IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing (Jan 2021)

Constrained Nonnegative Matrix Factorization for Blind Hyperspectral Unmixing Incorporating Endmember Independence

  • E. M. M. B. Ekanayake,
  • H. M. H. K. Weerasooriya,
  • D. Y. L. Ranasinghe,
  • S. Herath,
  • B. Rathnayake,
  • G. M. R. I. Godaliyadda,
  • M. P. B. Ekanayake,
  • H. M. V. R. Herath

DOI
https://doi.org/10.1109/JSTARS.2021.3126664
Journal volume & issue
Vol. 14
pp. 11853 – 11869

Abstract

Read online

Hyperspectral unmixing (HU) has become an important technique in exploiting hyperspectral data since it decomposes a mixed pixel into a collection of endmembers weighted by fractional abundances. The endmembers of a hyperspectral image (HSI) are more likely to be generated by independent sources and be mixed in a macroscopic degree before arriving at the sensor element of the imaging spectrometer as mixed spectra. Over the past few decades, many attempts have focused on imposing auxiliary regularizes on the conventional nonnegative matrix factorization (NMF) framework in order to effectively unmix these mixed spectra. As a promising step toward finding an optimum regularizer to extract endmembers, this article presents a novel blind HU algorithm, referred to as kurtosis-based smooth nonnegative matrix factorization (KbSNMF) which incorporates a novel regularizer based on the statistical independence of the probability density functions of endmember spectra. Imposing this regularizer on the conventional NMF framework promotes the extraction of independent endmembers while further enhancing the parts-based representation of data. Experiments conducted on diverse synthetic HSI datasets (with numerous numbers of endmembers, spectral bands, pixels, and noise levels) and three standard real HSI datasets demonstrate the validity of the proposed KbSNMF algorithm compared to several state-of-the-art NMF-based HU baselines. The proposed algorithm exhibits superior performance especially in terms of extracting endmember spectra from hyperspectral data; therefore, it could uplift the performance of recent deep learning HU methods which utilize the endmember spectra as supervisory input data for abundance extraction.

Keywords