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Effects of out-of-band and time-varying relative spectral response on the calibration of MODIS reflective solar bands

机译:带外和时变相对光谱响应对MODIS反射太阳能带的校准的影响

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Calibration of the on-orbit gain changes of the narrow bandwidth reflective solar bands (RSB) of Terra and Aqua MODIS is usually based on the band center wavelength. The relative spectral response (RSR) of each band is assumed to be constant on orbit, and the time dependence of an overall gain factor is calculated. Any on-orbit changes to the RSR of the MODIS bands will introduce some error into the calibration and may also have an impact on the Earth scene radiance retrieval. We consider two different ways to track how the RSR of the MODIS RSB may change on orbit and the effects that these changes have on the calibration. First, we study the broadband degradation of the MODIS scan mirror and how it may change the effective out-of-band response of the RSB. Second, we examine in-band RSR measurements from the spectroradiometric calibration assembly carried on-board both MODIS instruments. We find that RSR changes have a relatively small effect on the radiance calibrated using the on-board solar diffuser, generally <0.5% for all RSB at any time in the missions, though the effect may be slightly larger for some scan angles. The impact of RSR changes on the Earth scene radiance retrieval is highly dependent on the spectral properties of the scene and could be significantly larger. The bands showing the largest impacts are Terra bands 1, 4, 8, 9, 17, and 19 and Aqua bands 8 and 9. (C) 2020 Society of Photo-Optical Instrumentation Engineers (SPIE)
机译:校准Terra和Aqua Modis的窄带宽反射太阳能带(RSB)的轨道增益变化通常基于带中心波长。假设每个频带的相对光谱响应(RSR)在轨道上是恒定的,并且计算总增益因子的时间依赖性。 MODIS频段RSR的任何ON-ORIB更改都将对校准引入一些错误,并且也可能对地球场景光发射检索产生影响。我们考虑了两种不同的方法来跟踪MODIS RSB的RSR如何在轨道上改变以及这些变化对校准的影响。首先,我们研究了MODIS扫描镜的宽带劣化以及它如何改变RSB的有效外响应。其次,我们从携带的SpectrorAdiometric校准组件中检查带校准组件的带内RSR测量。我们发现RSR变化对使用车载太阳漫射器校准的光线的效果相对较小,所有RSB在任务中的任何时间都是<0.5%,但对于某些扫描角度来说,效果可能略大。 RSR变化对地球场景辐射检索的影响高度依赖于场景的光谱特性,并且可以显着更大。显示最大影响的乐队是Terra Bands 1,4,8,9,17和19和Aqua带8和9.(c)2020年光学光学仪表工程师协会(SPIE)

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