2015
DOI: 10.1109/tgrs.2014.2383440
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A Novel Negative Abundance‐Oriented Hyperspectral Unmixing Algorithm

Abstract: International audienceSpectral unmixing is a popular technique for analyzing remotely sensed hyperspectral data sets with subpixel precision. Over the last few years, many algorithms have been developed for each of the main processing steps involved in spectral unmixing (SU) under the LMM assumption: 1) estimation of the number of endmembers; 2) identification of the spectral signatures of the endmembers; and 3) estimation of the abundance of endmembers in the scene. Although this general processing chain has … Show more

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Cited by 26 publications
(9 citation statements)
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“…Three non eigen-based hyperspectral ID estimators have recently been proposed. The first one, introduced in [34] as part of a Negative ABundance-Oriented (NABO) unmixing algorithm, borrows the main idea from the HySIME algorithm. Basically, it decomposes the residual error from the unconstrained unmixing into two components, a first due to noise and a second due to ID.…”
Section: A Related Workmentioning
confidence: 99%
See 1 more Smart Citation
“…Three non eigen-based hyperspectral ID estimators have recently been proposed. The first one, introduced in [34] as part of a Negative ABundance-Oriented (NABO) unmixing algorithm, borrows the main idea from the HySIME algorithm. Basically, it decomposes the residual error from the unconstrained unmixing into two components, a first due to noise and a second due to ID.…”
Section: A Related Workmentioning
confidence: 99%
“…This technique [34] performs spectral unmixing and dimensionality estimation at the same time. It is noteworthy that this method is not eigenvalue-based.…”
Section: F Vertex Component Analysis/negative Abundance Oriented Algmentioning
confidence: 99%
“…where Y = [y 1 , y 2 , ..., y N ] is the hyperspectral image matrix, A = [α 1 , α 2 , ..., α N ] and N = [n 1 , n 2 , ..., n N ] represent the abundance matrix and the noise matrix, respectively. Due to physical limitations and constraints, the abundance needs to satisfy two constraints, namely the abundance sum-to-one constraint (ASC, ∑ m j=1 α j = 1) and the abundance nonnegative constraint (ANC, α j ≥ 0, j = 1, 2, ..., m) [10].…”
Section: Introductionmentioning
confidence: 99%
“…And the analysis of the influence of the ambient temperature on the spectrum of the space target has not been carried out. 6,7 Additional scattering correction method 8 , mean variance correction 9 and normalization 10 are often used to analyze the characteristics of visible light. Compared with the above methods, the nonlinear temperature correction has a unique advantage in the correction of the model.…”
Section: Introductionmentioning
confidence: 99%