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2020
DOI: 10.1109/lgrs.2019.2958203
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Spectral Unmixing: A Derivation of the Extended Linear Mixing Model From the Hapke Model

Abstract: In hyperspectral imaging, spectral unmixing aims at decomposing the image into a set of reference spectral signatures corresponding to the materials present in the observed scene and their relative proportions in every pixel. While a linear mixing model was used for a long time, the complex nature of the physical mixing processes led to shift the community's attention towards nonlinear models or algorithms accounting for the variability of the endmembers. Such intra-class variations are due to local changes in… Show more

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Cited by 23 publications
(11 citation statements)
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“…Then we simulate the effect on the reflectance spectra of a changing incidence angle θ0 from the sun within a few hours, while the emergence angle θ = 30 • is constant. We first obtain albedo spectra of the endmembers by inverting the Hapke model [18,19], assuming Lambertian photometric parameters. We simulate the evolution of the incidence angle with time using a similar model to that of Eq.…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…Then we simulate the effect on the reflectance spectra of a changing incidence angle θ0 from the sun within a few hours, while the emergence angle θ = 30 • is constant. We first obtain albedo spectra of the endmembers by inverting the Hapke model [18,19], assuming Lambertian photometric parameters. We simulate the evolution of the incidence angle with time using a similar model to that of Eq.…”
Section: Resultsmentioning
confidence: 99%
“…20 will be used for training, and 10 will be used for testing. Then we plug the angles in a simplified version of the Hapke model [19] to obtain reflectance spectra (in the same way for each material, hence we drop the index p here):…”
Section: Resultsmentioning
confidence: 99%
“…where Ψ ∈ R L h ×P is a matrix of positive scaling factors and • denotes the Hadamard product. This model can represent spectral variability caused by seasonal changes [31], [32], global illumination [34], [37] or global atmospheric variations [38], [39]. Then, the image fusion problem can finally be formulated as the problem of recovering the matrices M h , Ψ and A from the observed HS and MS images Y h and Y m .…”
Section: A the Proposed Modelmentioning
confidence: 99%
“…However, this model is much too complex to be directly used in blind unmixing, and also depends on many empirical parameters (the albedo of the materials, the acquisition angles, photometric parameters of each material), which are rarely (if at all) available in real scenarios. The application of Hapke model to generate variants of a given spectrum was theoretically and experimentally shown, however, to be reasonably approximated by (nonnegative) scaling variations of this signature [26]- [29], i.e. we can reasonably model S n = ψ n S 0 , where ψ n is a scaling factor accounting for brightness variations of a reference endmember matrix S 0 .…”
Section: A Illumination-induced Variabilitymentioning
confidence: 99%