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Within h R
Wi hi the Resolution Cell:
               l i C ll
Super-resolution in Tomographic SAR Imaging

Xiao Xiang Zhu, Richard Bamler

Remote Sensing Technology Institute, DLR/TUM
             g         gy          ,


                       IGARSS 2011, 24-29 July 2011, Vancouver, Canada
Very high resolution acquisition (1.1×0.6m2)
Medium resolution acquisition (5×25m2)
TerraSAR-X
ERS
Very high resolution (VHR)
opens up for the first time the opportunity to use
SAR for urban infrastructure monitoring
from space ...
Problems arise ...
P bl       i
SAR Side-looking Imaging Geometry




         elevation
         angle 




                                        s




                                    r
                   x
SAR Geometry in Range-Elevation Plane




                                s
          z                         3-D reflectivity
                                    distribution
      x
              y
                                      x, r , s 

                            r
Within the Resolution Cell_Super-resolution in Tomographic SAR Imaging.pdf
Complex 3-D Structures as Imaged by SAR

Bellagio hotel, Las Vegas
interpretation difficult  real 3 D imaging required  TomoSAR
                                3-D




    Optical image, © Google Earth         TerraSAR-X spotlight mode
TomoSAR, a Spectral Estimation Problem
             Complex pixel value in acquisition n (after some phase corrections):
                          b
                                                   g n     s  exp   j 2 n s  ds
                                                                                d
                                                         s
       b
                                                   FT [ ( s )] |n , n  1,..., N
                                                      2b
                                                  n  n
                                                       r
                                              TomoSAR = spectral estimation

elevation                                               • irregular sampling
aperture                                                • small N
                                                        • motion must be considered

                                              s              s
                          z                                       3-D reflectivity
                                                                  distribution
                      x
                                y
                                                                    x, r , s 

                                                          r
TomoSAR System Model

 Discrete system model:
                                                                           
                                                                       
              g                                                        
                                           R                             γ           ε
                                                                       
                N 1
                                 
                                                           N L
                                                                          
                                                                            L1
                                                                           
          Measurements                 Irregular FT                 Elevation profile   Noise




 SVD-Wiener, a MAP estimator with white noise and prior (reference)

                               γ   R T Cεε1R  C1  R T Cεε1g
                                                     1    
                               ˆ                  γγ



                         noise covariance       prior covariance
Single + Double
Topography
                  [m]
Sparsity of the Signal in Elevation

Elevation resolution ca. 50 times worse than in azimuth and range
   Super resolution is crucial
    Super-resolution
   Signal sparse in elevation
The SL1MMER Algorithm


            Scale-down by
                                            
            L1 norm                               Compressive sensing theory

            Minimization –                        Candès 2006, Donoho 2006 Baraniuk 2007
                                                          2006
                                                   Candès &Wakin 2008
                                                                       2006,         2007,



            Model selection –
            Estimation
            Reconstruction

Proposed by Zhu et al in IGARSS 2010, offers an aesthetic non parametric realization of NLS
                   al.          2010                      non-parametric

X. Zhu, R. Bamler, Tomographic SAR Inversion by L1 Norm Regularization – The Compressive Sensing Approach,
IEEE Transactions on Geoscience and Remote Sensing, 48(10), pp. 3839-3846.
X. Zhu R Bamler Super-Resolution
X Zhu, R. Bamler, Super Resolution Power and Robustness of Compressive Sensing for Spectral Estimation with
Application to Spaceborne Tomographic SAR, IEEE Transactions on Geoscience and Remote Sensing, in press.
Scale-down by L1 Norm Minimization
                                             
                                             
                                                     under determined
                                                           under-determined system
g                 R                    γ             infinitely many solutions
                                         
  N1
             
                                NL
                                            
                                              L1
                                             
Make use of special prior ─ sparsity

 Nonlinear least squares (NLS) ─ maximum likelihood estimator (MLE)
  (Theoretically the best but NP hard)
                     best,    NP-hard)

                                       2
                γ  arg min g  Rγ 2  MS γ
                ˆ
                        γ                          0   
 Compressive sensing (CS) based sparse reconstruction algorithms
  (Convex optimization, solved b li
  (C        ti i ti       l d by linear programming)
                                                i )
                                       2
                γ  arg min g  Rγ 2  K γ
                ˆ
                        γ                      1   
Scale-down by L1 Norm Minimization

                                    
                                    
                                
g                R            γ 
                                
  N1
             
                           NL
                                   
                                     L1
                                    
Model Selection

                                  
                                  
                                                 
g             R             γ       R ( s)  
                                               ˆ        
                                                 
  N1
            
                         NL
                                                 
                                                        N K
                                                         ˆ
                                   L1
                                  
Estimation (De-biasing)

                                                       
                                                       
                                                                      
g                     R                          γ       R ( s)  
                                                                    ˆ        
                                                                      
  N1
              
                                       NL
                                                                      
                                                                             N K
                                                                              ˆ
                                                        L1
                                                       



                               
              g        R ( s) 
                               ˆ          γ ( s) 
                                               ˆ                γ ( s)   
                                                                ˆ ˆ
                                     
                                                  K1
                                                  ˆ                       K1
                                                                             ˆ
                N 1
                       
                                  N K
                                   ˆ
Super-resolution of SL1MMER — Simulation
Two scatterers inside one SAR pixel
δs: Distance between two scatterers




                  


                                                 z  40m
      z

  x          y
                             y  69m
Super-resolution of SL1MMER — Simulation
Super-resolution of SL1MMER — Simulation
Super-resolution of SL1MMER — Simulation
Key Questions


1) Can we separate two close scatterers?

2) If yes: How accurately can we estimate their
 ) y                    y
    ▫ positions,                    
    ▫ amplitudes,                           SL1MMER is an efficient estimator
    ▫ phases?                                I.e. it
                                              I its estimation accuracy approaches th
                                                      ti ti                    h the
                                              Cramér–Rao lower bound

… as a function of SNR, N, distance, phase difference, …



    X. Zhu, R. Bamler, Super-Resolution Power and Robustness of Compressive Sensing for Spectral Estimation with
    Application to Spaceborne Tomographic SAR, IEEE Transactions on Geoscience and Remote Sensing, in press.
Key Questions


1) Can we separate two close scatterers?

2) If yes: How accurately can we estimate their
 ) y                    y
    ▫ positions,        
    ▫ amplitudes,            SL1MMER is an efficient estimator
    ▫ phases?                 I.e. it
                               I its estimation accuracy approaches th
                                       ti ti                    h the
                               Cramér–Rao lower bound

… as a function of SNR, N, distance, phase difference, …
Super-Resolution, a Detection Problem

                                                             s
                                              s         :
                                                             s

                               a1        a2
                                                               s
                                    s



                       PD  SNR  N , , a1 a2 ,  

H0: single scatterer         SNR  0 ... 10dB       H1: double scatterers
  (not resolved)              N  10 ... 100             (resolved)
                                                         (resol ed)
Super-Resolution Power




                                                PD = 50%




 The definition of resolution:
  The minimum distance between two scatterers that are separable at a
  prespecified probability of detection PD
Super-resolution Factor
             s    1
   50%         
             50% 50%




                               PD = 50%
                                     0%




50%  0 4
       0.4      50%  2.5
                        25
Fundamental Bounds for SR Factors
Δφ uniformly distributed in [-π, π]




                                       . d 
                                                   SR
                                                   factors:

                                                   1.5-25
Super-resolution of SL1MMER — Real Data

Bellagio hotel, Las Vegas




    Optical image, © Google Earth   TerraSAR-X spotlight mode
Number of Scatterers

   SVD - Wiener 13% double                        SL1MMER 30% double




Blue: Null scatterers per pixel; Green: Single;    Red: Double
Super-resolution of SL1MMER — Final Proof


                                            1) SL1MMER detects
                                            much more double
                                            scatterers
                3 dB point response
                width                       2) Mainly contributed by
                                            the SR power




                                       s
  Normalized elevation distance    :
                                       s
Bellagio Hotel in 3D
Conclusions

 VHR tomographic SAR inversion is able to reconstruct the shape and
  motion of individual buildings and city areas
                                          areas.

 Super-resolution is crucial and possible.

 The achievable super-resolution factors with the newly proposed
  SL1MMER algorithm in the typical parameter range of tomographic SAR
  are found to be promising and are on the order 1.5~25.

 SL1MMER algorithm is an efficient estimator, and offers an aesthetic
  non-parametric realization of NLS
City Tour
                Cit T




Thanks to Y. Wang & G.Hochleitner for visualization

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Within the Resolution Cell_Super-resolution in Tomographic SAR Imaging.pdf

  • 1. Within h R Wi hi the Resolution Cell: l i C ll Super-resolution in Tomographic SAR Imaging Xiao Xiang Zhu, Richard Bamler Remote Sensing Technology Institute, DLR/TUM g gy , IGARSS 2011, 24-29 July 2011, Vancouver, Canada
  • 2. Very high resolution acquisition (1.1×0.6m2) Medium resolution acquisition (5×25m2) TerraSAR-X ERS
  • 3. Very high resolution (VHR) opens up for the first time the opportunity to use SAR for urban infrastructure monitoring from space ...
  • 5. SAR Side-looking Imaging Geometry elevation angle  s r x
  • 6. SAR Geometry in Range-Elevation Plane s z 3-D reflectivity distribution x y   x, r , s  r
  • 8. Complex 3-D Structures as Imaged by SAR Bellagio hotel, Las Vegas interpretation difficult  real 3 D imaging required  TomoSAR 3-D Optical image, © Google Earth TerraSAR-X spotlight mode
  • 9. TomoSAR, a Spectral Estimation Problem Complex pixel value in acquisition n (after some phase corrections): b g n     s  exp   j 2 n s  ds  d s b  FT [ ( s )] |n , n  1,..., N 2b n  n r TomoSAR = spectral estimation elevation • irregular sampling aperture • small N • motion must be considered s s z 3-D reflectivity distribution x y   x, r , s  r
  • 10. TomoSAR System Model  Discrete system model:         g       R γ  ε         N 1      N L      L1   Measurements Irregular FT Elevation profile Noise  SVD-Wiener, a MAP estimator with white noise and prior (reference) γ   R T Cεε1R  C1  R T Cεε1g  1  ˆ γγ noise covariance prior covariance
  • 12. Sparsity of the Signal in Elevation Elevation resolution ca. 50 times worse than in azimuth and range  Super resolution is crucial Super-resolution  Signal sparse in elevation
  • 13. The SL1MMER Algorithm Scale-down by  L1 norm  Compressive sensing theory Minimization –  Candès 2006, Donoho 2006 Baraniuk 2007 2006 Candès &Wakin 2008 2006, 2007, Model selection – Estimation Reconstruction Proposed by Zhu et al in IGARSS 2010, offers an aesthetic non parametric realization of NLS al. 2010 non-parametric X. Zhu, R. Bamler, Tomographic SAR Inversion by L1 Norm Regularization – The Compressive Sensing Approach, IEEE Transactions on Geoscience and Remote Sensing, 48(10), pp. 3839-3846. X. Zhu R Bamler Super-Resolution X Zhu, R. Bamler, Super Resolution Power and Robustness of Compressive Sensing for Spectral Estimation with Application to Spaceborne Tomographic SAR, IEEE Transactions on Geoscience and Remote Sensing, in press.
  • 14. Scale-down by L1 Norm Minimization           under determined under-determined system g    R  γ   infinitely many solutions         N1      NL      L1   Make use of special prior ─ sparsity  Nonlinear least squares (NLS) ─ maximum likelihood estimator (MLE) (Theoretically the best but NP hard) best, NP-hard)  2 γ  arg min g  Rγ 2  MS γ ˆ γ 0   Compressive sensing (CS) based sparse reconstruction algorithms (Convex optimization, solved b li (C ti i ti l d by linear programming) i )  2 γ  arg min g  Rγ 2  K γ ˆ γ 1 
  • 15. Scale-down by L1 Norm Minimization           g    R  γ          N1      NL      L1  
  • 16. Model Selection             g    R  γ  R ( s)   ˆ            N1      NL       N K  ˆ   L1  
  • 17. Estimation (De-biasing)             g    R  γ  R ( s)   ˆ            N1      NL       N K  ˆ   L1       g    R ( s)  ˆ  γ ( s)  ˆ γ ( s)    ˆ ˆ        K1 ˆ   K1 ˆ   N 1      N K  ˆ
  • 18. Super-resolution of SL1MMER — Simulation Two scatterers inside one SAR pixel δs: Distance between two scatterers  z  40m z x y y  69m
  • 19. Super-resolution of SL1MMER — Simulation
  • 20. Super-resolution of SL1MMER — Simulation
  • 21. Super-resolution of SL1MMER — Simulation
  • 22. Key Questions 1) Can we separate two close scatterers? 2) If yes: How accurately can we estimate their ) y y ▫ positions,  ▫ amplitudes,   SL1MMER is an efficient estimator ▫ phases?  I.e. it I its estimation accuracy approaches th ti ti h the Cramér–Rao lower bound … as a function of SNR, N, distance, phase difference, … X. Zhu, R. Bamler, Super-Resolution Power and Robustness of Compressive Sensing for Spectral Estimation with Application to Spaceborne Tomographic SAR, IEEE Transactions on Geoscience and Remote Sensing, in press.
  • 23. Key Questions 1) Can we separate two close scatterers? 2) If yes: How accurately can we estimate their ) y y ▫ positions,  ▫ amplitudes,   SL1MMER is an efficient estimator ▫ phases?  I.e. it I its estimation accuracy approaches th ti ti h the Cramér–Rao lower bound … as a function of SNR, N, distance, phase difference, …
  • 24. Super-Resolution, a Detection Problem s s  : s a1 a2 s s PD  SNR  N , , a1 a2 ,   H0: single scatterer SNR  0 ... 10dB H1: double scatterers (not resolved) N  10 ... 100 (resolved) (resol ed)
  • 25. Super-Resolution Power PD = 50%  The definition of resolution: The minimum distance between two scatterers that are separable at a prespecified probability of detection PD
  • 26. Super-resolution Factor s 1  50%    50% 50% PD = 50% 0% 50%  0 4 0.4   50%  2.5  25
  • 27. Fundamental Bounds for SR Factors Δφ uniformly distributed in [-π, π]  . d  SR factors: 1.5-25
  • 28. Super-resolution of SL1MMER — Real Data Bellagio hotel, Las Vegas Optical image, © Google Earth TerraSAR-X spotlight mode
  • 29. Number of Scatterers  SVD - Wiener 13% double  SL1MMER 30% double Blue: Null scatterers per pixel; Green: Single; Red: Double
  • 30. Super-resolution of SL1MMER — Final Proof 1) SL1MMER detects much more double scatterers 3 dB point response width 2) Mainly contributed by the SR power s Normalized elevation distance  : s
  • 32. Conclusions  VHR tomographic SAR inversion is able to reconstruct the shape and motion of individual buildings and city areas areas.  Super-resolution is crucial and possible.  The achievable super-resolution factors with the newly proposed SL1MMER algorithm in the typical parameter range of tomographic SAR are found to be promising and are on the order 1.5~25.  SL1MMER algorithm is an efficient estimator, and offers an aesthetic non-parametric realization of NLS
  • 33. City Tour Cit T Thanks to Y. Wang & G.Hochleitner for visualization