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Dark endmember in spectral feature space under variable atmosphere [PDF]
One of the most important assumptions in most multispectral image transformation methods is that the position of the dark endmember is placed at the origin of the n-D spectral feature space regardless of the target spectral signature. A series of field experiments under varying illumination resulted that ‘shadowlines’, which hypothetically pass through
Choi, K.Y., Milton, E.J.
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A novel inequality-constrained weighted linear mixture model for endmember variability
Remote Sensing of Environment, 2021Fengting Li, Jianqing Cai
exaly
Proportional Perturbation Model for Hyperspectral Unmixing Accounting for Endmember Variability
IEEE Geoscience and Remote Sensing LettersWei Gao 0021, Jingyu Yang, Jie Chen 0022
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Hyperspectral unmixing with shared endmember variability in homogeneous region
Optics and Precision EngineeringNing WANG +3 more
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Variable Multiple Endmember Spectral Mixture Analysis for Geology Applications
2004Klaas Scholte +2 more
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