Hyperspectral imaging data atmospheric correction challenges and solutions using QUAC and FLAASH algorithms

Amol D. Vibhute, K. Kale, Rajesh K. Dhumal, S. Mehrotra
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引用次数: 27

Abstract

Recently, Hyperspectral remote sensing technology has been proved to be a valuable tool to get reliable information with details for identifying different objects on the earth surface with high spectral resolution. Due to atmospheric effects the valuable information may be lost from hyperspectral data. Hence it is necessary to remove these effects from hyperspectral data for reliable identification of the objects on the earth surface. The atmospheric correction is a very critical task of hyperspectral images. The present paper highlights the advantages of hyperspectral data, challenges over it as a pre-processing with solutions through QUAC and FLAASH algorithms. The hyperspectral data acquired for Aurangabad district were used to test these algorithms. The result indicates that the size of hyperspectral image can be reduced. The ENVI 5.1 software with IDL language is an efficient way to visualize and analysis the hyperspectral images. Implementation of atmospheric correction algorithms like QUAC and FLAASH is successfully carried out. The QUAC model gives accurate and reliable results without any ancillary information but requires only wavelength and radiometric calibration with less time than FLAASH.
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使用QUAC和FLAASH算法的高光谱成像数据大气校正挑战和解决方案
近年来,高光谱遥感技术已被证明是获得高光谱分辨率地球表面不同目标的可靠细节信息的宝贵工具。由于大气的影响,高光谱数据中有价值的信息可能会丢失。因此,为了可靠地识别地表目标,有必要从高光谱数据中去除这些影响。大气校正是高光谱图像的一项非常关键的任务。本文重点介绍了高光谱数据作为预处理的优势和挑战,并通过QUAC和FLAASH算法进行了解决。利用奥兰加巴德地区的高光谱数据对这些算法进行了测试。结果表明,该方法可以减小高光谱图像的尺寸。基于IDL语言的ENVI 5.1软件是实现高光谱图像可视化和分析的有效方法。成功实现了QUAC和FLAASH等大气校正算法。QUAC模型给出了准确可靠的结果,没有任何辅助信息,只需要波长和辐射校准,比FLAASH更短的时间。
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