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Reduction and Segmentation of Hyperspectral Data Cubes

机译:高光谱数据多维数据集的减少和分割

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The reduction and segmentation of multiwavelength images become problematic when the number of bands increases. Integral field spectroscopy and other instrument designs allowing for enhanced spectral and spatial resolution lead to extremely large hyperspectral data cubes (typically 370 million pixels per exposure for the MUSE instrument). New analysis tools jointly exploring spectral and spatial features are required. We propose a new approach, based on the Mean-Shift method (Comaniciu & Meer 2002), to reduce the dimensionality of large data cubes and extract the main spectral patterns. A set of spectra extracted from the cube is used as an initial reference basis. Each spectrum in the observation is projected on this basis, and represented by a vector of projection coefficients or weights. The Mean-Shift method is then carried out for the whole dataset to find the modes in the projection space. These modes are selected for a new projection basis and the algorithm is iterated until convergence. The distance between two spectra is defined as the angle between their related vector coefficients to increase efficiency: this speeds up the convergence and gives more weight to the comparison of spectral patterns, minimizing the effect of the average intensity of each spectrum. This approach has been tested on simulated data. It is promising, especially for very high spectral resolution data cubes.
机译:当频带的数量增加时,多波长图像的减小和分割变得有问题。积分场光谱和其他仪器设计允许增强的频谱和空间分辨率导致极大的高光谱数据立方体(通常为缪斯仪器的每次曝光370万像素)。需要新的分析工具,共同探索光谱和空间特征。我们提出了一种基于平均换档方法(Comaniciu和Meer 2002)的新方法,以减少大数据多维数据集的维度,提取主要谱模式。从立方体提取的一组光谱用作初始参考。在此基础上投射观察中的每个光谱,并由投影系数或重量的矢量表示。然后对平均数据集进行平均移位方法,以找到投影空间中的模式。选择这些模式以用于新的投影基础,并且算法迭代直到收敛。两个光谱之间的距离被定义为它们的相关载体系数之间的角度,以提高效率:这加速了收敛性并使更多的重量达到光谱模式的比较,最小化每个光谱的平均强度的效果。这种方法已经在模拟数据上进行了测试。它很有希望,特别是对于非常高的光谱分辨率数据多维数据集。

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