New Method for Ship Detection Jian Yang Hongji Zhang Dept. of Electronic Eng., Tsinghua Univ. Yoshio Yamaguchi Dept. of Inform. Eng., Niigata Univ. Outline Background Polarization Entropy and Similarity Parameter GOPCE based ship detection Experiment Results Summary 1. Background Polarimetric Whitening Filter (PWF) Novak, Burl Identity Likelihood Ratio Test DeGraff HH HV VV RR LL Entropy Span Touzi Touzi’s work Optimization of Polarimetric Contrast Enhancement (OPCE) h KA g t max h KB g t subject to : g g g 1 2 1 2 2 2 3 h12 h22 h32 1 Ioannidis Hammers Kostinski Boerner Yamaguchi Yang Problem Can we employ the OPCE for ship detection? It is easy to get the average Kennaugh matrix of sea clutter, but how can we get or construct the average Kennaugh matrix of ships? Can we extend the OPCE for ship detection? 2 Polarization entropy and similarity parameters T11 T12 T13 1 U H T T12* T22 T23 U 2 * * T13 T23 T33 3 1U1U1H 2U 2U 2H 3U 3U 3H Pi i 3 3 j 1 j H Pi log 3 Pi i 1 Approximate expression From the least square method and Vieta's Theorem b c b2 AH 3.9408 2 7.5818 3 5.3008 4 a a a a Span T11 T22 T33 b T11T22 T11T33 T22T33 T12T12 T13T13 T23T23 c T The average error: 1 H AH dk dk 1 2 0.006 The Formula has a good approximation to the theoretical value of the polarization entropy Eigenvalues and logarithm are unnecessary!!! Running Time by the proposed formula is only 5% of that by the traditional approach J. Yang, Y. Chen, Y. Peng, Y. Yamaguchi, H. Yamada, “New formula of the polarization entropy”, IEICE Trans. Commun., 2006, E89-B(3), 1033-1035 Similarity parameter 1 T k shh svv , shh svv , 2shv 2 single-look case r (k1 , k2 ) 0 1 H (k ) k 0 2 1 2 k k 0 2 2 0 2 2 2 Multi-look case R(T1 , T2 ) 0 1 0 2 T ,T tr T 0 H 1 T20 0 tr T T tr T T F F 2 J. Yang, et al., “Similarity between two scattering matrices,” Electronics Letters, vol.37, no. 3, pp. 193-194, 2001. T10 T20 0 H 1 0 1 0 H 2 Similarity between a target and a plate: surface scattering 2 1 0 0 S HH SVV r1 r k , 0 2 2 0 0 0 0 2 S HH S VV 2 S HV 0 S HH S 2 0 VV 2 Span S HH S VV 2 2 2 Span Similarity between a target and a diplane: Double-bounce scattering 0 0 0 S S HH VV r2 r k , 1 2 Span 0 2 Generalized OPCE (GOPCE) based ship detection h KA g t max h KB g t subject to : g g g 1 2 1 2 2 2 3 h12 h22 h32 1 J. Yang, Y. Yamaguchi, W. -M. Boerner, S. M. Lin, “Numerical methods for solving the optimal problem of contrast enhancement,” IEEE Trans. Geosci. Remote Sensing, 2000, 38(2), pp. 965-971 GOPCE: Generalized OPCE 2 GP xi ri htm K g m i 1 3 2 3 t x r h i i m K A gm max i 1 2 3 t xi ri h m K B g m i 1 r1 r ([ S ], diag (1,1)) 2 0 0 sHH sVV 2( s r2 r ([ S ], diag (1, 1)) 2 0 HH 0 2 VV s 2 s 0 0 sHH sVV 2 2 0 2 HV ) 2 0 0 0 2 ( sHH sVV 2 sHV 2 ) r3 : Cloude entropy J. Yang, et al., “Generalized optimization of polarimetric contrast enhancement”, IEEE GRSL., vol.1, no.3, pp.171-174, 2004 GOPCE based ship detection 2 3 GP xi ri htm K g m i 1 For a sea area 2 3 min Var ( xi ri htm K g m ) i 1 subject to: x12 x22 x32 1 Average Kennaugh matrix of ships the scattering contributions of a ship direct reflection of plates double reflections of diplates of the ship some multi-reflections of the surface of the ship, or some multi-reflections between the ship and the sea surface K (TA) a K plate b K (0)diplate c K ( )diplate d K multi For example : a 0.4, b 0.5, c 0.1, d 0, 450 Experimental results NASA/JPL AirSAR over Sydney coast, Australia. Span image Experiment results K (TA) a K plate b K (0)diplate c K ( )diplate d K multi a 0.4, b 0.5, c 0.1, d 0, 450 2 3 GP xi ri htm K g m i 1 gm (1, 0.9453, -0.1497, 0.2897)t hm (1, -0.6313, 0.2925, 0.7182)t xm (-0.4000, -0.2750, 0.8743)t Experiment results Power Image by OPCE Experiment results GP Image by GOPCE Experiment results Filtered result by PWF Detection results: false alarm rate 1% span OPCE PWF GOPCE 5. Summary (1) OPCE has been developed (2) GOPCE is effective for ship detection Thank you! yangjian_ee@tsinghua.edu.cn Speckle Filtering Speckle phenomenon in SAR/POLSAR Observation Point Surface Roughness Scattering from distributed scatterers Coherent interferences of waves scattered from many randomly distributed scatterers in the resolution cell Granular Noise Speckle Phenomenon 24/28 Speckle Filtering Challenge of speckle filtering Speckle Filtering Speckle Reduction These two objectives should be achieved simultaneously Detail Preservation 25/28 Pre-test Approach for Speckle Filtering Classical Methods for Speckle Filtering Boxcar Filter 3*3 boxcar To-be-filtered pixel Pixel selected for averaging MMSE Lee’s filter with edge detector 8-direction edge detectors 26/28 Pre-test Approach for Speckle Filtering Summary of Speckle Filtering : Two-Step Methodology Selecting homogenous pixels Boxcar Lee Pre-test local area Averaging homogenous pixels In neighboring area Uniformly weight In aligned matching window By mmse criteria In non-local area patch : pixel itself and its local neighboring By the similarity of patch To-be-filtered pixel patch Pre-tested pixels non-local area : other than neighboring area pre-test : selecting homogenous pixels in non-local area by patch An example of pre-testing homogenous pixels in non-local area by patch 27/28 Pre-test Approach for Speckle Filtering Non-local but homogeneous pixels using proposed method 28/28 Pre-test Approach for Speckle Filtering For each pixel xi , yi - For each pixel xj , yj in non-local searching area 1. Calculate the similarity test Ti , j between the patches with xi , yi and x j , y j as the center respectivel 2. If test Ti , j > threshold, accept x j , y j as the homogenous pixel to xi , yi , and calculate the weight 3. Average homogenous pixels with their normalized weight to get filtered covariance matrix Calculate the similarity between 2 patches xj , yj xi , yi patch searching area of xi , yi 29/28 Pre-test Approach for Speckle Filtering Experimental Results (a) Original (b) Refined Lee SAR-Convair 580 C-band Image size : 340*220 Resolution : 6.4m*10m (c) Pre-test 30/28 C-band AirSAR data SAN Francisco area (a)Original (b)Boxcar (c)Refined Lee (d)Pre-test 4 multi-look Image size : 300*300 Resolution : About 10m*10m 31/28