TY - GEN
T1 - Kernel-based weighted abundance constrained linear spectral mixture analysis
AU - Liu, Keng Hao
AU - Wong, Englin
AU - Chang, Chein I.
PY - 2011
Y1 - 2011
N2 - Linear Spectral Mixture Analysis (LSMA) is a theory developed to perform spectral unmixing where three major LSMA techniques, Least Squares Orthogonal Subspace Projection (LSOSP), Non-negativity Constrained Least Squares (NCLS) and Fully Constrained Least Squares (FCLS) for this purpose. Later on these three techniques were further extended to Fisher's LSMA (FLSMA), Weighted Abundance Constrained-LSMA (WAC-LSMA) and kernel-based LSMA (KLSMA). This paper combines both approaches of KLSMA and WACLSMA to derive a most general version of LSMA, Kernel-based WACLSMA (KWAC-LSMA) which includes all the above-mentioned LSMAs as its special cases. The utility of the KWAC-LSMA is further demonstrated by multispectral and hyperspectral experiments for performance analysis.
AB - Linear Spectral Mixture Analysis (LSMA) is a theory developed to perform spectral unmixing where three major LSMA techniques, Least Squares Orthogonal Subspace Projection (LSOSP), Non-negativity Constrained Least Squares (NCLS) and Fully Constrained Least Squares (FCLS) for this purpose. Later on these three techniques were further extended to Fisher's LSMA (FLSMA), Weighted Abundance Constrained-LSMA (WAC-LSMA) and kernel-based LSMA (KLSMA). This paper combines both approaches of KLSMA and WACLSMA to derive a most general version of LSMA, Kernel-based WACLSMA (KWAC-LSMA) which includes all the above-mentioned LSMAs as its special cases. The utility of the KWAC-LSMA is further demonstrated by multispectral and hyperspectral experiments for performance analysis.
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U2 - 10.1117/12.884650
DO - 10.1117/12.884650
M3 - Conference contribution
AN - SCOPUS:80053000972
SN - 9780819486226
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - Algorithms and Technologies for Multispectral, Hyperspectral, and Ultraspectral Imagery XVII
T2 - Algorithms and Technologies for Multispectral, Hyperspectral, and Ultraspectral Imagery XVII
Y2 - 25 April 2011 through 28 April 2011
ER -