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Content Provider | IEEE Xplore Digital Library |
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Author | Bin Luo Chanussot, J. Doute, S. Ceamanos, X. |
Copyright Year | 2009 |
Description | Author affiliation: GIPSA-Lab, 38402 Grenoble, France (Bin Luo; Chanussot, J.) || LPG 38041 Grenoble, France (Doute, S.; Ceamanos, X.) |
Abstract | In this paper, we try to identify and quantify the chemical species present on the surface of planet Mars with the help of hyperspectral images provided by the instrument OMEGA [1]. For this purpose, we suppose that the spectrum of each pixel is a linear mixture of the spectra of different endmembers. From this linear mixture hypothesis, our work is divided into two steps. Firstly, we propose a new unsupervised method for estimating the number of endmembers based on the eigenvalues of covariance and correlation matrix of the hyperspectral data. This method is then validated on synthetic data. With the help of the number estimated by the precedent step, we use the Vertex Component Analysis (VCA) to extract the spectra and the abundances of the endmembers. The results on hyperspectral image acquired by the OMEGA instrument are shown. |
Starting Page | 1 |
Ending Page | 4 |
File Size | 908327 |
Page Count | 4 |
File Format | |
ISBN | 9781424446865 |
DOI | 10.1109/WHISPERS.2009.5289070 |
Language | English |
Publisher | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
Publisher Date | 2009-08-26 |
Publisher Place | France |
Access Restriction | Subscribed |
Rights Holder | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
Subject Keyword | Mars Hyperspectral sensors Planets Instruments Independent component analysis Eigenvalues and eigenfunctions Covariance matrix Data mining Chemicals Hyperspectral imaging |
Content Type | Text |
Resource Type | Article |
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