利用EO-1 Hyperion数据计算L7 ETM+和Terra MODIS传感器之间的光谱波段调整因子(SBAF)

G. Chander, N. Mishra, D. Helder, D. Aaron, T. Choi, A. Angal, X. Xiong
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引用次数: 18

摘要

地球观测的不同应用和技术发展必然需要不同的光谱覆盖范围。因此,即使设计用于观察电磁波谱的同一区域的光谱带,不同传感器的相对光谱响应(RSR)也可能不同。在本研究中,利用高光谱地球观测-1 (EO-1) Hyperion测量得到光谱波段调整因子(SBAF),以调整2000 - 2009年伪不变利比亚4参考标准试验点上Landsat 7 (L7) Enhanced Thematic Mapper Plus (ETM+)和Terra中分辨率成像光谱仪(MODIS)大气顶(TOA)反射率测量值之间的光谱波段差异。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Use of EO-1 Hyperion data to calculate spectral band adjustment factors (SBAF) between the L7 ETM+ and Terra MODIS sensors
Different applications and technology developments in Earth observations necessarily require different spectral coverage. Thus, even for the spectral bands designed to look at the same region of the electromagnetic spectrum, the relative spectral responses (RSR) of different sensors may be different. In this study, spectral band adjustment factors (SBAF) are derived using hyperspectral Earth Observing-1 (EO-1) Hyperion measurements to adjust for the spectral band differences between the Landsat 7 (L7) Enhanced Thematic Mapper Plus (ETM+) and the Terra Moderate Resolution Imaging Spectroradiometer (MODIS) top-of-atmosphere (TOA) reflectance measurements from 2000 to 2009 over the pseudo-invariant Libya 4 reference standard test site.
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