Euclidean Distance to Convex Polyhedra and Application to Class Representation in Spectral Images
Antoine Bottenmuller, Florent Magaud, Arnaud Demortière, Etienne Decencière, Petr Dokladal
TL;DR
The paper addresses the challenge of estimating abundance or probability maps in spectral images when the linear unmixing model $Y = M A$ is unsuitable due to few bands or highly correlated spectra. It introduces a density function based on the signed Euclidean distances to polyhedral class frontiers defined by a chosen linear classifier and provides an exact algorithm for computing the minimum-norm point to convex polyhedra, enabling precise distance evaluations. The approach yields superior abundance-map reconstruction on the Samson dataset and delivers strong probability-map performance, while also handling datasets (e.g., Li-ion battery spectral images) incompatible with linear mixing. Together, these contributions enable robust, general-purpose class representation in high-dimensional spectral data, with practical applicability beyond traditional unmixing frameworks.
Abstract
With the aim of estimating the abundance map from observations only, linear unmixing approaches are not always suitable to spectral images, especially when the number of bands is too small or when the spectra of the observed data are too correlated. To address this issue in the general case, we present a novel approach which provides an adapted spatial density function based on any arbitrary linear classifier. A robust mathematical formulation for computing the Euclidean distance to polyhedral sets is presented, along with an efficient algorithm that provides the exact minimum-norm point in a polyhedron. An empirical evaluation on the widely-used Samson hyperspectral dataset demonstrates that the proposed method surpasses state-of-the-art approaches in reconstructing abundance maps. Furthermore, its application to spectral images of a Lithium-ion battery, incompatible with linear unmixing models, validates the method's generality and effectiveness.
