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Geological Applications of Machine Learning in Hyperspectral Remote Sensing Data

机译:机器学习在高光谱遥感数据中的地质应用

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The CRISM imaging spectrometer orbiting Mars has been producing a vast amount of data in the visible to infrared wavelengths in the form of hyperspectral data cubes. These data, compared with those obtained from previous remote sensing techniques, yield an unprecedented level of detailed spectral resolution in additional to an ever increasing level of spatial information. A major challenge brought about by the data is the burden of processing and interpreting these datasets and extract the relevant information from it. This research aims at approaching the challenge by exploring machine learning methods especially unsupervised learning to achieve cluster density estimation and classification, and ultimately devising an efficient means leading to identification of minerals. A set of software tools have been constructed by Python to access and experiment with CRISM hyperspectral cubes selected from two specific Mars locations. A machine learning pipeline is proposed and unsupervised learning methods were implemented onto pre-processed datasets. The resulting data clusters are compared with the published ASTER spectral library and browse data products from the Planetary Data System (PDS). The result demonstrated that this approach is capable of processing the huge amount of hyperspectral data and potentially providing guidance to scientists for more detailed studies.
机译:围绕火星运行的CRISM成像光谱仪已经以高光谱数据立方体的形式生成了从可见光到红外波长的大量数据。与从以前的遥感技术获得的数据相比,这些数据除空间信息水平不断提高外,还提供了前所未有的详细光谱分辨率。数据带来的主要挑战是处理和解释这些数据集并从中提取相关信息的负担。这项研究旨在通过探索机器学习方法(尤其是无监督学习)来实现挑战,以实现簇密度估计和分类,并最终设计出一种有效的方法来鉴定矿物。 Python构造了一套软件工具来访问和试验从两个特定的火星位置选择的CRISM高光谱立方体。提出了机器学习管道,并在预处理的数据集上实现了无监督学习方法。将所得的数据簇与已发布的ASTER光谱库进行比较,并浏览来自行星数据系统(PDS)的数据产品。结果表明,该方法能够处理大量的高光谱数据,并可能为科学家进行更详细的研究提供指导。

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