以高頻譜影像分析為例
Hyperspectral Image Analysis
In the linear mixture model for hyperspectral images, all the image spectra lie on a high-dimensional simplex with corners called endmembers. Given a set of endmembers, the standard calculation of fractional abundances with constrained least squares typically identifies the spectra as combinations of most, if not all, endmembers. We instead assume that pixels are combinations of only a few endmembers, yielding abundance vectors that are sparse. We introduce Sparse Demixing (SD), a method, similar to Orthogonal Matching Pursuit (OMP), for calculating these sparse abundances. We demonstrate that SD outperforms an existing L1 demixing algorithm, which we prove depends adversely on the angles between endmembers. We combine SD with dictionary learning methods to automatically calculate endmembers for a provided set of spectra. Applying to an AVIRIS image of Cuprite, Nevada yields endmembers that compare favorably with signatures from the USGS spectral library.
Keywords: hyperspectral; demix; hsy; hyperspectral image; image; sparse; omp; abundance; spectra; usg; match pursuit; spectral library; dictionary; mixture model; nevada;
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Extreme Learning Machines (ELM)
網易公開課程
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Abstract—A significant recent advance in hyperspectral image
classification relies on the observation that the spectral signature
of a pixel can be represented by a sparse linear combination of
training spectra which come from an over-complete dictionary.
以機率密度函數估計為例
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gaussian mixture model density estimation
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Model selection - introduction and examplesLecture 08, part 1 | Pattern Recognition
the difficulty is then to select the appropriate Hilbert space E. And this is where and why Sobolev
spaces appeared.
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L. Rudin, S. Osher, and E. Fatemi. Nonlinear Total Variation based
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