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EOS 840 Hyperspectral Imaging Applications

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1. EOS 840 Hyperspectral Imaging Applications. October 20, 2004 Week 8. Ron Resmini ... Distinguishing sky lights from unbroken tube roof ... – PowerPoint PPT presentation

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Title: EOS 840 Hyperspectral Imaging Applications


1
EOS 840 Hyperspectral Imaging Applications
October 20, 2004 Week 8
Ron Resmini v 703-735-3899 ronald.g.resmini_at_boein
g.com Office hours by appointment
2
Outline
  • Reading for next week
  • Review/context/a thread...
  • Algorithms...continued
  • My semester project status
  • Your semester project status

3
Reading Assignment
  • Read chapters 11 and 12 in Richards and Jia
    (1999)
  • Be prepared to discuss the problems at the endof
    each of the chapters in class next week
  • I.e., read the problems make mental notes be
    able to sayat least 1 or 2 sentences addressing
    the issue(s)
  • You will be called on to lead a discussion
  • Im not looking for the right answer Im looking
    forhow youd think about/approach/attack
    problemsand issues in RS
  • Theres no grade and no right/wrong I just want
    tohave another seminar-like discussion
  • Traditional classification vs. HSI methods...

4
Review/Context/A Thread...
5
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6
Algorithms for Information Extraction...Why?
Use HSI for Material...
  • Detection
  • Identification
  • Characterization
  • Quantification

BTW...the inverse of the covariance matrix...
Page 348 of Richards and Jia (1999)
7
Algorithms (continued)
8
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9
(Remind me to cover this topic as we gothrough
the algorithm classes. Thanks!)
10
The Mixed Pixel Spectral Mixture Analysis
(SMA) (review/continued)
11
  • The mixed pixel
  • Building a mixed pixel - ENVI, MS Excel
  • Linear spectral mixture analysis
  • Determining quantity of material
  • Endmember selection
  • Manual
  • Convex hull
  • Pixel-Purity Index (PPI)
  • Adaptive/updating/pruning...
  • Other (e.g., N-FINDR, ORASIS, URSSA, etc...)
  • Wild outliers

12
  • Spectral mixture analysis
  • applications
  • scene characterization
  • material mapping
  • anomaly detection
  • other...

13
A linear equation...
x
A
b
5 endmembers in a 7-band spectral data set
14
  • Unmixing inversion
  • Interpretation of results
  • RMS, RSS, algebraic and geometricinterpretations
    (pg. 155 of Strang, 1988)
  • Band residual cube
  • Iterative process
  • Fraction-plane color-composites
  • Change detection with fraction planes
  • Inversion constraints?...
  • Application strategies (i.e., in-scenespectra/lib
    rary spectra)

15
  • application strategies (continued)
  • directed search? anomaly detection?
  • Shade/shadow
  • shade endmember
  • shade removal
  • Other...
  • objective endmember determinationTompkins et al.

16
  • Is the mixing linear?
  • Non-linear spectral mixture analysis
  • Checker-board mixtures
  • Intimate mixtures
  • Spectral transformations (e.g., SSA)and use of
    ENVI

17
...Recap Where have we been? Where are we
going? BTW...Always do the math!
  • More on the statistical characterizationof
    multi-dimensional data
  • Covariance matrices
  • Eigenvectors of the covariance matrix
  • Geometric interpretation
  • Half-way to PCA...
  • Statistics with ENVI

18
  • Orthogonal Subspace Projection (OSP)
  • Derivation in detail (next several slides...)
  • Application of the filter
  • Endmembers
  • Statistics
  • Interpretation of results
  • OSP w/endmembers unconstrained SMA
  • Different ways to apply the filter/application
    strategies(i.e., in-scene spectra/library
    spectra)

19
OSP/LPD/DSR Scene-Derived Endmembers
(Harsanyi et al., 1994)
20
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21
(No Transcript)
22
The value of xT which maximizes l is given by xT
dT
This is equivalent to Unconstrained SMA
23
Statistical Characterization of the
Background (LPD/DSR)
(Harsanyi et al., 1994)
24
(No Transcript)
25
Constrained Energy Minimization (CEM)
  • The description of CEM is similar to that of
    OSP/DSR (previous slides)
  • Like OSP and DSR, CEM is an Orthogonal Subspace
    Projection (OSP)family algorithm
  • CEM differs from OSP/DSR in the following,
    important ways
  • CEM does not simply project away the first n
    eigenvectors
  • The CEM operator is built using a weighted
    combination of theeigenvectors (all or a subset)
  • Though an OSP algorithm, the structure of CEM is
    equally readily observed bya formal derivation
    using a Lagrange multiplier
  • CEM is a commonly used statistical spectral
    matched filter
  • CEM for spectral remote sensing has been
    published on for over 10 years
  • CEM has a much longer history in the
    multi-dimensional/array signalprocessing
    literature
  • Just about all HSI tools today contain CEM or a
    variant of CEM
  • If an algorithm is using M-1d as the heart of its
    filter kernel (where M is thedata covariance
    matrix and d is the spectrum of the target of
    interest), thenthat algorithm is simply a CEM
    variant

26
  • The statistical spectral matched filter (SSMF)
  • Derivation in detail
  • Application of the filter
  • Statistics
  • Endmembers (FBA/MCEM)
  • Interpretation of results
  • Many algorithms are actually the basic SSMF
  • Different ways to apply the filter/application
    strategies(i.e., in-scene spectra/library
    spectra)
  • Matched filter in ENVI

27
Derivation taken from
Stocker, A.D., Reed, I.S., and Yu, X., (1990).
Multi-dimensional signal processing for
electro-Optical target detection. In Signal
and Data Processing of Small Targets 1990,
Proceedingsof the SPIE, v. 1305, pp. 218-231.
J of Bands
Form the log-likelihood ratio test of Hº and H1
28
Some algebra...
29
A trick...recast as a univariable problem
After lots of simple algebra applied to the r.h.s
Now, go back to matrix-vector notation
30
Take the natural log
31
Constrained Energy Minimization (CEM)
(Harsanyi et al., 1994)
32
(No Transcript)
33
An Endnote...
  • Previous techniques exploit shape and albedo
  • this can cause problems...
  • Sub-classes of algorithms developed to mitigate
    this
  • shape, only, operators
  • MED, RSD of ASIT, Inc.
  • MTMF of ENVI

34
Last Class of Algorithms
  • Spectral feature fitting/derivativespectroscopy
  • Spectral parameterizations
  • Wavelets
  • Band depth/band depth mapping
  • Application strategies (i.e., in-scenespectra/lib
    rary spectra)
  • Mixed pixels...

35
Another Endnote...
  • Performance prediction/scoring/NP-Theory, etc...
  • Hybrid techniques
  • still some cream to be skimmed...
  • Caveat emptor...
  • lots of reproduction of work already accomplished
  • who invented what? when?
  • waste of resources
  • please do your homework!read the lit.!

36
My Semester Project Status
  • Tools/approach
  • 1D and 2D analytical solutions to heat equation
  • FlexPDE finite element modeling
  • Data analysis with ENVI
  • Analytical solutions to 1D and 2D heat equation
  • Additional TIMS data analysis in ENVI
  • TES on going (this is a challenge)
  • Literature research on-going
  • Additional modeling with FlexPDE
  • Dealing with (as yet) unconstrained parameters

37
Surface Temperature vs. Lava Tube Roof Thickness
Tenviron 0º C TLava 1200º C
38
Numerical 2D Modeling
39
(No Transcript)
40
Analytical solution to
On the following
(Tenviron 0º C)
Y 0
Radiative boundary condition added
Y D
41
The Solution
and
D Lava tube roof thickness
Solve with a root-finding algorithm
42
Another Approach...
43
X0
XL
Y0

YD
X0
XL
Y0
Y0

YD
YD
44
The Solution
Technique Principle of superposition and
separation of variables
Evaluate the boundary condition at y D
Evaluate the coefficients
45
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46
The B.C. at Y D
At y D
47
My Semester Project Issues
  • Constraining the value of h
  • What should the diameter of the lava tube be?
  • Distinguishing sky lights from unbroken tube roof
  • Widely ranging surface temperatures in the data
  • Validity of B.C.s used in modeling
  • Radiative upper B.C.?
  • Mapping/contouring roof thickness throughoutthe
    entire TIMS Kilauea scene
  • Need to double-check my math!
  • Other...

48
Your Semester Project Status
49
Backup Slides
50
Lagrange Multiplier Derivation of CEM Filter
Minimizing E is equivalent to minimizing each yi2
(for k 1, 2, 3, ... )
51
In Matrix Notation
52
(No Transcript)
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