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MODIS on-orbit spatial characterization results using ground measurements

机译:使用地面测量的MODIS在轨空间表征结果

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MODerate resolution Imaging Spectro-radiometer (MODIS), as part of NASA's Earth Observe System (EOS) mission, is widely utilized in diversified scientific research areas. Both Terra and Aqua MODIS observe the earth in sun-synchronous orbit at three nadir spatial resolutions. MODIS has thirty-six bands that are located in four Focal Plane Assembles (FPAs) by wavelength: Visible (VIS), Near-Infrared (NIR), Short-and Middle-wavelength IR (SMIR), and Long wavelength IR (LWIR). MODIS Band-to-Band Registration (BBR) was measured pre-launch at the instrument vendor. Mis-registration exists between bands and FPAs. The spatial characterization could change in storage, at launch, and years on-orbit. In this study, a special ground scene with unique features has been selected as our study area to calculate the spatial registration in both along-scan and along-track for bands 2-7 relative to band 1. The results from the earth scene targets have been compared with on-board calibrator, the Spectro-Radiometric Calibration Assembly (SRCA), with good agreement. The measured differences between the SRCA and our ground scene approach are less than 20m on average for VIS/NIR bands both along-scan and along-track. The differences for SMIR bands are 20m along-scan and 0.1 - 0.18 km for along track. The SMIR FPA crosstalk could be a contributor to the difference. For Aqua MODIS instruments, the spatial deviation is very small between the bands located on the same FPA or between VIS and NIR FPAs but is relatively large between warm (VIS and NIR) and cold (SMIR and LWIR) FPAs. The spatial deviation for MODIS/Terra can be ignorable but not for MODIS/Aqua. The results from this study show that the spatial deviation of Aqua MODIS may impact on the science data when multi-band data from both warm and cold FPAs is combined.
机译:作为NASA的地球观测系统(EOS)任务的一部分,中等分辨率成像光谱辐射仪(MODIS)被广泛用于各种科学研究领域。 Terra和Aqua MODIS均以三个天底的空间分辨率在太阳同步轨道上观测地球。 MODIS具有36个波段,按波长位于四个焦平面组件(FPA)中:可见(VIS),近红外(NIR),短和中波长IR(SMIR)和长波长IR(LWIR) 。 MODIS频段间注册(BBR)是在仪器供应商启动前进行测量的。频段和FPA之间存在注册错误。空间特性可能会在存储,发射和在轨多年的情况下发生变化。在这项研究中,我们选择了一个具有独特特征的特殊地面场景作为我们的研究区域,以计算相对于波段1的2-7波段在沿扫描和沿轨道的空间配准。与车载校准器“光谱辐射校准组件”(SRCA)进行了比较,具有很好的一致性。沿扫描和沿轨道的VIS / NIR波段,SRCA和我们的地面场景方法之间的测量差异平均小于20m。 SMIR频段的差异沿扫描为20m,沿轨道的差异为0.1-0.18 km。 SMIR FPA串扰可能是造成这种差异的原因。对于Aqua MODIS仪器,位于同一FPA上的频段之间或VIS与NIR FPA之间的频段之间的空间偏差非常小,而在暖(VIS和NIR)与冷(SMIR和LWIR)FPA之间的空间偏差相对较大。 MODIS / Terra的空间偏差可以忽略不计,但MODIS / Aqua的空间偏差则可以忽略。这项研究的结果表明,当组合来自冷和热FPA的多波段数据时,Aqua MODIS的空间偏差可能会影响科学数据。

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