4.7 Article

Adaptive Ship Detection in Hybrid-Polarimetric SAR Images Based on the Power-Entropy Decomposition

Journal

IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING
Volume 56, Issue 9, Pages 5394-5407

Publisher

IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC
DOI: 10.1109/TGRS.2018.2815592

Keywords

Compact polarization (CP); constant false-alarm rate (CFAR); ship detection; synthetic aperture radar (SAR)

Funding

  1. Outstanding Young People Scientific Research Plan of National University of Defense Technology [JQ14-04-01]
  2. Outstanding Young People of Natural Science Foundation of Hunan Province [2016JJ1004]
  3. National Natural Science Foundation of China [41171316]

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Based on its advantages, compact polarimetric (CP) synthetic aperture radar (SAR) is considered to be a good option for earth observations. This paper proposes an adaptive method of ship detection in CP SAR images operating in the hybrid-polarimetric (HP) mode. First, according to the analysis of scattering between ships and sea background, a novel decomposition approach, named power-entropy (PE) decomposition, is developed. Based on this approach, two components of the scattering power, the high-entropy scattering amplitude (HESA) and low-entropy scattering amplitude, are separated. We demonstrate that the HESA component is an effective physical quantity indicating the difference between the ship and its background and hence can potentially be used for ship detection using HP SAR data. The generalized Gamma distribution (G Gamma D) is found suitable for the characterization of HESA statistics of sea clutter with a wide range of homogeneity. As a result, the adaptive constant false-alarm rate (CFAR) technique based on the HESA detector is proposed. Experiments performed using HP measurements emulated from L-band ALOS-PALSAR and C-band RADARSAT-2 full polarimetric data validate the soundness and superiority of the proposed CFAR method based on the HESA detector. Both the theoretical proof and experimental results show that the HESA improves the ship-sea contrast (or the signal-clutter ratio) more than popular detectors, such as the entropy and SPAN. Moreover, the G Gamma D is a versatile model for the description of the statistical behavior of both the HESA and comparable detectors.

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