Improvements in the on-orbit calibration of the Terra MODIS short-wave infrared spectral bands

X. Xiong, A. Angal, Yonghong Li
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引用次数: 10

Abstract

The short-wave infrared (SWIR) bands (5-7, 26) of Terra MODIS, co-located with the mid-wave infrared (MWIR) bands (20-25) on the short and mid-wave infrared (SMIR) Focal Plane Assembly (FPA) have a known issue related to 5.3 μm out-of-band (OOB) thermal leak and electronic crosstalk that was identified prelaunch. Intensive efforts were undertaken shortly after launch to mitigate its impacts on the on-orbit calibration and in turn the level 1B (L1B) products. In order to the isolate the OOB contribution among the SWIR bands, special night time day mode (NTDM) operations have been regularly scheduled to collect Earth scene reflective solar bands (RSB) data during spacecraft night time. As MODIS does not have a spectral band centered at 5.3 μm, measurements from the MODIS Airborne Simulator (MAS) spectrometer field campaigns in the early months after Terra launch were used to help identify band 28 (7.325 μm) as the best surrogate to simulate the radiances at 5.3 μm. As a result, band 28 is used as the sending band for the SWIR crosstalk correction for Terra MODIS. In the case of Aqua MODIS, band 25 (4.52 μm) was found to be more effective as the sending band for the SWIR crosstalk correction. In recent years, the Terra MODIS PV LWIR electronic crosstalk (including band 28), has gradually increased, more significantly after the safe-mode event occurred in Feb, 2016. This accentuated degradation in the PV LWIR performance has also impacted the performance of on-orbit SWIR crosstalk correction algorithm and thus the L1B products. In this paper, we examine the use of band 25 as the sending band for Terra MODIS SWIR crosstalk correction and compare its performance with that based on band 28 as the sending band. Results indicate an improvement in the stability of the on-orbit gain for the SWIR bands and a reduced detector-detector and subframe striping in the L1B products, especially during the period when the PV LWIR electronic crosstalk is more severe.
Terra MODIS短波红外波段在轨定标的改进
Terra MODIS的短波红外(SWIR)波段(5-7,26)与短波和中波红外(SMIR)焦平面组件(FPA)上的中波红外(MWIR)波段(20-25)位于同一位置,存在已知的5.3 μm带外(OOB)热泄漏和电子串扰问题,该问题在发射前已被确定。发射后不久,为减轻其对在轨校准和1B级(L1B)产品的影响,开展了大量工作。为了隔离在SWIR波段中OOB的贡献,在航天器夜间定期安排特殊的昼夜模式(NTDM)操作来收集地球场景反射太阳波段(RSB)数据。由于MODIS没有以5.3 μm为中心的光谱带,在Terra发射后的最初几个月,MODIS机载模拟器(MAS)光谱仪现场活动的测量数据被用来帮助确定波段28 (7.325 μm)是模拟5.3 μm辐射的最佳替代波段。因此,波段28被用作Terra MODIS的SWIR串扰校正的发送波段。在Aqua MODIS中,波段25 (4.52 μm)作为SWIR串扰校正的发送波段更为有效。近年来,Terra MODIS PV LWIR电子串扰(包括波段28)逐渐增加,在2016年2月发生安全模式事件后更为明显。PV LWIR性能的恶化也影响了在轨SWIR串扰校正算法的性能,从而影响了L1B产品的性能。在本文中,我们研究了使用波段25作为发送波段的Terra MODIS SWIR串扰校正,并将其性能与以波段28作为发送波段的性能进行了比较。结果表明,L1B产品的在轨增益稳定性得到了改善,特别是在PV - LWIR电子串扰较为严重的时期,L1B产品的探测器-探测器和子框条带减少。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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