TY - GEN
T1 - Space object material identification of hyperspectral data using nonnegative tensor factorization
AU - Yang, Chao
AU - Cheng, Xiao Ming
AU - Shi, Zhen Wei
PY - 2011
Y1 - 2011
N2 - Among kinds of ways to improve the early-warning of a country, identifying the space object material in a better and faster way is an important and effective method. The hyperspectral image, which is a 3-D data cube and contains the spatial and spectral information of the interest objects, will play a more important role in identifying the space object material. However, the low spatial resolution of the hyperspectral remote sensing instrument makes the single pixel spectrum often mixed up several different materials'spectra, which is called mixed pixel. So it is a considerable question to decompose the mixed pixels into spectra of pure materials (called endmembers) and get their corresponding fractions (called abundances). Since a hyperspectral image can be seen as a 3-D tensor, nonnegative tensor factorization (NTF) algorithm based on tensor analysis can be introduced into the field of hyperspectral unmixing. However, random initialization, a classical way to initialize the NTF algorithm, causes a slow rate of convergence, which can be improved through other methods to initialize this algorithm. This paper selects the vertex component analysis (VCA) algorithm to initialize the NTF algorithm. In this way, a faster and better result is obtained, and furthermore, four simulated hyperspectral images dataset of 3-D model of Hubble Space Telescope with different spatial resolutions are processed by the improved algorithm in this paper, and good results are obtained.
AB - Among kinds of ways to improve the early-warning of a country, identifying the space object material in a better and faster way is an important and effective method. The hyperspectral image, which is a 3-D data cube and contains the spatial and spectral information of the interest objects, will play a more important role in identifying the space object material. However, the low spatial resolution of the hyperspectral remote sensing instrument makes the single pixel spectrum often mixed up several different materials'spectra, which is called mixed pixel. So it is a considerable question to decompose the mixed pixels into spectra of pure materials (called endmembers) and get their corresponding fractions (called abundances). Since a hyperspectral image can be seen as a 3-D tensor, nonnegative tensor factorization (NTF) algorithm based on tensor analysis can be introduced into the field of hyperspectral unmixing. However, random initialization, a classical way to initialize the NTF algorithm, causes a slow rate of convergence, which can be improved through other methods to initialize this algorithm. This paper selects the vertex component analysis (VCA) algorithm to initialize the NTF algorithm. In this way, a faster and better result is obtained, and furthermore, four simulated hyperspectral images dataset of 3-D model of Hubble Space Telescope with different spatial resolutions are processed by the improved algorithm in this paper, and good results are obtained.
KW - Hyperspectral unmixing
KW - Initialization
KW - Nonnegative tensor factorization (NTF)
KW - Space object material identification
KW - Vertex component analysis (VCA)
UR - https://www.scopus.com/pages/publications/80052243940
U2 - 10.1117/12.900482
DO - 10.1117/12.900482
M3 - 会议稿件
AN - SCOPUS:80052243940
SN - 9780819488374
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - International Symposium on Photoelectronic Detection and Imaging 2011
T2 - International Symposium on Photoelectronic Detection and Imaging 2011: Space Exploration Technologies and Applications
Y2 - 24 May 2011 through 26 May 2011
ER -