Improvements for the Reflective Solar Bands of Terra and Aqua MODIS

机译:Terra和Aqua MODIS反射太阳波段的在轨性能和校准改进

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Moderate Resolution Imaging Spectroradiometer (MODIS) is the keystone instrument for NASA's EOS Terra and Aqua missions, designed to extend and improve heritage sensor measurements and data records of the land, oceans and atmosphere. The reflective solar bands (RSB) of MODIS covering wavelengths from 0.41 μm to 2.2 μm, are calibrated on-orbit using a solar diffuser (SD), with its on-orbit bi-directional reflectance factor (BRF) changes tracked using a solar diffuser stability monitor (SDSM). MODIS is a scanning radiometer using a two-sided paddle-wheel mirror to collect earth view (EV) data over a range of ±55~0 off instrument nadir. In addition to the solar calibration provided by the SD and SDSM system, lunar observations at nearly constant phase angles are regularly scheduled to monitor the RSB calibration stability. For both Terra and Aqua MODIS, the SD and lunar observations are used together to track the on-orbit changes of RSB response versus scan angle (RVS) as the SD and S V port are viewed at different angles of incidence (AOI) on the scan mirror. The MODIS Level IB (LIB) Collection 6 (C6) algorithm incorporated several enhancements over its predecessor Collection 5 (C5) algorithm. A notable improvement was the use of the earth-view (EV) response trends from pseudo-invariant desert targets to characterize the on-orbit RVS for select RSB (Terra bands 1-4, 8, 9 and Aqua bands 8, 9) and the time, AOI, and wavelength-dependent uncertainty. The MODIS Characterization Support Team (MCST) has been maintaining and enhancing the C6 algorithm since its first update in November, 2011 for Aqua MODIS, and February, 2012 for Terra MODIS. Several calibration improvements have been incorporated that include extending the EV-based RVS approach to other RSB, additional correction for SD degradation at SWIR wavelengths, and alternative approaches for on-orbit RVS characterization. In addition to the on-orbit performance of the MODIS RSB, this paper also discusses in detail the recent calibration improvements implemented in the MODIS L1B C6.
机译:中分辨率成像光谱仪(MODIS)是NASA EOS Terra和Aqua任务的主要仪器,旨在扩展和改进遗产传感器的测量以及陆地,海洋和大气层的数据记录。 MODIS的反射太阳波段(RSB)覆盖从0.41μm到2.2μm的波长,使用太阳漫射器(SD)在轨道上进行校准,并使用太阳漫射器跟踪其在途双向反射系数(BRF)的变化稳定性监视器(SDSM)。 MODIS是一种扫描辐射计,使用双面桨轮镜在仪器最低点的±55〜0范围内收集地球视图(EV)数据。除了SD和SDSM系统提供的太阳校准外,还定期安排在几乎恒定的相位角进行月球观测,以监视RSB校准的稳定性。对于Terra和Aqua MODIS,SD和月球观测值一起用于跟踪RSB响应与扫描角度(RVS)的在轨变化,因为在扫描时以不同的入射角(AOI)观察了SD和SV端口镜子。 MODIS级别IB(LIB)集合6(C6)算法在其先前的集合5(C5)算法的基础上进行了多项增强。一个显着的改进是利用伪不变沙漠目标的地球视线(EV)响应趋势来表征选定RSB(Terra 1-4、8、9和Aqua频带8、9)的在轨RVS的特性,以及时间,AOI和与波长有关的不确定性。自从2011年11月对Aqua MODIS和2012年2月对Terra MODIS进行首次更新以来,MODIS特征描述支持团队(MCST)一直在维护和增强C6算法。已合并了几项校准改进,包括将基于EV的RVS方法扩展到其他RSB,针对SWIR波长下SD劣化的附加校正以及在轨RVS表征的替代方法。除了MODIS RSB的在轨性能外,本文还详细讨论了MODIS L1B C6中实现的最新校准改进。

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  • 会议地点 New Delhi(IN)
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    Science Systems and Applications Inc. 10210 Greenbelt Rd, Lanham, MD 20706;

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

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

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

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

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

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

    Global Science and Technology Inc. 7855 Walker Drive, Suite 200 Greenbelt, Maryland 20770;

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

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