2021
DOI: 10.1109/jstars.2020.3048820
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Sparse and Low-Rank Constrained Tensor Factorization for Hyperspectral Image Unmixing

Abstract: Third-order tensors have been widely used in hyperspectral remote sensing because of their ability to maintain the three-dimensional structure of hyperspectral images. In recent years, hyperspectral unmixing algorithms based on tensor factorization have emerged, but these decomposition processes may be inconsistent with physical mechanism of unmixing. To solve this problem, this paper proposes a sparse and low-rank constrained tensor factorization unmixing algorithm (SPLRTF) based on a matrix-vector nonnegativ… Show more

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Cited by 38 publications
(36 citation statements)
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“…1) Samson Data: the data are generated by the SAMSON sensor [14]. It contains 156 channels with the wavelengths from 0.401 ~ 0.889𝜇𝑚 .…”
Section: B Real Hyperspectral Data Experimentsmentioning
confidence: 99%
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“…1) Samson Data: the data are generated by the SAMSON sensor [14]. It contains 156 channels with the wavelengths from 0.401 ~ 0.889𝜇𝑚 .…”
Section: B Real Hyperspectral Data Experimentsmentioning
confidence: 99%
“…Several spectral unmixing approaches based on geometry [7]- [9], statistics [10], [11], nonnegative matrix factorization (NMF) [12]- [14] and sparse regression [5], [15] are mainly introduced in LMM. Although geometry and statistics approaches are simple and fast, the presence of pure materials assumptions in hyperspectral data are usually required and accompanied with higher computational complexity.…”
Section: Introductionmentioning
confidence: 99%
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“…On the other hand, in [24] and [25], a weighted sparse unmixing framework with weighted l 1 norm is proposed, which penalizes the nonzero elements in the abundance matrix by introducing one or more weighting factors. Meanwhile, a variety of spatial and/or spectral weighted regularizers [26]- [30] have also been proposed to introduce related spatial and spectral information in HSI to improve the unmixing results.…”
Section: Introductionmentioning
confidence: 99%
“…The high spatial correlation of the image implies the low rankness of the abundance matrix [26]. Accordingly, when the low-rank constraint is imposed on the abundance matrix, the low-dimensional subspace structure of the image will be well preserved [27]. More recently, the sparsity and lowrank constraints [28] were simultaneously imposed on the abundance matrix to reduce the solution space.…”
Section: Introductionmentioning
confidence: 99%