Nonnegativity Constraints in Numerical Analysis - CiteSeer
Nonnegativity Constraints in Numerical Analysis - CiteSeer
Nonnegativity Constraints in Numerical Analysis - CiteSeer
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Figure 3: Artist rendition of a JSAT satellite. Image obta<strong>in</strong>ed from the Boe<strong>in</strong>g SatelliteDevelopment Center.0.09Alum<strong>in</strong>um0.086Mylar0.0850.0840.080.0750.070.0820.080.0780.0760.0650.0740.060 0.5 1 1.5 2Wavelength, microns0.0720 0.5 1 1.5 2Wavelength, microns0.35Solar Cell0.1White Pa<strong>in</strong>t0.30.250.080.20.060.150.040.10.050.0200 0.5 1 1.5 2Wavelength, microns00 0.5 1 1.5 2Wavelength, micronsFigure 4: Laboratory spectral signatures for alum<strong>in</strong>um, mylar, solar cell, and white pa<strong>in</strong>t.For details see [70].The objective is then, given a set of spectral measurements or traces of an object, todeterm<strong>in</strong>e i) the type of constituent materials and ii) the proportional amount <strong>in</strong> which thesematerials appear. The first problem <strong>in</strong>volves the detection of material spectral signaturesor endmembers from the spectral data. The second problem <strong>in</strong>volves the computation ofcorrespond<strong>in</strong>g proportional amounts or fractional abundances. This is known as the spectralunmix<strong>in</strong>g problem <strong>in</strong> the hyperspectral imag<strong>in</strong>g community.Recall that <strong>in</strong> In Nonnegative Matrix Factorization (NMF), an m × n (nonnegative)mixed data matrix X is approximately factored <strong>in</strong>to a product of two nonnegative rankkmatrices, with k small compared to m and n, X ≈ WH. This factorization has theadvantage that W and H can provide a physically realizable representation of the mixeddata, see e.g. [68]. Two sets of factors, one as endmembers and the other as fractionalabundances, are optimally fitted simultaneously. And due to reduced sizes of factors, data24