Collaborative Sparse Hyperspectral Unmixing Using [Formula Omitted] Norm
Sparse unmixing has been applied on hyperspectral imagery popularly in recent years. It assumes that every observed signature is a linear combination of just a few spectra (end-members) from a known spectral library. However, solving the sparse unmixing problem directly (using [Formula Omitted] norm...
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Veröffentlicht in: | IEEE transactions on geoscience and remote sensing 2018-01, Vol.56 (9), p.5495 |
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Sprache: | eng |
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Zusammenfassung: | Sparse unmixing has been applied on hyperspectral imagery popularly in recent years. It assumes that every observed signature is a linear combination of just a few spectra (end-members) from a known spectral library. However, solving the sparse unmixing problem directly (using [Formula Omitted] norm to control the sparsity of solution at a low level) is NP-hard. Most related works focus on convex relaxation methods, but the sparsity and accuracy of results cannot be well guaranteed. Under these circumstances, this paper proposes a novel algorithm termed collaborative sparse hyperspectral unmixing using [Formula Omitted] norm (CSUnL0), which aims at solving [Formula Omitted] problem directly. First, it introduces a row-hard-threshold function. The row-hard-threshold function makes it possible to combine [Formula Omitted] norm, instead of its approximate norms, with alternating direction method of multipliers. Compared with the convex relaxation methods, the [Formula Omitted] norm constraint guarantees sparser and more accurate results. Moreover, the antinoise ability of CSUnL0 also gets improved. Second, CSUnL0 uses [Formula Omitted] norm of each end-members’ abundance across the whole map as a collaborative constraint, which can take advantage of the hyperspectral dat’s subspace property. The experimental results indicate that [Formula Omitted] norm contributes to acquiring a more sparser solution and helps CSUnL0 to enhance calculation accuracy. |
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ISSN: | 0196-2892 1558-0644 |
DOI: | 10.1109/TGRS.2018.2818703 |