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Non-linear fully-constrained spectral
             unmixing.

   Rob Heylen, Dẑevdet Burazerović, Paul Scheunders
       IBBT-Visionlab, University of Antwerp, Belgium



                       IGARSS 2011
              July 25-29, Vancouver, Canada




                                                        1
Outline
•   Introduction: Spectral unmixing
•   Non-linear endmember extraction
•   Distance-based unmixing algorithm
•   Results
•   Conclusions and future work




                                              2
Spectral unmixing
  The linear mixing model



  Non-linear mixing models are far more generic



  One does not always know the function F:
• Model-based unmixing
• Data-driven manifold techniques



                                              3
Non-linear unmixing
A data driven, fully-constrained non-linear
unmixing method:

• Endmember extraction by combining graph-
based manifold learning with N-findR.

• Unmixing via a distance-geometry based fully-
constrained unmixing algorithm, applied to the
geodesic distances.




                                              4
Distance geometry
All properties are expressed as (Euclidean)
distances between the constituents.




                                              5
Endmember extraction


• Rewrite N-findR to work with mutual distances.
e.g.:




• Use approximate geodesic distances on the
data manifold: Shortest-path distances in
nearest-neighbor graph



                                               6
Endmember extraction




                   7
Non-linear unmixing


Next step: Unmix the data to find abundances of
each pixel.

Aim: Use geodesic distance matrix as input of
the unmixing algorithm.

The DSPU algorithm is fit for this task.




                                                8
The minimization problem
Linear spectral unmixing can be viewed as a
minimization problem



Simplex projection is equivalent problem:




                                              9
Simplex projection unmixing
Recursive simplex projection unmixing (SPU)
algorithm:

1. Project the point orthogonally onto the
simplex plane.
2. If the point lies inside the simplex, finish.
3. Else, find which abundance has to be zero.
4. Remove the endmember from the set of
endmembers and go to step 1.

Can be expressed in distance geometry: DSPU

                                                   10
Results: Cuprite data set
• Cuprite data set
• Linear unmixing via N-findR and FCLSU/DSPU
• Non-linear unmixing via the proposed method




                                            11
Cuprite: Linear unmixing
Typical situation: 99.7% of abundances differ by
less than 10-7 . E.g. for the alunite endmember:




        FCLSU                     DSPU

                                              12
Cuprite: Non-linear EEA
Kaolinite 0.056, Montmorrilonite 0.048, Alunite 0.043




                                                13
Cuprite: Non-linear unmixing
Alunite endmember:




 N-findR + FCLSU       Non-lin. EEA + DSPU

                                       14
Conclusions and future work
• A data-driven non-linear unmixing algorithm.
• Promising results on artificial data.
• Significant deviations from linear unmixing
results. Hard to quantify on Cuprite data set.



• Assess method on non-linearly mixed data with
ground truth.
• Lots of testing



                                             15

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NON-LINEAR FULLY-CONSTRAINED SPECTRAL UNMIXING

  • 1. Non-linear fully-constrained spectral unmixing. Rob Heylen, Dẑevdet Burazerović, Paul Scheunders IBBT-Visionlab, University of Antwerp, Belgium IGARSS 2011 July 25-29, Vancouver, Canada 1
  • 2. Outline • Introduction: Spectral unmixing • Non-linear endmember extraction • Distance-based unmixing algorithm • Results • Conclusions and future work 2
  • 3. Spectral unmixing The linear mixing model Non-linear mixing models are far more generic One does not always know the function F: • Model-based unmixing • Data-driven manifold techniques 3
  • 4. Non-linear unmixing A data driven, fully-constrained non-linear unmixing method: • Endmember extraction by combining graph- based manifold learning with N-findR. • Unmixing via a distance-geometry based fully- constrained unmixing algorithm, applied to the geodesic distances. 4
  • 5. Distance geometry All properties are expressed as (Euclidean) distances between the constituents. 5
  • 6. Endmember extraction • Rewrite N-findR to work with mutual distances. e.g.: • Use approximate geodesic distances on the data manifold: Shortest-path distances in nearest-neighbor graph 6
  • 8. Non-linear unmixing Next step: Unmix the data to find abundances of each pixel. Aim: Use geodesic distance matrix as input of the unmixing algorithm. The DSPU algorithm is fit for this task. 8
  • 9. The minimization problem Linear spectral unmixing can be viewed as a minimization problem Simplex projection is equivalent problem: 9
  • 10. Simplex projection unmixing Recursive simplex projection unmixing (SPU) algorithm: 1. Project the point orthogonally onto the simplex plane. 2. If the point lies inside the simplex, finish. 3. Else, find which abundance has to be zero. 4. Remove the endmember from the set of endmembers and go to step 1. Can be expressed in distance geometry: DSPU 10
  • 11. Results: Cuprite data set • Cuprite data set • Linear unmixing via N-findR and FCLSU/DSPU • Non-linear unmixing via the proposed method 11
  • 12. Cuprite: Linear unmixing Typical situation: 99.7% of abundances differ by less than 10-7 . E.g. for the alunite endmember: FCLSU DSPU 12
  • 13. Cuprite: Non-linear EEA Kaolinite 0.056, Montmorrilonite 0.048, Alunite 0.043 13
  • 14. Cuprite: Non-linear unmixing Alunite endmember: N-findR + FCLSU Non-lin. EEA + DSPU 14
  • 15. Conclusions and future work • A data-driven non-linear unmixing algorithm. • Promising results on artificial data. • Significant deviations from linear unmixing results. Hard to quantify on Cuprite data set. • Assess method on non-linearly mixed data with ground truth. • Lots of testing 15