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Machine learning techniques for the inversion of planetary hyperspectral images

机译:机器学习技术,用于行星高光谱图像的反转

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In this paper, the physical analysis of planetary hyperspectral images is addressed. To deal with high dimensional spaces (image cubes present 256 bands), two methods are proposed. The first method is the support vectors machines regression (SVM-R) which applies the structural risk minimization to perform a non-linear regression. Several kernels are investigated in this work. The second method is the Gaussian regularized sliced inverse regression (GRSIR). It is a two step strategy; the data are map onto a lower dimensional vector space where the regression is performed. Experimental results on simulated data sets have showed that the SVM-R is the most accurate method. However, when dealing with real data sets, the GRSIR gives the most interpretable results.
机译:本文解决了行星高光谱图像的物理分析。为了处理高维空间(图像立方体存在256个带),提出了两种方法。第一种方法是支持矢量的回归(SVM-R),其应用结构风险最小化以执行非线性回归。在这项工作中调查了几个内核。第二种方法是高斯正则化切片逆回归(GRSIR)。这是一个两步战略;数据是在执行回归的较低维矢量空间上的地图。模拟数据集的实验结果表明,SVM-R是最准确的方法。但是,在处理真实数据集时,GRSIR会产生最可接定的结果。

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