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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Bivariate Pearson Distributions for Radar andOptical Remote Sensing Images.
M. Chabert and J.-Y. Tourneret
University of Toulouse, IRIT-ENSEEIHT-TeSA, Toulouse, France
{ marie.chabert,jean-yves.tourneret }@enseeiht.fr
IGARSS 2011
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Outline
I Problem formulation
I The univariate Pearson system
I The multivariate Pearson system
I Method of moments
I Performance analysis
I Conclusion
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Problem formulation
Problem Formulation
Images provided by the CNES, Toulouse, France
Optical imageAirborne PELICAN
Synthetic Aperture Radar (SAR)image TerraSAR-X sensor
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Problem formulation
Multivariate Distribution
ApplicationsI change detectionI image registration
Extraction of relevant parametersI correlation coefficient [Tourneret et al. IGARSS09],I mutual information [Chatelain et al. IEEE Trans. IP 2007],I Kullback divergence [Inglada IGARSS03].
Previous work on multi-date SAR imagesI multivariate Gamma distributions
[Chatelain et al. IEEE Trans. IP 2007].
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Problem formulation
Multivariate Distribution for Heterogeneous Data
Previous works on optical image and databaseI Bivariate distribution for Gaussian and thresholded Gaussian
random variables [Tourneret et al. IGARSS09].
Previous works on optical and/or SAR image and database:I logistic regression model [Chabert et al. IGARSS10].
Optical image SAR image Database5 / 25
Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Problem formulation
Marginal Distributions
Optical images
I Gaussian distribution for the residual noise [Tupin, Wiley 2010].
SAR images [Oliver and Quegan, Artech House 1998]
I Single lookI At low resolution: Gaussian complex field with Rayleigh
amplitude and negative exponential intensityI At higher resolution: log-normal distribution for the
intensity of build-up areas, Weibull distribution for ocean, landand sea-ice clutters...
I Multi-lookI Gamma distribution for intensity images.
I Flexible modelUnivariate Pearson system [Inglada IGARSS03],[Delignon et al. IEE Proc. Radar, Sonar, Nav. 1997].
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Univariate Pearson system
Univariate Pearson System
Probability density function defined by the following differentialequation [Nagahara 2004]
−p′(x)
p(x)=
b0 + b1x
c0 + c1x+ c2x2
8 types defined by β1 = E[X3]2 (squared skewness) and β2 = E[X4](kurtosis)
I type 0: Gaussian
I type I: Beta with β1 6= 0
I type II: Beta with β1 = 0
I type III: Gamma
I type IV: non standard
I type V: Inverse-gamma
I type VI: F
I type VII: Student
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Univariate Pearson system
Univariate Pearson System
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Multivariate Pearson system
Multivariate Pearson System
General definition [Nagahara 2004]The random vector X defined by
X = Mξ
withI ξ a random vector with independent Pearson componentsξ1,...,ξm (E(ξj) = 0, E(ξ2
j ) = 1, E(ξ3j ) = ζj , E(ξ4
j ) = κj),I M a deterministic mixing matrix
follows a multivariate Pearson distribution with covariance matrixΣ = MMT .
Bivariate Pearson systemX = (X1, X2)T with
I M =
(m11 m12
m21 m22
)I ξ = (ξ1, ξ2)T with κ = (κ1, κ2), ζ = (ζ1, ζ2).
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Multivariate Pearson system
Moments of the Bivariate Pearson Distribution
f1 = E(X31 ) = m3
11ζ1 +m312ζ2
f2 = E(X32 ) = m3
21ζ1 +m322ζ2
f3 = E(X21X2) = m2
11m221ζ1 +m2
12m22ζ2f4 = E(X1X
22 ) = m11m
221ζ1 +m12m
222ζ2
f5 = E(X41 ) = m4
11κ1 + 6m211m
221 +m4
12κ2
f6 = E(X42 ) = m4
21κ1 + 6m222m
212 +m4
22κ2
f7 = E(X31X2) = m3
11m21κ1 + 3(m11m321 +m2
11m22m21) +m321m22κ2
f8 = E(X21X
22 )
= m211m
221κ1 + (m4
12 + 4m11m221m22 +m2
11m222) +m2
21m222κ2
f9 = E(X1X32 ) = m11m
321κ1 + 3(m22m
312 +m2
22m11m21) +m21m322κ2
f10 = E(X21 ) = m2
11 +m212
f11 = E(X22 ) = m2
22 +m212
f12 = E(X1X2) = m12(m11 +m22)
with M =
(m11 m12
m21 m22
), κ = (κ1, κ2) and ζ = (ζ1, ζ2).
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Parameter estimation
Parameter Estimation using the Method of Moments
ProblemEstimation of the mixing matrix M and the parameters ζ and κ
Method of momentsI Principle: Matching the theoretical fi and empirical momentsfi of the distribution by minimization of
J(M , ζ,κ) =
12∑i=1
wi
[fi − fi
]2I Linear solution
I estimation of M from the covariance matrix estimateΣ = 1
n
∑nl=1X(l)XT (l) and Σ = MMT
I estimation of ζ and κ by solving a linear system leading to theusual least-squares estimators.
I Nonlinear optimization procedure use the unconstrainedNelder-Mead simplex method (starting value obtained by thelinear method)
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Performance study
Estimation Performance - Simulated Data
I Simulated dataI 10000 realizations of independent Pearson variables ξ = (ξ1, ξ2)T
(generated using pearsrnd.m) with κ = (3,3) and ζ = (0,1)
I M =
(0.8 0.60.6 0.8
)I Parameter estimation with the method of moments
I Generation of 100000 realizations of the estimated bivariatePearson random vector
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Performance study
Estimation Performance - Simulated Data
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Performance study
Estimation Performance - Simulated Data
Mean square errors of the estimates
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Performance study
Real Data - Toulouse (France)
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Performance study
Real Data - Haıti
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Performance study
Results on Real Images (Toulouse)
Window size: n = 1050
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Performance study
Results on Real Images (Toulouse)
Window size: n = 1050
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Performance study
Results on Real Images (Toulouse)
Window size: n = 338
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Performance study
Results on Real Images (Toulouse)
Window size: n = 338
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Performance study
Results on Real Images (Haıti)
Window size: n = 26576
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Performance study
Results on Real Images (Haıti)
Window size: n = 26576
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Conclusion and future works
Conclusion and Future Works
Conclusion
I High flexibility of the multivariate Pearson system forheterogeneous data
I Parameter estimation with the method of moments
I Performance studied on synthetic and real data
Future works
I Generalized method of moments
I Method of log-moments
I Application to change detection and image registration
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Conclusion and future works
Bivariate Pearson Distributions for Radar andOptical Remote Sensing Images.
M. Chabert and J.-Y. Tourneret
University of Toulouse, IRIT-ENSEEIHT-TeSA, Toulouse, France
{ marie.chabert,jean-yves.tourneret }@enseeiht.fr
IGARSS 2011
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Bivariate Pearson Distributions for Radar and Optical Remote Sensing Images
Conclusion and future works
Real Images (Goma)
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