Abstract

Hyperspectral spectral mixture analysis (SMA), which intends to decompose mixed pixels into a collection of endmembers weighted by their corresponding fraction abundances, has been successfully used to tackle mixed-pixel problem in hyperspectral remote sensing applications. As an approach of decomposing a high-dimensional data matrix into the multiplication of two nonnegative matrices, nonnegative matrix factorization (NMF) has shown its advantages and been widely applied to SMA. Unfortunately, most of the NMF-based unmixing methods can easily lead to an unsuitable solution, due to inadequate mining of spatial and spectral information and the influence of outliers and noise. To overcome such limitations, a spatial constraint over abundance and a spectral constraint over endmembers are imposed over NMF-based unmixing model for spectral-spatial constrained unmixing. Specifically, a spatial neighborhood preserving constraint is proposed to preserve the local geometric structure of the hyperspectral data by assuming that pixels in a spatial neighborhood generally fall into a low-dimensional manifold, while a minimum spectral distance constraint is formulated to optimize endmember spectra as compact as possible. Furthermore, to handle non-Gaussian noises or outliers, an L <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">2,1</sub> -norm based loss function is ultimately adopted for the proposed spectral-spatial constrained nonnegative matrix factorization model and a projected gradient based optimization algorithm is designed for optimization. Experimental results over both synthetic and real-world datasets demonstrate that the proposed spatial and spectral constraints can certainly improve the performance of NMF-based unmixing and outperform state-of-the-art NMF-based unmixing algorithms.

Highlights

  • H YPERSPECTRAL remote sensing image, which involves collecting abundant spectral information over hundreds of contiguous bands, has been widely applied to many civil and military fields [1]–[3]

  • In which J1(M) and J2(A) are additional constraints imposed on endmember matrix M and abundance matrix A respectively, and λ1 and λ2 are their trade-offs among different objective functions

  • Observed from the linear mixture model (LMM) defined by (1), spectral information of an image can be represented by its endmembers since all the pixels can be represented by these endmembers, while spatial information, which reflects the structural relationship of pixels and their neighbors, can be expressed in the similarity of their corresponding abundance

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Summary

Introduction

H YPERSPECTRAL remote sensing image, which involves collecting abundant spectral information over hundreds of contiguous bands, has been widely applied to many civil and military fields [1]–[3]. Feng et al proposed a sparsity-constrained deep NMF with the total variation (SDNMF-TV) technique for hyperspectral unmixing, which introduced an L1/2 constraint for the sparse distribution of each endmember in the 2-D space and the TV regularizer for promoting piecewise smoothness in abundance maps [30]. Many other related methods, such as graph regularized based [43], self-paced based NMF algorithms [44], tensor based [45], [46], and deep learning based unmixing algorithms [47]– [49], hava been developed These algorithms do not deal well with outliers or noise and the effect on spatial structure of abundance distribution still needs to be further verified. To alleviate the above-mentioned problems and take full advantage of spatial and spectral information, in this paper, a spectral-spatial constrained NMF algorithm is proposed by imposing constraints on both endmembers and abundance simultaneously.

NMF Model for SMA
PG based NMF algorithm for SMA
Our Proposed Spectral and Spatial constrained NMF algorithms for SMA
Spectral constraint for endmembers
Spectral and Spatial constrained NMF algorithm for SMA
Experiments Over Synthetic Dataset
38 Synthetic dataset
Convergence Analysis
Conclusion
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