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Time Reversal Techniques in Wave Imaging andApplications
Abdul WahabLPMA, University of Paris VII,
&CMAP, Ecole Polytechnique,
France.
CAMP, National University of Science & Technology,Pakistan.
Joint work with H. Ammari (ENS-Paris), E. Bretin (INSA-Lyon), J. Garnier (Paris VII),
S. Gdoura (Supelec-Paris), D. Lesselier (Supelec-Paris)
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 1 / 57
Outlines
Principles of Time Reversal
Inverse Source Problems
Time Reversal Cavity
Applications of Time Reversal
Open Questions
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 1 / 57
Principle of Time reversalIntroduced by M. Fink (Paris VII & ESPCI) in 1989.
The wave equation with compressibility K, density ρ and speed c = 1/√ρK :
W[u](x, t) :=
(∇ ·
1
ρ∇−
1
ρc2∂2
∂t2
)u(x, t) = 0, x ∈ Rd.
is time invariant (under transformation t→ −t).If u(x, t) is solution then so does u(x,−t) !
The fundamental solution, G, to the operator W verifies spatial reciprocity i.e.
G(x− y, t) = G(y − x, t), ∀x, y ∈ Rd, x 6= y.
One can revert a wave from its final state to initial state.
Time reversalIt is a technique that focuses waves onto a source or a scatter by emitting a time reversedversion of the received wave field measured by an array of transducers.(C. Bardos, 09)
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 2 / 57
Principle of Time reversalIntroduced by M. Fink (Paris VII & ESPCI) in 1989.
The wave equation with compressibility K, density ρ and speed c = 1/√ρK :
W[u](x, t) :=
(∇ ·
1
ρ∇−
1
ρc2∂2
∂t2
)u(x, t) = 0, x ∈ Rd.
is time invariant (under transformation t→ −t).If u(x, t) is solution then so does u(x,−t) !
The fundamental solution, G, to the operator W verifies spatial reciprocity i.e.
G(x− y, t) = G(y − x, t), ∀x, y ∈ Rd, x 6= y.
One can revert a wave from its final state to initial state.
Time reversalIt is a technique that focuses waves onto a source or a scatter by emitting a time reversedversion of the received wave field measured by an array of transducers.(C. Bardos, 09)
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 2 / 57
Principle of Time reversalIntroduced by M. Fink (Paris VII & ESPCI) in 1989.
The wave equation with compressibility K, density ρ and speed c = 1/√ρK :
W[u](x, t) :=
(∇ ·
1
ρ∇−
1
ρc2∂2
∂t2
)u(x, t) = 0, x ∈ Rd.
is time invariant (under transformation t→ −t).If u(x, t) is solution then so does u(x,−t) !
The fundamental solution, G, to the operator W verifies spatial reciprocity i.e.
G(x− y, t) = G(y − x, t), ∀x, y ∈ Rd, x 6= y.
One can revert a wave from its final state to initial state.
Time reversalIt is a technique that focuses waves onto a source or a scatter by emitting a time reversedversion of the received wave field measured by an array of transducers.(C. Bardos, 09)
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 2 / 57
Principle of Time reversalIntroduced by M. Fink (Paris VII & ESPCI) in 1989.
The wave equation with compressibility K, density ρ and speed c = 1/√ρK :
W[u](x, t) :=
(∇ ·
1
ρ∇−
1
ρc2∂2
∂t2
)u(x, t) = 0, x ∈ Rd.
is time invariant (under transformation t→ −t).If u(x, t) is solution then so does u(x,−t) !
The fundamental solution, G, to the operator W verifies spatial reciprocity i.e.
G(x− y, t) = G(y − x, t), ∀x, y ∈ Rd, x 6= y.
One can revert a wave from its final state to initial state.
Time reversalIt is a technique that focuses waves onto a source or a scatter by emitting a time reversedversion of the received wave field measured by an array of transducers.(C. Bardos, 09)
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 2 / 57
Principle of Time reversalIntroduced by M. Fink (Paris VII & ESPCI) in 1989.
The wave equation with compressibility K, density ρ and speed c = 1/√ρK :
W[u](x, t) :=
(∇ ·
1
ρ∇−
1
ρc2∂2
∂t2
)u(x, t) = 0, x ∈ Rd.
is time invariant (under transformation t→ −t).If u(x, t) is solution then so does u(x,−t) !
The fundamental solution, G, to the operator W verifies spatial reciprocity i.e.
G(x− y, t) = G(y − x, t), ∀x, y ∈ Rd, x 6= y.
One can revert a wave from its final state to initial state.
Time reversalIt is a technique that focuses waves onto a source or a scatter by emitting a time reversedversion of the received wave field measured by an array of transducers.(C. Bardos, 09)
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 2 / 57
Principle of Time reversalAcoustic Time-reversal Cavity : Physical Experiment
Time reversal of a scattered wave by an obstacle. [Fink 99]
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 3 / 57
Principle of Time reversalAcoustic Time-reversal Cavity : Physical Experiment
Time reversal of a scattered wave by an obstacle. [Fink 99]
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 3 / 57
Principle of Time reversalAcoustic Time-reversal Cavity : Physical Experiment
Time reversal of a scattered wave by an obstacle. [Fink 99]
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 3 / 57
Principle of Time reversalAcoustic Time-reversal Cavity : Physical Experiment
Time reversal of a scattered wave by an obstacle. [Fink 99]
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 3 / 57
Principle of Time reversalAcoustic Time-reversal Cavity : Physical Experiment
Time reversal of a scattered wave by an obstacle. [Fink 99]
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 3 / 57
Principle of Time reversalAcoustic Time-reversal Cavity : Physical Experiment
Time reversal of a scattered wave by an obstacle. [Fink 99]
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 3 / 57
Principle of Time reversalAcoustic Time-reversal Cavity : Physical Experiment
Time reversal of a scattered wave by an obstacle. [Fink 99]
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 3 / 57
Principle of Time reversalAcoustic Time-reversal Cavity : Applications
TRCGiven the measurements of wave field scattered by a (point or extended) scatterer at asurface(in far field). Find
- Properties of the medium or scatterer such as refractive index, Young’s modulus,Poisson’s ratio, electric permittivity, magnetic permeability etc.
- Find the shape (for extended scatterers) and the location of the scatterers.
Applications
- Biomedical imaging with diffracting sources.
- Non-destructive evolution.
- Exploration geophysics and seismology.
- Telecommunications.
- Synthetic aperture radar imaging.
- Passive tomography and travel time imaging.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 4 / 57
Principle of Time reversalAcoustic Time-reversal Cavity : Applications
TRCGiven the measurements of wave field scattered by a (point or extended) scatterer at asurface(in far field). Find
- Properties of the medium or scatterer such as refractive index, Young’s modulus,Poisson’s ratio, electric permittivity, magnetic permeability etc.
- Find the shape (for extended scatterers) and the location of the scatterers.
Applications
- Biomedical imaging with diffracting sources.
- Non-destructive evolution.
- Exploration geophysics and seismology.
- Telecommunications.
- Synthetic aperture radar imaging.
- Passive tomography and travel time imaging.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 4 / 57
Principle of Time reversalInverse Source Problems : Physical Experiment
Time reversal of a secondary (or modulated) wave.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 5 / 57
Principle of Time reversalInverse Source Problems : Physical Experiment
Time reversal of a secondary (or modulated) wave.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 5 / 57
Principle of Time reversalInverse Source Problems : Physical Experiment
Time reversal of a secondary (or modulated) wave.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 5 / 57
Principle of Time reversalInverse Source Problems : Physical Experiment
Time reversal of a secondary (or modulated) wave.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 5 / 57
Principle of Time reversalInverse Source Problems : Applications
ISPSuppose a primary incident wave passes through a medium and is modulated or triggers asecondary wave due to the presence of an anomaly. Given the measurements of themodulated or secondary wave field at a surface(in far field). Find the source (i.e. theanomaly) of the modulation or the secondary wave.
Applications
- Biomedical imaging with non-diffracting sources.
- Reservoir localization.
- EM source localization with applications in Robotics.
- Earthquake source localization.
- Identification of the initial state of a dynamical system.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 6 / 57
Principle of Time reversalInverse Source Problems : Applications
ISPSuppose a primary incident wave passes through a medium and is modulated or triggers asecondary wave due to the presence of an anomaly. Given the measurements of themodulated or secondary wave field at a surface(in far field). Find the source (i.e. theanomaly) of the modulation or the secondary wave.
Applications
- Biomedical imaging with non-diffracting sources.
- Reservoir localization.
- EM source localization with applications in Robotics.
- Earthquake source localization.
- Identification of the initial state of a dynamical system.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 6 / 57
Principle of Time reversalSome Important Results
Physics & Experiments
- [Cassereau & Fink 92, TR Cavity], [Fink 97], [Carminati 07, EM-Waves], [Anderson11, Elastic-ISP], [Johnson, Solids and non-linear elastic media].
Mathematical Analysis
- [Bardos & Fink, TRC], [Blomgren, Papanicolaou, Zhao, Randomness Hypothesis],[Garnier, Papanicolaou, Solna, Wave guides, Layered media, Dispersive media], [Bal,Changing Environment].
Applications
- [Lerosey, Rosny, Tourin, Fink, Science 07], [Larmat 10, Seismology], [Larmat 08 Glacialearthquake], [de Rosny, Telecommunications], [Stojanovic 05, Underwater acoustics],[Gallot 11, Passive elastography].
Biomedical Imaging - [Ammari 11, Elastography], [Burgholzer 08, Photo-acoustics],[Kuchment & Hristova 08, Thermo-acoustics], [Treeby 08, Photo-aocustics].
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 7 / 57
Inverse Source Problems
Inverse Source Problems
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 8 / 57
Inverse Source ProblemsMotivation : Multi-Physics Imaging
Tissue optical absorption:
p(y,t)
f(x)
Optical pulsePhoto-acoustic imaging
- Absorbed energy density.
Magneto-acoustic imaging
- Divergence of the Lorentz force.
Acoustic radiation force imaging
- Radiation force.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 9 / 57
Inverse Source ProblemsMathematical Formulation
Let f be compactly supported in a bounded smooth domain Ω ⊂ Rd with d = 2, 3 andboundary ∂Ω.
ProblemFind supp
f(x)
given
ga(y, t) := pa(y, t) : (y, t) ∈ ∂Ω× [0, T ]
such that :
(1
c2∂2
∂t2−∆− a
∂
∂t∆
)pa(x, t) =
∂
∂tδ0(t)f(x), (x, t) ∈ Rd × R,
pa(x, t) = 0 =∂pa(x, t)
∂t, x ∈ Rd, t 0,
for T sufficiently large.
- a ≥ 0 : Medium dependant attenuation parameter,
- c : Speed of the wave front.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 10 / 57
Inverse Source ProblemsMathematical Formulation
Let f be compactly supported in a bounded smooth domain Ω ⊂ Rd with d = 2, 3 andboundary ∂Ω.
ProblemFind supp
f(x)
given
ga(y, t) := ua(y, t) : (y, t) ∈ ∂Ω× [0, T ]
such that :
(∂2
∂t2−
∂
∂tLηλ,ηµ − Lλ,µ
)ua(x, t) =
∂
∂tδ0(t)f(x), (x, t) ∈ Rd × R,
ua(x, t) = 0 =∂
∂tua(x, t), x ∈ Rd, t 0,
for T sufficiently large.
- (λ, µ) : Lame parameters,
- (ηλ, ηµ) : visco-elastic moduli,
- Lα,β [~pa] = (α+ β)∇∇ · ua − β∆ua,
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 10 / 57
Inverse Source ProblemsAcoustic Time-reversal : Integral formulation
Adjoint WaveLet v be the solution of the wave equation
∂ttv(x, t)−∆v(x, t) = 0, (x, t) ∈ Ω× (0, T )
v(x, 0) = 0, ∂tv(x, 0) = 0, x ∈ Ω
v(x, t) = g0(x, T − t), (x, t) ∈ ∂Ω× [0, T ]
Then,v(x, t) = p0(x, T − t), ∀(x, t) ∈ Ω× [0, T ], and v(x, T ) = f(x)
Exact Integral FormulationGreen’s theorem and integration by parts yield
f(x) = v(x, T ) =
∫ T
0
∫∂Ω
∂GD(x, y, t− T )
∂νyg0(y, t− T )dσ(y) ∀x ∈ Ω
where GD is the Dirichlet Green function and v is the adjoint wave.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 11 / 57
Inverse Source ProblemsAcoustic Time-reversal : Integral formulation
Adjoint WaveLet v be the solution of the wave equation
∂ttv(x, t)−∆v(x, t) = 0, (x, t) ∈ Ω× (0, T )
v(x, 0) = 0, ∂tv(x, 0) = 0, x ∈ Ω
v(x, t) = g0(x, T − t), (x, t) ∈ ∂Ω× [0, T ]
Then,v(x, t) = p0(x, T − t), ∀(x, t) ∈ Ω× [0, T ], and v(x, T ) = f(x)
Exact Integral FormulationGreen’s theorem and integration by parts yield
f(x) = v(x, T ) =
∫ T
0
∫∂Ω
∂GD(x, y, t− T )
∂νyg0(y, t− T )dσ(y) ∀x ∈ Ω
where GD is the Dirichlet Green function and v is the adjoint wave.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 11 / 57
Inverse Source ProblemsAcoustic Time-reversal : Experiment
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A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 12 / 57
Inverse Source ProblemsAcoustic Time-reversal : Experiment
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A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 12 / 57
Inverse Source ProblemsAcoustic Time-reversal : Integral formulation II
Modified TR-functionalLet G0(x, y, t) be the outgoing fundamental solution and vs(x, t) be such that
∂ttvs(x, t)−∆vs(x, t) = ∂tδs(t)g0(x, T − s)δ∂Ω(x), ∀(x, t) ∈ Rd × R,vs(x, t) = 0, ∂tvs(x, t) = 0 ∀x ∈ Rd, t s.
Then, a modified time-reversal functional is given by
I(x) :=
∫ T
0vs(x, T )ds
=
∫ T
0
∫∂Ω
∂tG0(x, y, T − s)g0(y, T − s)dσ(y)ds ∀x ∈ Ω.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 13 / 57
Inverse Source ProblemsAcoustic Time-reversal : Integral formulation II
Remark that g0(y) = −iω∫
ΩG0(z, y)f(z)dz for all y ∈ ∂Ω
Helmholtz-Kirchhoff Identity : For x, z ∈ Ω sufficiently far from y ∈ ∂Ω∫∂Ω
G0(x, y)G0(z, y)dσ(y) '1
ω=m
G0(x, z)
1
2π
∫Rω=m
G0(x, z)
dω = δx(z)
Therefore,
I(x) =1
2π
∫Rdf(z)
∫R
∫∂Ωω2G0(x, y)G0(z, y)dσ(y)dωdz
'1
2π
∫Rdf(z)
∫Rω=m
G0(x, z)
dωdz
TheoremFor x far from ∂Ω (w.r.t. wavelength), we have I(x) ' f(x).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 14 / 57
Inverse Source ProblemsAcoustic Time-reversal : Integral formulation II
Remark that g0(y) = −iω∫
ΩG0(z, y)f(z)dz for all y ∈ ∂Ω
Helmholtz-Kirchhoff Identity : For x, z ∈ Ω sufficiently far from y ∈ ∂Ω∫∂Ω
G0(x, y)G0(z, y)dσ(y) '1
ω=m
G0(x, z)
1
2π
∫Rω=m
G0(x, z)
dω = δx(z)
Therefore,
I(x) =1
2π
∫Rdf(z)
∫R
∫∂Ωω2G0(x, y)G0(z, y)dσ(y)dωdz
'1
2π
∫Rdf(z)
∫Rω=m
G0(x, z)
dωdz
TheoremFor x far from ∂Ω (w.r.t. wavelength), we have I(x) ' f(x).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 14 / 57
Inverse Source ProblemsAcoustic Time-reversal : Integral formulation II
Remark that g0(y) = −iω∫
ΩG0(z, y)f(z)dz for all y ∈ ∂Ω
Helmholtz-Kirchhoff Identity : For x, z ∈ Ω sufficiently far from y ∈ ∂Ω∫∂Ω
G0(x, y)G0(z, y)dσ(y) '1
ω=m
G0(x, z)
1
2π
∫Rω=m
G0(x, z)
dω = δx(z)
Therefore,
I(x) =1
2π
∫Rdf(z)
∫R
∫∂Ωω2G0(x, y)G0(z, y)dσ(y)dωdz
'1
2π
∫Rdf(z)
∫Rω=m
G0(x, z)
dωdz
TheoremFor x far from ∂Ω (w.r.t. wavelength), we have I(x) ' f(x).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 14 / 57
Inverse Source ProblemsAcoustic Time-reversal : Reconstructions
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Left to Right : Initial image, Exact time-reversal, Modified time-reversal
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TR in Attenuating Media
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 15 / 57
Inverse Source ProblemsAcoustic Time-reversal : Reconstructions
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Left to Right : Initial image, Exact time-reversal, Modified time-reversal
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TR in Attenuating Media
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 15 / 57
Inverse Source ProblemsAcoustic Time-reversal : TR in attenuating media
Consider the thermo-viscous wave equation∂ttpa(x, t)−∆pa(x, t)− a∂t(∆pa(x, t)) = 0
pa(x, 0) = f(x), and ∂tpa(x, 0) = 0.
Attenuated TR-functionalDefine
Ia(x) =
∫ T
0vs,a(x, T )ds ∀x ∈ Ω
where vs,a(x, t) is the solution of the adjoint attenuated wave equation [Burgholzer 07], [Treeby 10]
∂ttvs,a(x, t)−∆vs,a(x, t)+a∂t(∆vs,a(x, t)) = ∂tδs(t)ga(x, T − s)δ∂Ω(x).
- Stability,
- Order of correction,
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 16 / 57
Inverse Source ProblemsAcoustic Time-reversal : TR in attenuating media
Consider the thermo-viscous wave equation∂ttpa(x, t)−∆pa(x, t)− a∂t(∆pa(x, t)) = 0
pa(x, 0) = f(x), and ∂tpa(x, 0) = 0.
Attenuated TR-functionalDefine
Ia(x) =
∫ T
0vs,a(x, T )ds ∀x ∈ Ω
where vs,a(x, t) is the solution of the adjoint attenuated wave equation [Burgholzer 07], [Treeby 10]
∂ttvs,a(x, t)−∆vs,a(x, t)+a∂t(∆vs,a(x, t)) = ∂tδs(t)ga(x, T − s)δ∂Ω(x).
- Stability,
- Order of correction,
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 16 / 57
Inverse Source ProblemsAcoustic Time-reversal : TR in attenuating media
Consider the thermo-viscous wave equation∂ttpa(x, t)−∆pa(x, t)− a∂t(∆pa(x, t)) = 0
pa(x, 0) = f(x), and ∂tpa(x, 0) = 0.
Attenuated TR-functionalDefine
Ia(x) =
∫ T
0vs,a(x, T )ds ∀x ∈ Ω
where vs,a(x, t) is the solution of the adjoint attenuated wave equation [Burgholzer 07], [Treeby 10]
∂ttvs,a(x, t)−∆vs,a(x, t)+a∂t(∆vs,a(x, t)) = ∂tδs(t)ga(x, T − s)δ∂Ω(x).
- Stability,
- Order of correction,
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 16 / 57
Inverse Source ProblemsAcoustic Time-reversal : Truncated TR functional
LetGa be the fundamental solution of the Lossy Helmholtz equation
ω2 Ga(x, y) + (1 + iaω) ∆yGa(x, y) = −δx(y) in Rd.
Let Ga,ρ(x, y, t) :=1
2π
∫|ω|<ρ
Ga(x, y) exp(−iωt)dω
Consider an approximation vs,a,ρ(x, t) of vs,a(x, t) given by :
vs,a,ρ(x, t) =
∫∂Ω
∂tGa,ρ(x, y, t− s)ga(y, T − s)dσ(y)
We define :
Truncated TR-FunctionalFor all x ∈ Ω :
Ia,ρ(x) :=
∫ T
0vs,a,ρ(x, T )ds =
∫ T
0
∫∂Ω
∂tGa,ρ(x, y, T − s)ga(y, T − s)dσ(y)ds.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 17 / 57
Inverse Source ProblemsAcoustic Time-reversal : Truncated TR functional
LetGa be the fundamental solution of the Lossy Helmholtz equation
ω2 Ga(x, y) + (1 + iaω) ∆yGa(x, y) = −δx(y) in Rd.
Let Ga,ρ(x, y, t) :=1
2π
∫|ω|<ρ
Ga(x, y) exp(−iωt)dω
Consider an approximation vs,a,ρ(x, t) of vs,a(x, t) given by :
vs,a,ρ(x, t) =
∫∂Ω
∂tGa,ρ(x, y, t− s)ga(y, T − s)dσ(y)
We define :
Truncated TR-FunctionalFor all x ∈ Ω :
Ia,ρ(x) :=
∫ T
0vs,a,ρ(x, T )ds =
∫ T
0
∫∂Ω
∂tGa,ρ(x, y, T − s)ga(y, T − s)dσ(y)ds.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 17 / 57
Inverse Source ProblemsAcoustic Time-reversal : Truncated TR functional
LetGa be the fundamental solution of the Lossy Helmholtz equation
ω2 Ga(x, y) + (1 + iaω) ∆yGa(x, y) = −δx(y) in Rd.
Let Ga,ρ(x, y, t) :=1
2π
∫|ω|<ρ
Ga(x, y) exp(−iωt)dω
Consider an approximation vs,a,ρ(x, t) of vs,a(x, t) given by :
vs,a,ρ(x, t) =
∫∂Ω
∂tGa,ρ(x, y, t− s)ga(y, T − s)dσ(y)
We define :
Truncated TR-FunctionalFor all x ∈ Ω :
Ia,ρ(x) :=
∫ T
0vs,a,ρ(x, T )ds =
∫ T
0
∫∂Ω
∂tGa,ρ(x, y, T − s)ga(y, T − s)dσ(y)ds.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 17 / 57
Inverse Source ProblemsAcoustic Time-reversal : Attenuation operators
Remark that p0(x, ω) and pa(x, ω) satisfy(κ2(ω) + ∆
)pa(x, ω) =
iκ2(ω)
ωf(x), and
(ω2 + ∆
)p0(x, ω) = iωf(x).
Therefore, pa(x, ω) =κ(ω)ω
p0(x, κ(ω)) or pa(x, t) = L[p0(x, ·)](t) where
Attenuation Operator
L[φ](t) =1
2π
∫R
κ(ω)
ω
∫Rφ(s)eiκ(ω)sds
e−iωtdω.
with κ(ω) =ω
√1− iaω
is the complex wave number.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 18 / 57
Inverse Source ProblemsAcoustic Time-reversal : Attenuation operators
Remark that p0(x, ω) and pa(x, ω) satisfy(κ2(ω) + ∆
)pa(x, ω) =
iκ2(ω)
ωf(x), and
(ω2 + ∆
)p0(x, ω) = iωf(x).
Therefore, pa(x, ω) =κ(ω)ω
p0(x, κ(ω)) or pa(x, t) = L[p0(x, ·)](t) where
Attenuation Operator
L[φ](t) =1
2π
∫R
κ(ω)
ω
∫Rφ(s)eiκ(ω)sds
e−iωtdω.
with κ(ω) =ω
√1− iaω
is the complex wave number.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 18 / 57
Inverse Source ProblemsAcoustic Time-reversal : Attenuation operators
Moreover, we define operator Lρ associated with κ(ω) = ω√1+iaω
by
Lρ[φ](t) :=1
2π
∫ ∞0
φ(s)
∫|ω|≤ρ
κ(ω)
ωeiκ(ω)se−iωtdω
ds,
We denote its adjoint operator by L∗ρ given by
L∗ρ[φ](t) =1
2π
∫|ω|≤ρ
κ(ω)
ωeiκ(ω)t
∫ ∞0
φ(s)e−iωsds
dω.
As
∫R
exp
−
1
2caω2s
expiω(s− t)dω =
2π√cas
exp
−
(t− s)2
2cas
ds,
for κ(ω) = ω + iaω2
2
L[φ](t) =1
2√π
(1−
ac
2
∂
∂t
)∫ ∞0
φ(s)2π√cas
exp
−
(t− s)2
2cas
ds
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 19 / 57
Inverse Source ProblemsAcoustic Time-reversal : Attenuation operators
Moreover, we define operator Lρ associated with κ(ω) = ω√1+iaω
by
Lρ[φ](t) :=1
2π
∫ ∞0
φ(s)
∫|ω|≤ρ
κ(ω)
ωeiκ(ω)se−iωtdω
ds,
We denote its adjoint operator by L∗ρ given by
L∗ρ[φ](t) =1
2π
∫|ω|≤ρ
κ(ω)
ωeiκ(ω)t
∫ ∞0
φ(s)e−iωsds
dω.
As
∫R
exp
−
1
2caω2s
expiω(s− t)dω =
2π√cas
exp
−
(t− s)2
2cas
ds,
for κ(ω) = ω + iaω2
2
L[φ](t) =1
2√π
(1−
ac
2
∂
∂t
)∫ ∞0
φ(s)2π√cas
exp
−
(t− s)2
2cas
ds
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 19 / 57
Inverse Source ProblemsAcoustic Time-reversal : Attenuation operators
Moreover, we define operator Lρ associated with κ(ω) = ω√1+iaω
by
Lρ[φ](t) :=1
2π
∫ ∞0
φ(s)
∫|ω|≤ρ
κ(ω)
ωeiκ(ω)se−iωtdω
ds,
We denote its adjoint operator by L∗ρ given by
L∗ρ[φ](t) =1
2π
∫|ω|≤ρ
κ(ω)
ωeiκ(ω)t
∫ ∞0
φ(s)e−iωsds
dω.
As
∫R
exp
−
1
2caω2s
expiω(s− t)dω =
2π√cas
exp
−
(t− s)2
2cas
ds,
for κ(ω) = ω + iaω2
2
L[φ](t) =1
2√π
(1−
ac
2
∂
∂t
)∫ ∞0
φ(s)2π√cas
exp
−
(t− s)2
2cas
ds
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 19 / 57
Inverse Source ProblemsAcoustic Time-reversal : Stationary Phase Analysis
Theorem (Stationary Phase Theorem [Hormander 03])
Let K ⊂ [0,∞) be a compact set, X an open neighbourhood of K and k ∈ N. Let
ψ ∈ C2k0 (K) and h ∈ C3k+1
0 (X) be such that :
=mh ≥ 0, =mh(t0) = 0 = h′(t0), h′′(t0) 6= 0, h′ 6= 0 in K\t0
then for ε > 0∣∣∣∣∣∫Kψ(t)eih(t)/εdt− eih(t0)/ε
(h′′(t0)/2iπε
)−1/2∑j<k
εjDj [ψ]
∣∣∣∣∣≤ Cεk
∑α≤2k
supx∈K
∣∣ψ(α)(x)∣∣
where
Dj [ψ] =∑
ν−µ=j
∑2ν≥3µ
i−j(−1)ν1
2ν ν!µ!h′′(t0)−v
(θµt0ψ
)(2ν)(t0)
with
θt0 (t) := h(t)− h(t0)−1
2h′′(t0)(t− t0)2.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 20 / 57
Inverse Source ProblemsAcoustic Time-reversal : Asymptotic approximation : a ω−1
Proposition
For κ(ω) ' ω + iaω2
2and a→ 0 following results hold :
Let φ(t) ∈ S([0,∞[), then
L[φ](t) = φ(t) +a
2
(tφ′)′
(t) + o(a).
Let φ(t) ∈ D([0,∞[), then for all ρ > 0
L∗ρ[φ](t) = Sρ[φ](t)−a
2Sρ[(tφ′)′] + o(a).
Let φ(t) ∈ D([0,∞[) and ρ > 0, then
L∗ρ [L[φ]] (t) = Sρ[φ](t) + o(a).
where S is the Schwartz space, D is the space of C∞−functions of compact support and
Sρ[φ](t) =1
2π
∫|ω|≤ρ
e−iωtφ(ω)dω
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 21 / 57
Inverse Source ProblemsAcoustic Time-reversal : Analysis of truncated functional
Consequently we have
Ia,ρ(x) =
∫ T
0
∫∂Ω
∂tGa,ρ(x, y, t)ga(y, t)dσ(y)dt
=
∫ T
0
∫∂ΩLρ [∂tG0(x, y, ·)] (t)L [g(y, ·)] (t)dσ(y)dt
=
∫ T
0
∫∂Ω
∂tG0(x, y, t)L∗ρ [L [g0(y, ·)]] (t)dσ(y)dt
=
∫ T
0
∫∂Ω
∂tG0(x, y, t)Sρ [g0(y, ·)] (t)dσ(y)dt+ o(a)
Finally remark that
δρ,x(z) =1
2π
∫|ω|≤ρ
ω=mG0(x, z)
dω → δx(z) as ρ→ +∞.
Therefore,
Ia,ρ(x) ' δρ,x(y) ∗ f(y) + o(a)
ρ→∞−−−−→
f(x) + o(a).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 22 / 57
Inverse Source ProblemsAcoustic Time-reversal : Analysis of truncated functional
Consequently we have
Ia,ρ(x) =
∫ T
0
∫∂Ω
∂tGa,ρ(x, y, t)ga(y, t)dσ(y)dt
=
∫ T
0
∫∂ΩLρ [∂tG0(x, y, ·)] (t)L [g(y, ·)] (t)dσ(y)dt
=
∫ T
0
∫∂Ω
∂tG0(x, y, t)L∗ρ [L [g0(y, ·)]] (t)dσ(y)dt
=
∫ T
0
∫∂Ω
∂tG0(x, y, t)Sρ [g0(y, ·)] (t)dσ(y)dt+ o(a)
Finally remark that
δρ,x(z) =1
2π
∫|ω|≤ρ
ω=mG0(x, z)
dω → δx(z) as ρ→ +∞.
Therefore,
Ia,ρ(x) ' δρ,x(y) ∗ f(y) + o(a)
ρ→∞−−−−→
f(x) + o(a).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 22 / 57
Inverse Source ProblemsAcoustic Time-reversal : Analysis of truncated functional
Consequently we have
Ia,ρ(x) =
∫ T
0
∫∂Ω
∂tGa,ρ(x, y, t)ga(y, t)dσ(y)dt
=
∫ T
0
∫∂ΩLρ [∂tG0(x, y, ·)] (t)L [g(y, ·)] (t)dσ(y)dt
=
∫ T
0
∫∂Ω
∂tG0(x, y, t)L∗ρ [L [g0(y, ·)]] (t)dσ(y)dt
=
∫ T
0
∫∂Ω
∂tG0(x, y, t)Sρ [g0(y, ·)] (t)dσ(y)dt+ o(a)
Finally remark that
δρ,x(z) =1
2π
∫|ω|≤ρ
ω=mG0(x, z)
dω → δx(z) as ρ→ +∞.
Therefore,
Ia,ρ(x) ' δρ,x(y) ∗ f(y) + o(a)
ρ→∞−−−−→
f(x) + o(a).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 22 / 57
Inverse Source ProblemsAcoustic Time-reversal : Truncated TR-functional Reconstructions
−1 −0.8 −0.6 −0.4 −0.2 0 0.2 0.4 0.6 0.8
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
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0.8
0
0.1
0.2
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0.5
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0.7
0.8
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1
−1 −0.8 −0.6 −0.4 −0.2 0 0.2 0.4 0.6 0.8
−1
−0.8
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0
0.2
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0.8
0
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0.7
0.8
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1
−1 −0.8 −0.6 −0.4 −0.2 0 0.2 0.4 0.6 0.8
−1
−0.8
−0.6
−0.4
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0
0.2
0.4
0.6
0.8
0
0.1
0.2
0.3
0.4
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0.7
0.8
0.9
1
Test with a = 0.0005. Left to Right : Without correction, with correction & ρ = 15, withcorrection & ρ = 20.
−1 −0.8 −0.6 −0.4 −0.2 0 0.2 0.4 0.6 0.8
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
0
0.1
0.2
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0.5
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0.7
0.8
0.9
1
−1 −0.8 −0.6 −0.4 −0.2 0 0.2 0.4 0.6 0.8
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
−1 −0.8 −0.6 −0.4 −0.2 0 0.2 0.4 0.6 0.8
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
Test with a = 0.001. Left to Right : Without correction, with correction & ρ = 15, with correction& ρ = 20.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 23 / 57
Inverse Source ProblemsAcoustic Time-reversal : Pre-processing TR-scheme
As ga(y, t) = L[g0(y, ·)](t), an alternative strategy is to
- pre-process the measured data ga(y, t) using a pseudo-inverse of L as a filter
- apply the ideal time-reversal functional I(x) to identify source location.
Using higher order asymptotic expansion :
L[φ](t) =
k∑m=0
am
m! 2m
(tmφ′
)(2m−1)(t) + o(ak)
L−1k [φ](t) =
k∑m=0
amφk,m(t) such that L−1k L[φ](t) = φ(t) + o(ak).
and φk,m verifyφk,0 = φ
φk,m = −m∑l=1
Dl[φk,m−l],and Dmφ(t) =
1
m! 2m
(tmφ′
)(2m−1)(t).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 24 / 57
Inverse Source ProblemsAcoustic Time-reversal : Pre-processing TR-scheme
As ga(y, t) = L[g0(y, ·)](t), an alternative strategy is to
- pre-process the measured data ga(y, t) using a pseudo-inverse of L as a filter
- apply the ideal time-reversal functional I(x) to identify source location.
Using higher order asymptotic expansion :
L[φ](t) =k∑
m=0
am
m! 2m
(tmφ′
)(2m−1)(t) + o(ak)
L−1k [φ](t) =
k∑m=0
amφk,m(t) such that L−1k L[φ](t) = φ(t) + o(ak).
and φk,m verifyφk,0 = φ
φk,m = −m∑l=1
Dl[φk,m−l],and Dmφ(t) =
1
m! 2m
(tmφ′
)(2m−1)(t).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 24 / 57
Inverse Source ProblemsAcoustic Time-reversal : Pre-processing TR-scheme
As ga(y, t) = L[g0(y, ·)](t), an alternative strategy is to
- pre-process the measured data ga(y, t) using a pseudo-inverse of L as a filter
- apply the ideal time-reversal functional I(x) to identify source location.
Using higher order asymptotic expansion :
L[φ](t) =k∑
m=0
am
m! 2m
(tmφ′
)(2m−1)(t) + o(ak)
L−1k [φ](t) =
k∑m=0
amφk,m(t) such that L−1k L[φ](t) = φ(t) + o(ak).
and φk,m verifyφk,0 = φ
φk,m = −m∑l=1
Dl[φk,m−l],and Dmφ(t) =
1
m! 2m
(tmφ′
)(2m−1)(t).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 24 / 57
Inverse Source ProblemsAcoustic Time-reversal : Pre-processing TR-scheme Reconstructions
−1 −0.8 −0.6 −0.4 −0.2 0 0.2 0.4 0.6 0.8
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
−1 −0.8 −0.6 −0.4 −0.2 0 0.2 0.4 0.6 0.8
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
−1 −0.8 −0.6 −0.4 −0.2 0 0.2 0.4 0.6 0.8
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
Test with a = 0.0005. Left to Right : Without correction, with correction & k = 1, with correction& k = 4.
−1 −0.8 −0.6 −0.4 −0.2 0 0.2 0.4 0.6 0.8
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
0
0.1
0.2
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0.6
0.7
0.8
0.9
1
−1 −0.8 −0.6 −0.4 −0.2 0 0.2 0.4 0.6 0.8
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
−1 −0.8 −0.6 −0.4 −0.2 0 0.2 0.4 0.6 0.8
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
Test with a = 0.001. Left to Right : Without correction, with correction & k = 1, with correction& k = 4.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 25 / 57
Inverse Source ProblemsElastic Time-reversal
ProblemFind supp
f(x)
given
g0(y, t) := u0(y, t) : (y, t) ∈ ∂Ω× [0, T ]
such that :(
∂tt − Lλ,µ)u0(x, t) = ∂tδ0(t)f(x), (x, t) ∈ Rd × R,
u0(x, t) = 0, ∂tu0(x, t) = 0, x ∈ Rd, t 0,
for T sufficiently large and
Lα,β [u] = (α+ β)∇∇ · u− β∆u.
Elastic TR-functionalConsider
I(x) :=
∫ T
0vs(x, T )ds,
where vs(x, t) is the adjoint elastic wave :∂ttvs(x, t)− Lλ,µvs(x, t) = ∂tδs(t)g0(x, T − s)δ∂Ω(x), ∀(x, t) ∈ Rd × R,vs(x, t) = 0, ∂tvs(x, t) = 0 ∀x ∈ Rd, t s.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 26 / 57
Inverse Source ProblemsElastic Time-reversal
ProblemFind supp
f(x)
given
g0(y, t) := u0(y, t) : (y, t) ∈ ∂Ω× [0, T ]
such that :(
∂tt − Lλ,µ)u0(x, t) = ∂tδ0(t)f(x), (x, t) ∈ Rd × R,
u0(x, t) = 0, ∂tu0(x, t) = 0, x ∈ Rd, t 0,
for T sufficiently large and
Lα,β [u] = (α+ β)∇∇ · u− β∆u.
Elastic TR-functionalConsider
I(x) :=
∫ T
0vs(x, T )ds,
where vs(x, t) is the adjoint elastic wave :∂ttvs(x, t)− Lλ,µvs(x, t) = ∂tδs(t)g0(x, T − s)δ∂Ω(x), ∀(x, t) ∈ Rd × R,vs(x, t) = 0, ∂tvs(x, t) = 0 ∀x ∈ Rd, t s.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 26 / 57
Inverse Source ProblemsElastic Time-reversal : Integral formulation and Green’s Tensors
Integral formulation
I(x) := <e
1
2π
∫Rd
∫Rω2
[∫∂Ω
G(x, y)G(y, z)dσ(y)
]dωf(z) dz
We have defined G(x, y) := G0(x− y) such that G0(x− y) is the fundamental solutionof the Navier equation i.e.(
Lλ,µ + ω2)G0(x) = −δ0(x)I, x ∈ Rd.
It can be expressed as
G0(x) =1
µκ2s
(κ2sG
s0(x)I +∇x∇x
(Gs0 − G
p0
)(x)), x ∈ Rd,
where
- [∆ + κ2α]Gα0 (x) = −δ(x),
- κ2p = ω2(λ+ 2µ)−1,
- κ2s = ω2µ−1
- α = p, s.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 27 / 57
Inverse Source ProblemsElastic Time-reversal : Integral formulation and Green’s Tensors
Integral formulation
I(x) := <e
1
2π
∫Rd
∫Rω2
[∫∂Ω
G(x, y)G(y, z)dσ(y)
]dωf(z) dz
We have defined G(x, y) := G0(x− y) such that G0(x− y) is the fundamental solutionof the Navier equation i.e.(
Lλ,µ + ω2)G0(x) = −δ0(x)I, x ∈ Rd.
It can be expressed as
G0(x) =1
µκ2s
(κ2sG
s0(x)I +∇x∇x
(Gs0 − G
p0
)(x)), x ∈ Rd,
where
- [∆ + κ2α]Gα0 (x) = −δ(x),
- κ2p = ω2(λ+ 2µ)−1,
- κ2s = ω2µ−1
- α = p, s.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 27 / 57
Inverse Source ProblemsElastic Time-reversal : Helmholtz-Kirchhoff identities
Let Gp and Gs be the pressure and shear modes of G such that G(x) = Gp(x) + Gs(x).Then
Proposition (Elastic H.K.-identities)
For all x, z ∈ Ω, we have
1.
∫∂Ω
[∂G(x, y)
∂νG(y, z)− G(x, y)
∂G(y, z)
∂ν
]dσ(y) = 2i=m
G(x, z)
.
2.
∫∂Ω
[∂Gα(x, y)
∂νGα(y, z)− Gα(x, y)
∂Gα(y, z)
∂ν
]dσ(y) = 2i=m
Gα(x, z)
.
3.
∫∂Ω
[∂Gs(x, y)
∂νGp(y, z)− Gs(x, y)
∂Gp(y, z)
∂ν
]dσ(y) = 0.
where α = p, s and the co-normal derivative in the outward unit normal direction n isdefined by
∂u
∂ν:= λ(∇ · u)n + µ
(∇uT + (∇uT )T
)n.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 28 / 57
Inverse Source ProblemsElastic Time-reversal : Helmholtz-Kirchhoff identities
Let Gp and Gs be the pressure and shear modes of G such that G(x) = Gp(x) + Gs(x).Then
Proposition (Elastic H.K.-identities)
For all x, z ∈ Ω, we have
1.
∫∂Ω
[∂G(x, y)
∂νG(y, z)− G(x, y)
∂G(y, z)
∂ν
]dσ(y) = 2i=m
G(x, z)
.
2.
∫∂Ω
[∂Gα(x, y)
∂νGα(y, z)− Gα(x, y)
∂Gα(y, z)
∂ν
]dσ(y) = 2i=m
Gα(x, z)
.
3.
∫∂Ω
[∂Gs(x, y)
∂νGp(y, z)− Gs(x, y)
∂Gp(y, z)
∂ν
]dσ(y) = 0.
where α = p, s and the co-normal derivative in the outward unit normal direction n isdefined by
∂u
∂ν:= λ(∇ · u)n + µ
(∇uT + (∇uT )T
)n.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 28 / 57
Inverse Source ProblemsElastic Time-reversal : Helmholtz-Kirchhoff identities II
Proposition
If n = y − x and |x− y| 1 then
∂Gα
∂ν(x, y) = iωcαGα(x, y) + o
(|x− y|1−d/2
), α = p, s.
where cs =õ and cp =
√λ+ 2µ are shear and pressure wave speeds.
LemmaLet Ω ⊂ Rd be a ball with large radius (w.r.t. wavelength). Then, for all x, z ∈ Ω sufficientlyfar from the boundary ∂Ω, we have
1. <e∫
∂ΩGα(x, y)Gα(y, z)dσ(y)
'
1
ωcα=m
Gα(x, z)
, α = p, s.
2. <e∫
∂ΩGs(x, y)Gp(y, z)dσ(y)
' 0
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 29 / 57
Inverse Source ProblemsElastic Time-reversal : Helmholtz-Kirchhoff identities II
Proposition
If n = y − x and |x− y| 1 then
∂Gα
∂ν(x, y) = iωcαGα(x, y) + o
(|x− y|1−d/2
), α = p, s.
where cs =õ and cp =
√λ+ 2µ are shear and pressure wave speeds.
LemmaLet Ω ⊂ Rd be a ball with large radius (w.r.t. wavelength). Then, for all x, z ∈ Ω sufficientlyfar from the boundary ∂Ω, we have
1. <e∫
∂ΩGα(x, y)Gα(y, z)dσ(y)
'
1
ωcα=m
Gα(x, z)
, α = p, s.
2. <e∫
∂ΩGs(x, y)Gp(y, z)dσ(y)
' 0
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 29 / 57
Inverse Source ProblemsElastic Time-reversal : Analysis of TR-functional
For x far from ∂Ω,
I(x) = <e
1
2π
∫Rd
∫Rω2
[∫∂Ω
G(x, y)G(y, z)dσ(y)
]dωf(z) dz
'
cs + cp
cscp
1
4π
∫Rd
∫Rω=m
(Gp + Gs
)(x, z)
dωf(z) dz
+cs − cpcscp
1
4π
∫Rd
∫Rω=m
(Gp − Gs
)(x, z)
dωf(z) dz
'cs + cp
2cscpf(x) +
cs − cp2cscp
∫Rd
B(x, z)f(z)dz.
The operator B(x, z) :=1
2π
∫Rω=m
(Gp − Gs
)(x, z)
dω, is not diagonal.
The reconstruction mixes the components of f when cs 6= cp.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 30 / 57
Inverse Source ProblemsElastic Time-reversal : Analysis of TR-functional
For x far from ∂Ω,
I(x) = <e
1
2π
∫Rd
∫Rω2
[∫∂Ω
G(x, y)G(y, z)dσ(y)
]dωf(z) dz
'
cs + cp
cscp
1
4π
∫Rd
∫Rω=m
(Gp + Gs
)(x, z)
dωf(z) dz
+cs − cpcscp
1
4π
∫Rd
∫Rω=m
(Gp − Gs
)(x, z)
dωf(z) dz
'cs + cp
2cscpf(x) +
cs − cp2cscp
∫Rd
B(x, z)f(z)dz.
The operator B(x, z) :=1
2π
∫Rω=m
(Gp − Gs
)(x, z)
dω, is not diagonal.
The reconstruction mixes the components of f when cs 6= cp.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 30 / 57
Inverse Source ProblemsElastic Time-reversal : Reconstructions using I
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Left to Right : Initial data, reconstruction with (λ, µ) = (1, 1), with (λ, µ) = (10, 1).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 31 / 57
Inverse Source ProblemsElastic Time-reversal : Weighted TR-functional
Let Ψ and Φ be the divergence and the curl free functions respectively such that
I = ∇×Ψ +∇Φ.
Define the weighted time-reversal functional by
I := cs∇×Ψ + cp∇Φ.
= <e
1
2π
∫Rd
∫Rω2
[∫∂Ω
(csGs(x, y) + cpGp(x, y)
)G(y, z)
]f(z)
'1
4π
∫Rd
∫R−iω
[∂G(x, y)
∂νG(y, z)− G(x, y)
∂G(y, z)
∂ν
]dωf(z) dz
'1
2π
∫Rd
∫Rω=m
G(x, z)
dωf(z) dz
Theorem
Let x ∈ Ω be sufficiently far (w.r.t. wavelength) from the boundary ∂Ω. Then, I(x) ' f(x).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 32 / 57
Inverse Source ProblemsElastic Time-reversal : Weighted TR-functional
Let Ψ and Φ be the divergence and the curl free functions respectively such that
I = ∇×Ψ +∇Φ.
Define the weighted time-reversal functional by
I := cs∇×Ψ + cp∇Φ.
= <e
1
2π
∫Rd
∫Rω2
[∫∂Ω
(csGs(x, y) + cpGp(x, y)
)G(y, z)
]f(z)
'1
4π
∫Rd
∫R−iω
[∂G(x, y)
∂νG(y, z)− G(x, y)
∂G(y, z)
∂ν
]dωf(z) dz
'1
2π
∫Rd
∫Rω=m
G(x, z)
dωf(z) dz
Theorem
Let x ∈ Ω be sufficiently far (w.r.t. wavelength) from the boundary ∂Ω. Then, I(x) ' f(x).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 32 / 57
Inverse Source ProblemsElastic Time-reversal : Weighted TR-functional
Let Ψ and Φ be the divergence and the curl free functions respectively such that
I = ∇×Ψ +∇Φ.
Define the weighted time-reversal functional by
I := cs∇×Ψ + cp∇Φ.
= <e
1
2π
∫Rd
∫Rω2
[∫∂Ω
(csGs(x, y) + cpGp(x, y)
)G(y, z)
]f(z)
'1
4π
∫Rd
∫R−iω
[∂G(x, y)
∂νG(y, z)− G(x, y)
∂G(y, z)
∂ν
]dωf(z) dz
'1
2π
∫Rd
∫Rω=m
G(x, z)
dωf(z) dz
Theorem
Let x ∈ Ω be sufficiently far (w.r.t. wavelength) from the boundary ∂Ω. Then, I(x) ' f(x).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 32 / 57
Inverse Source ProblemsElastic Time-reversal : Reconstructions using I :
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Reconstruction with (λ, µ) = (1, 1). Left to Right : Initial data, I(x), I(x).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 33 / 57
Inverse Source ProblemsElastic Time-reversal : Reconstructions using I
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Reconstruction with (λ, µ) = (10, 1). Left to Right : Initial data, I(x), I(x).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 34 / 57
Inverse Source ProblemsElastic Time-reversal : Visco-elastic media
Consider for visco-elastic moduli (ηλ, ηµ)(∂tt − Lλ,µ − ∂tLηλ,ηµ
)ua(x, t) = ∂tδ0(t)f(x), (x, t) ∈ Rd × R,
ua(x, 0) = 0, ∂tua(x, 0) = 0, x ∈ Rd, t s.
Define
vs,a,ρ(x, t) = −1
2π
∫|ω|≤ρ
∫∂Ω
iωG−a(x, y)ga(y, T − s)dσ(y)
e−iω(t−s)dω
where (Lλ,µ ± iωLηλ,ηµ + ω2
)G∓a(x, y) = −δy(x)I, x, y ∈ Rd.
Define
Ia,ρ(x) :=
∫ T
0vs,a,ρ(x, T )ds
Finally, for Ψ and Φ the divergence and curl free components of Ia,ρ, let
Ia,ρ(x) := cp∇Φ + cs∇×Ψ
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 35 / 57
Inverse Source ProblemsElastic Time-reversal : Visco-elastic media
Consider for visco-elastic moduli (ηλ, ηµ)(∂tt − Lλ,µ − ∂tLηλ,ηµ
)ua(x, t) = ∂tδ0(t)f(x), (x, t) ∈ Rd × R,
ua(x, 0) = 0, ∂tua(x, 0) = 0, x ∈ Rd, t s.
Define
vs,a,ρ(x, t) = −1
2π
∫|ω|≤ρ
∫∂Ω
iωG−a(x, y)ga(y, T − s)dσ(y)
e−iω(t−s)dω
where (Lλ,µ ± iωLηλ,ηµ + ω2
)G∓a(x, y) = −δy(x)I, x, y ∈ Rd.
Define
Ia,ρ(x) :=
∫ T
0vs,a,ρ(x, T )ds
Finally, for Ψ and Φ the divergence and curl free components of Ia,ρ, let
Ia,ρ(x) := cp∇Φ + cs∇×Ψ
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 35 / 57
Inverse Source ProblemsElastic Time-reversal : Visco-elastic media
Consider for visco-elastic moduli (ηλ, ηµ)(∂tt − Lλ,µ − ∂tLηλ,ηµ
)ua(x, t) = ∂tδ0(t)f(x), (x, t) ∈ Rd × R,
ua(x, 0) = 0, ∂tua(x, 0) = 0, x ∈ Rd, t s.
Define
vs,a,ρ(x, t) = −1
2π
∫|ω|≤ρ
∫∂Ω
iωG−a(x, y)ga(y, T − s)dσ(y)
e−iω(t−s)dω
where (Lλ,µ ± iωLηλ,ηµ + ω2
)G∓a(x, y) = −δy(x)I, x, y ∈ Rd.
Define
Ia,ρ(x) :=
∫ T
0vs,a,ρ(x, T )ds
Finally, for Ψ and Φ the divergence and curl free components of Ia,ρ, let
Ia,ρ(x) := cp∇Φ + cs∇×Ψ
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 35 / 57
Proposition
Let Ω ⊂ Rd be a ball with large radius. Then,
<e∫
∂ΩGs−a(x, y)Gpa(y, z)dσ(y)
' 0
<e∫
∂ΩGp−a(x, y)Gsa(y, z)dσ(y)
' 0
for all x, z ∈ Ω sufficiently far from the boundary ∂Ω w.r.t. wavelength
TheoremFor all x ∈ Ω sufficiently far from the boundary ∂Ω, we have
Ia,ρ(x) = Iρ(x) + o(ν2s/c
2s + ν2
p/c2p)
whereIρ(x)
ρ→∞−→ I(x) ' f(x),
νs and νp are shear and bulk viscosities and
Iρ(x) =
∫∂Ω
∫ T
0∂t[csGs(x, y, t) + cpGp(x, y, t)
]Sρg0(y, ·)
(t)dt dσ(y)
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 36 / 57
Proposition
Let Ω ⊂ Rd be a ball with large radius. Then,
<e∫
∂ΩGs−a(x, y)Gpa(y, z)dσ(y)
' 0
<e∫
∂ΩGp−a(x, y)Gsa(y, z)dσ(y)
' 0
for all x, z ∈ Ω sufficiently far from the boundary ∂Ω w.r.t. wavelength
TheoremFor all x ∈ Ω sufficiently far from the boundary ∂Ω, we have
Ia,ρ(x) = Iρ(x) + o(ν2s/c
2s + ν2
p/c2p)
whereIρ(x)
ρ→∞−→ I(x) ' f(x),
νs and νp are shear and bulk viscosities and
Iρ(x) =
∫∂Ω
∫ T
0∂t[csGs(x, y, t) + cpGp(x, y, t)
]Sρg0(y, ·)
(t)dt dσ(y)
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 36 / 57
Inverse Source ProblemsElastic Time-reversal : Visco-elastic Weighted TR Reconstructions
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Reconstruction with (λ, µ) = (1, 1) and a = 0.0002. Left to Right : Initial data, without correction
using I(x), correction using Ia,ρ with ρ = 15, with ρ = 20.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 37 / 57
Noise Source Localization
Noise Source Localization
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 38 / 57
Noise Source LocalizationStatement of the Problem
Let p0 satisfy the wave equation1
c2(x)
∂2
∂t2p0(x, t)−∆p0(x, t) = n(x, t), (x, t) ∈ Rd × R
p0(x, t) = 0, and∂
∂tp0(x, t) = 0, x ∈ Rd, t 0, d = 2, 3.
n is compactly supported in a bounded smooth domain Ω.
n is a stationary Gaussian process with mean zero and covariance
〈n(x, t)n(y, s)〉 = F (t− s)K(x)δ(x− y).
ProblemFind suppn given
p0(y, t) : (y, t) ∈ ∂Ω× [0, T ]
for sufficiently large T .
- 〈·〉 : Statistical average,
- c : Positive, smooth and boundedfunction,
- F : Time covariance function,
- K : Spatial support of n.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 39 / 57
Noise Source LocalizationStatement of the Problem
Let p0 satisfy the wave equation1
c2(x)
∂2
∂t2p0(x, t)−∆p0(x, t) = n(x, t), (x, t) ∈ Rd × R
p0(x, t) = 0, and∂
∂tp0(x, t) = 0, x ∈ Rd, t 0, d = 2, 3.
n is compactly supported in a bounded smooth domain Ω.
n is a stationary Gaussian process with mean zero and covariance
〈n(x, t)n(y, s)〉 = F (t− s)K(x)δ(x− y).
ProblemFind suppn given
p0(y, t) : (y, t) ∈ ∂Ω× [0, T ]
for sufficiently large T .
- 〈·〉 : Statistical average,
- c : Positive, smooth and boundedfunction,
- F : Time covariance function,
- K : Spatial support of n.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 39 / 57
Noise Source LocalizationStatement of the Problem
Let p0 satisfy the wave equation1
c2(x)
∂2
∂t2p0(x, t)−∆p0(x, t) = n(x, t), (x, t) ∈ Rd × R
p0(x, t) = 0, and∂
∂tp0(x, t) = 0, x ∈ Rd, t 0, d = 2, 3.
n is compactly supported in a bounded smooth domain Ω.
n is a stationary Gaussian process with mean zero and covariance
〈n(x, t)n(y, s)〉 = F (t− s)K(x)δ(x− y).
ProblemFind suppn given
p0(y, t) : (y, t) ∈ ∂Ω× [0, T ]
for sufficiently large T .
- 〈·〉 : Statistical average,
- c : Positive, smooth and boundedfunction,
- F : Time covariance function,
- K : Spatial support of n.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 39 / 57
Noise Source LocalizationCross-correlation based functional
Imaging functional
I(zS) :=
∫R
∫∫∂Ω×∂Ω
G0(x, zS , ω)G0(y, zS , ω)C0(x, y, ω)dσ(x)dσ(y)dω.
(ω2
c2(x)+ ∆
)G0(x, y, ω) = −δ(x− y), x, y ∈ Rd.
The statistical cross-correlation C0 is defined by
C0(x, y, τ) = 〈p0(x, t)p0(y, t+τ)〉 =1
2π
∫R
[ ∫ΩG0(x, z, ω)G0(y, z, ω)K(z)dz
]F (ω)e−iωτ .
TheoremFunctional I gives K up to a smoothing operator, that is
I(zS) '∫
ΩQ(zS , z)K(z)dz, where
Q(zS , z) =
∫R
F (ω)
ω2=m
G0(zS , z, ω)
2dω.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 40 / 57
Noise Source LocalizationCross-correlation based functional
Imaging functional
I(zS) :=
∫R
∫∫∂Ω×∂Ω
G0(x, zS , ω)G0(y, zS , ω)C0(x, y, ω)dσ(x)dσ(y)dω.
(ω2
c2(x)+ ∆
)G0(x, y, ω) = −δ(x− y), x, y ∈ Rd.
The statistical cross-correlation C0 is defined by
C0(x, y, τ) = 〈p0(x, t)p0(y, t+τ)〉 =1
2π
∫R
[ ∫ΩG0(x, z, ω)G0(y, z, ω)K(z)dz
]F (ω)e−iωτ .
TheoremFunctional I gives K up to a smoothing operator, that is
I(zS) '∫
ΩQ(zS , z)K(z)dz, where
Q(zS , z) =
∫R
F (ω)
ω2=m
G0(zS , z, ω)
2dω.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 40 / 57
Noise Source LocalizationCross-correlation based functional
Imaging functional
I(zS) :=
∫R
∫∫∂Ω×∂Ω
G0(x, zS , ω)G0(y, zS , ω)C0(x, y, ω)dσ(x)dσ(y)dω.
(ω2
c2(x)+ ∆
)G0(x, y, ω) = −δ(x− y), x, y ∈ Rd.
The statistical cross-correlation C0 is defined by
C0(x, y, τ) = 〈p0(x, t)p0(y, t+τ)〉 =1
2π
∫R
[ ∫ΩG0(x, z, ω)G0(y, z, ω)K(z)dz
]F (ω)e−iωτ .
TheoremFunctional I gives K up to a smoothing operator, that is
I(zS) '∫
ΩQ(zS , z)K(z)dz, where
Q(zS , z) =
∫R
F (ω)
ω2=m
G0(zS , z, ω)
2dω.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 40 / 57
Noise Source LocalizationWeighted imaging functional
Consider the power spectral density F(ω) =
∫∂Ω
C0(x, x, ω)dσ(x).
F(ω) =1
∆ω
∫ ω+∆ω/2
ω−∆ω/2F(ω′)dω′ ' F (ω)
∫Ω
1
ω=m
G0(z, z, ω)
K(z)dz
Moving frequency window ∆ω should be large than 1/T and smaller than noisebandwidth.
Imaging functional
IW (zS) :=
∫R
W (ω)
F(ω)
∫∫∂Ω×∂Ω
G0(x, zS , ω)G0(y, zS , ω)C0(x, y, ω)dσ(x)dσ(y)dω.
Theorem
IW (zS) '∫
ΩQW (zS , z)
K(z)
K0dz, with K0 =
1
4π
∫ΩK(z)dz and
QW (zS , z) =W (ω)
ω2=m
G0(zS , z, ω)
2dω =
116W (ω)
ω2 J20 (ω|z|)dω, d = 2
116π2
W (ω)
ω2 sinc2(ω|z|)dω, d = 3.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 41 / 57
Noise Source LocalizationWeighted imaging functional
Consider the power spectral density F(ω) =
∫∂Ω
C0(x, x, ω)dσ(x).
F(ω) =1
∆ω
∫ ω+∆ω/2
ω−∆ω/2F(ω′)dω′ ' F (ω)
∫Ω
1
ω=m
G0(z, z, ω)
K(z)dz
Moving frequency window ∆ω should be large than 1/T and smaller than noisebandwidth.
Imaging functional
IW (zS) :=
∫R
W (ω)
F(ω)
∫∫∂Ω×∂Ω
G0(x, zS , ω)G0(y, zS , ω)C0(x, y, ω)dσ(x)dσ(y)dω.
Theorem
IW (zS) '∫
ΩQW (zS , z)
K(z)
K0dz, with K0 =
1
4π
∫ΩK(z)dz and
QW (zS , z) =W (ω)
ω2=m
G0(zS , z, ω)
2dω =
116W (ω)
ω2 J20 (ω|z|)dω, d = 2
116π2
W (ω)
ω2 sinc2(ω|z|)dω, d = 3.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 41 / 57
Noise Source LocalizationWeighted imaging functional
Consider the power spectral density F(ω) =
∫∂Ω
C0(x, x, ω)dσ(x).
F(ω) =1
∆ω
∫ ω+∆ω/2
ω−∆ω/2F(ω′)dω′ ' F (ω)
∫Ω
1
ω=m
G0(z, z, ω)
K(z)dz
Moving frequency window ∆ω should be large than 1/T and smaller than noisebandwidth.
Imaging functional
IW (zS) :=
∫R
W (ω)
F(ω)
∫∫∂Ω×∂Ω
G0(x, zS , ω)G0(y, zS , ω)C0(x, y, ω)dσ(x)dσ(y)dω.
Theorem
IW (zS) '∫
ΩQW (zS , z)
K(z)
K0dz, with K0 =
1
4π
∫ΩK(z)dz and
QW (zS , z) =W (ω)
ω2=m
G0(zS , z, ω)
2dω =
116W (ω)
ω2 J20 (ω|z|)dω, d = 2
116π2
W (ω)
ω2 sinc2(ω|z|)dω, d = 3.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 41 / 57
Noise Source LocalizationWeighted imaging functional
Consider the power spectral density F(ω) =
∫∂Ω
C0(x, x, ω)dσ(x).
F(ω) =1
∆ω
∫ ω+∆ω/2
ω−∆ω/2F(ω′)dω′ ' F (ω)
∫Ω
1
ω=m
G0(z, z, ω)
K(z)dz
Moving frequency window ∆ω should be large than 1/T and smaller than noisebandwidth.
Imaging functional
IW (zS) :=
∫R
W (ω)
F(ω)
∫∫∂Ω×∂Ω
G0(x, zS , ω)G0(y, zS , ω)C0(x, y, ω)dσ(x)dσ(y)dω.
Theorem
IW (zS) '∫
ΩQW (zS , z)
K(z)
K0dz, with K0 =
1
4π
∫ΩK(z)dz and
QW (zS , z) =W (ω)
ω2=m
G0(zS , z, ω)
2dω =
116W (ω)
ω2 J20 (ω|z|)dω, d = 2
116π2
W (ω)
ω2 sinc2(ω|z|)dω, d = 3.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 41 / 57
Noise Source LocalizationWeighted imaging functional
Consider the power spectral density F(ω) =
∫∂Ω
C0(x, x, ω)dσ(x).
F(ω) =1
∆ω
∫ ω+∆ω/2
ω−∆ω/2F(ω′)dω′ ' F (ω)
∫Ω
1
ω=m
G0(z, z, ω)
K(z)dz
Moving frequency window ∆ω should be large than 1/T and smaller than noisebandwidth.
Imaging functional
IW (zS) :=
∫R
W (ω)
F(ω)
∫∫∂Ω×∂Ω
G0(x, zS , ω)G0(y, zS , ω)C0(x, y, ω)dσ(x)dσ(y)dω.
Theorem
IW (zS) '∫
ΩQW (zS , z)
K(z)
K0dz, with K0 =
1
4π
∫ΩK(z)dz and
QW (zS , z) =W (ω)
ω2=m
G0(zS , z, ω)
2dω =
116W (ω)
ω2 J20 (ω|z|)dω, d = 2
116π2
W (ω)
ω2 sinc2(ω|z|)dω, d = 3.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 41 / 57
Noise Source LocalizationWeighted imaging functional : Remarks
A potential candidate for W should be
W (ω) =
|ω|31|ω|<ωmax
, d = 2
ω21|ω|<ωmax, d = 3.
based on the closure formulae [Abramowitz 65]∫R+
ωJ20 (ω|z|)dω =
1
|z|δ(z),
and ∫R+
ω2sinc2(ω|z|)dω =1
|z|2δ(z),
where 1 denotes the characteristic function.
IW can seen as an application of I on filtered data p0(x, t) where
p0(x, ω) :=
√W (ω)
F(ω)p0(x, ω).
where (−ωmax, ωmax) is the estimated support of F(ω)
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 42 / 57
Noise Source LocalizationWeighted imaging functional : Remarks
A potential candidate for W should be
W (ω) =
|ω|31|ω|<ωmax
, d = 2
ω21|ω|<ωmax, d = 3.
based on the closure formulae [Abramowitz 65]∫R+
ωJ20 (ω|z|)dω =
1
|z|δ(z),
and ∫R+
ω2sinc2(ω|z|)dω =1
|z|2δ(z),
where 1 denotes the characteristic function.
IW can seen as an application of I on filtered data p0(x, t) where
p0(x, ω) :=
√W (ω)
F(ω)p0(x, ω).
where (−ωmax, ωmax) is the estimated support of F(ω)
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 42 / 57
Noise Source LocalizationAnalogy with time-reversal
I(zS) =
∫R
∫∂Ω
∫∂Ω
G0(x, zS , ω)G0(y, zS , ω)C0(x, y, ω)dσ(x)dσ(y)dω
=
∫R
∫∂Ω
∫∂Ω
G0(x, zS , ω)G0(y, zS , ω)p0(x, ω)p0(y, ω)dσ(x)dσ(y)dω
=
∫R
∣∣∣ ∫∂Ω
G0(x, zS , ω)p0(x, ω)dσ(x)∣∣∣2dω
= 2π
∫ T
0v(zS , t)2dt,
v is the adjoint wave expressed in the form
v(x, t) =
∫ T
0vs(x, t)ds, with
∂2
∂t2vs(x, t)−∆vs(x, t) = δ(t− s)p0(x, T − s)δ∂Ω(x), ∀(x, t) ∈ Rd × (0, T ),
vs(x, t) = 0,∂
∂tvs(x, t) = 0 ∀x ∈ Rd, t < s.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 43 / 57
Noise Source LocalizationAnalogy with time-reversal
I(zS) =
∫R
∫∂Ω
∫∂Ω
G0(x, zS , ω)G0(y, zS , ω)C0(x, y, ω)dσ(x)dσ(y)dω
=
∫R
∫∂Ω
∫∂Ω
G0(x, zS , ω)G0(y, zS , ω)p0(x, ω)p0(y, ω)dσ(x)dσ(y)dω
=
∫R
∣∣∣ ∫∂Ω
G0(x, zS , ω)p0(x, ω)dσ(x)∣∣∣2dω
= 2π
∫ T
0v(zS , t)2dt,
v is the adjoint wave expressed in the form
v(x, t) =
∫ T
0vs(x, t)ds, with
∂2
∂t2vs(x, t)−∆vs(x, t) = δ(t− s)p0(x, T − s)δ∂Ω(x), ∀(x, t) ∈ Rd × (0, T ),
vs(x, t) = 0,∂
∂tvs(x, t) = 0 ∀x ∈ Rd, t < s.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 43 / 57
Noise Source LocalizationReconstructions
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Top : point sources. Bottom : extended sources.Left to Right : K(x) ; I ; IW withW (ω) = |ω|31|ω|<ωmax .
T = 8, ωmax = 1000, Nx = 28, and Nt = 211.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 44 / 57
Noise Source LocalizationEstimation of power spectral density
−500 −400 −300 −200 −100 0 100 200 300 400 5000
0.5
1
1.5
2
2.5
3
3.5
ω
F(ω) estimated F(ω) estimated and denoised F(ω) exact
F (ω) = exp
(−π ω2
ω2max
)with ωmax = 1000.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 45 / 57
Noise Source LocalizationEstimation of power spectral density
−500 −400 −300 −200 −100 0 100 200 300 400 5000
0.5
1
1.5
2
2.5
3
ω
F(ω) estimated F(ω) estimated and denoised F(ω) exact
F (ω) = 1|ω|≤100 exp
(−π ω2
ω2max
).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 45 / 57
Noise Source LocalizationSpatially correlated sources
Let n be a stationary Gaussian process with mean zero and covariance function
〈n(x, t)n(y, s)〉 = F (t− s)Γ(x, y)
where Γ characterizes spatial support and covariance of the sources.
C0(x, y, τ) =1
2π
∫R
[ ∫∫Ω×Ω
G0(x, z, ω)G0(y, z′, ω)Γ(z, z′)dz dz′]F (ω)e−iωτdω.
J(zS , zS′) :=
∫R
∫∫∂Ω×∂Ω
G0(x, zS , ω)G0(y, zS′, ω)C0(x, y, ω)dσ(x)dσ(y)dω.
Proposition
J(zS , zS′) :=
∫∫Ω×Ω
∫R
F (ω)
ω2=m
G(z, zS , ω)
=m
G(z′, zS
′, ω)dω︸ ︷︷ ︸
Ψ(zS ,zS′,z,z′)
Γ(z, z′) dz dz′.
In 3D homogeneous media, Ψ(zS , zS′, z, z′) = ψ(zS − z, zS′ − z′) with
ψ(z, z′) =1
16π2
∫RF (ω)sinc(ω|z|)sinc(ω|z′|)dω.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 46 / 57
Noise Source LocalizationSpatially correlated sources
Let n be a stationary Gaussian process with mean zero and covariance function
〈n(x, t)n(y, s)〉 = F (t− s)Γ(x, y)
where Γ characterizes spatial support and covariance of the sources.
C0(x, y, τ) =1
2π
∫R
[ ∫∫Ω×Ω
G0(x, z, ω)G0(y, z′, ω)Γ(z, z′)dz dz′]F (ω)e−iωτdω.
J(zS , zS′) :=
∫R
∫∫∂Ω×∂Ω
G0(x, zS , ω)G0(y, zS′, ω)C0(x, y, ω)dσ(x)dσ(y)dω.
Proposition
J(zS , zS′) :=
∫∫Ω×Ω
∫R
F (ω)
ω2=m
G(z, zS , ω)
=m
G(z′, zS
′, ω)dω︸ ︷︷ ︸
Ψ(zS ,zS′,z,z′)
Γ(z, z′) dz dz′.
In 3D homogeneous media, Ψ(zS , zS′, z, z′) = ψ(zS − z, zS′ − z′) with
ψ(z, z′) =1
16π2
∫RF (ω)sinc(ω|z|)sinc(ω|z′|)dω.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 46 / 57
Noise Source LocalizationSpatially correlated sources
Let n be a stationary Gaussian process with mean zero and covariance function
〈n(x, t)n(y, s)〉 = F (t− s)Γ(x, y)
where Γ characterizes spatial support and covariance of the sources.
C0(x, y, τ) =1
2π
∫R
[ ∫∫Ω×Ω
G0(x, z, ω)G0(y, z′, ω)Γ(z, z′)dz dz′]F (ω)e−iωτdω.
J(zS , zS′) :=
∫R
∫∫∂Ω×∂Ω
G0(x, zS , ω)G0(y, zS′, ω)C0(x, y, ω)dσ(x)dσ(y)dω.
Proposition
J(zS , zS′) :=
∫∫Ω×Ω
∫R
F (ω)
ω2=m
G(z, zS , ω)
=m
G(z′, zS
′, ω)dω︸ ︷︷ ︸
Ψ(zS ,zS′,z,z′)
Γ(z, z′) dz dz′.
In 3D homogeneous media, Ψ(zS , zS′, z, z′) = ψ(zS − z, zS′ − z′) with
ψ(z, z′) =1
16π2
∫RF (ω)sinc(ω|z|)sinc(ω|z′|)dω.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 46 / 57
Noise Source LocalizationSpatially correlated sources
Let n be a stationary Gaussian process with mean zero and covariance function
〈n(x, t)n(y, s)〉 = F (t− s)Γ(x, y)
where Γ characterizes spatial support and covariance of the sources.
C0(x, y, τ) =1
2π
∫R
[ ∫∫Ω×Ω
G0(x, z, ω)G0(y, z′, ω)Γ(z, z′)dz dz′]F (ω)e−iωτdω.
J(zS , zS′) :=
∫R
∫∫∂Ω×∂Ω
G0(x, zS , ω)G0(y, zS′, ω)C0(x, y, ω)dσ(x)dσ(y)dω.
Proposition
J(zS , zS′) :=
∫∫Ω×Ω
∫R
F (ω)
ω2=m
G(z, zS , ω)
=m
G(z′, zS
′, ω)dω︸ ︷︷ ︸
Ψ(zS ,zS′,z,z′)
Γ(z, z′) dz dz′.
In 3D homogeneous media, Ψ(zS , zS′, z, z′) = ψ(zS − z, zS′ − z′) with
ψ(z, z′) =1
16π2
∫RF (ω)sinc(ω|z|)sinc(ω|z′|)dω.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 46 / 57
Noise Source LocalizationSpatially correlated sources II
Correlated point sources : Γ(z, z′) =
Ns∑i,j=1
ρijδ(z − zi)δ(z − zj)
- Find zi from I(zS) 'Ns∑i,j=1
ρij
∫R
F (ω)
ω2=m
G(z, zS , ω)
2dω.
- Estimate ρij from
J(zi, zj) = ρij
∫R=m
G(zi, zi, ω)
=m
G(zj , zj , ω)
dω ' ρij
1
16π
∫RF (ω)dω.
ρ =
1 1/
√2 1/
√2 0
1/√
2 1 0 0
1/√
2 0 1 00 0 0 1
ρ =
1.000 0.733 0.701 0.0610.733 1.000 0.049 0.0610.701 0.049 1.000 0.0300.061 0.061 0.030 1.000
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 47 / 57
Noise Source LocalizationSpatially correlated sources II
Correlated point sources : Γ(z, z′) =
Ns∑i,j=1
ρijδ(z − zi)δ(z − zj)
- Find zi from I(zS) 'Ns∑i,j=1
ρij
∫R
F (ω)
ω2=m
G(z, zS , ω)
2dω.
- Estimate ρij from
J(zi, zj) = ρij
∫R=m
G(zi, zi, ω)
=m
G(zj , zj , ω)
dω ' ρij
1
16π
∫RF (ω)dω.
ρ =
1 1/
√2 1/
√2 0
1/√
2 1 0 0
1/√
2 0 1 00 0 0 1
ρ =
1.000 0.733 0.701 0.0610.733 1.000 0.049 0.0610.701 0.049 1.000 0.0300.061 0.061 0.030 1.000
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 47 / 57
Noise Source LocalizationCorrelated point sources : Reconstruction
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0.6
0.8
Top : K(z) (left), IW with W (ω) = |ω|31|ω|<ωmax (middle), and z → JW (z1, z) (right).Bottom : z → JW (z2, z) (left),z → JW (z3, z) (middle), and z → JW (z4, z) (right).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 48 / 57
Noise Source LocalizationExtended correlated sources : Reconstruction
z1
z2
z3
z4
−1 −0.5 0 0.5
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
z1
z2
z3
z4
−1 −0.5 0 0.5
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
z2
z3
z4
z1
−1 −0.5 0 0.5
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
z2
z3
z4
z1
−1 −0.5 0 0.5
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
z2
z3
z4
z1
−1 −0.5 0 0.5
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
z2
z3
z4
z1
−1 −0.5 0 0.5
−1
−0.8
−0.6
−0.4
−0.2
0
0.2
0.4
0.6
0.8
Top : K(z) (left), IW with W (ω) = |ω|31|ω|<ωmax (middle), and z → JW (z1, z) (right).Bottom : z → JW (z2, z) (left),z → JW (z3, z) (middle), and z → JW (z4, z) (right).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 49 / 57
Time Reversal Cavity
Time Reversal Cavity
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 50 / 57
Time Reversal CavitySpherical Dielectric Inclusion
D = z + δB with permittivity ε and permeability µ0, radiated by an electric dipole at y with
direction e.
Let Gee (resp. Gme) be the electric-electric (resp. magnetic-electric) Green’s functionfor the Maxwell’s equations in R3 i.e. for all (x, t) ∈ R3 × R
∇×Gee(x, t) = −µ0∂Gme
∂t(x, t),
∇×Gme(x, t) = ε0∂Gee
∂t(x, t) + Iδ0 (x) δ0 (t) ,
Let Ey(x, t) := −Gee(x− y, t) · e,
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 51 / 57
Time Reversal CavitySpherical Dielectric Inclusion
D = z + δB with permittivity ε and permeability µ0, radiated by an electric dipole at y with
direction e.
Let Gee (resp. Gme) be the electric-electric (resp. magnetic-electric) Green’s functionfor the Maxwell’s equations in R3 i.e. for all (x, t) ∈ R3 × R
∇×Gee(x, t) = −µ0∂Gme
∂t(x, t),
∇×Gme(x, t) = ε0∂Gee
∂t(x, t) + Iδ0 (x) δ0 (t) ,
Let Ey(x, t) := −Gee(x− y, t) · e,
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 51 / 57
Time Reversal CavitySpherical Dielectric Inclusion
D = z + δB with permittivity ε and permeability µ0, radiated by an electric dipole at y with
direction e.
Let Gee (resp. Gme) be the electric-electric (resp. magnetic-electric) Green’s functionfor the Maxwell’s equations in R3 i.e. for all (x, t) ∈ R3 × R
∇×Gee(x, t) = −µ0∂Gme
∂t(x, t),
∇×Gme(x, t) = ε0∂Gee
∂t(x, t) + Iδ0 (x) δ0 (t) ,
Let Ey(x, t) := −Gee(x− y, t) · e,
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 51 / 57
Time Reversal CavityElectromagnetic Scattering
Consider the following scattering problem
∇×(
1
ε0∇×E
)+ µ0
∂2E
∂t2= −µ0δye
∂δ0
∂t, (R3 \D)× R,
∇×(
1
ε∇×E
)+ µ0
∂2E
∂t2= 0, D × R,
1
ε0(∇×E)+ × ν =
1
ε(∇×E)− × ν, ∂D × R,
µ0E+ · ν = µ0E− · ν, ∂D × R,
E(x, t) = 0 =∂E
∂t(x, t), t 0,
Lemma (Asymptotic expansion of the scattered field
Let x, y be sufficiently far from z, and ωc = O(δ−α), then
Sωc [E−Ey ](x, t) = δ3
∫R
∂
∂tSωc [Gee](x− z, t− τ) ·M(ε, B)Sωc [Ey ](z, τ − t0) dτ +O(δ4−3α)
M =3(ε−ε0)(ε+2ε0)
|B|I is the polarization tensor associated with D [Ammari 07].
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 52 / 57
Time Reversal CavityElectromagnetic Scattering
Consider the following scattering problem
∇×(
1
ε0∇×E
)+ µ0
∂2E
∂t2= −µ0δye
∂δ0
∂t, (R3 \D)× R,
∇×(
1
ε∇×E
)+ µ0
∂2E
∂t2= 0, D × R,
1
ε0(∇×E)+ × ν =
1
ε(∇×E)− × ν, ∂D × R,
µ0E+ · ν = µ0E− · ν, ∂D × R,
E(x, t) = 0 =∂E
∂t(x, t), t 0,
Lemma (Asymptotic expansion of the scattered field
Let x, y be sufficiently far from z, and ωc = O(δ−α), then
Sωc [E−Ey ](x, t) = δ3
∫R
∂
∂tSωc [Gee](x− z, t− τ) ·M(ε, B)Sωc [Ey ](z, τ − t0) dτ +O(δ4−3α)
M =3(ε−ε0)(ε+2ε0)
|B|I is the polarization tensor associated with D [Ammari 07].
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 52 / 57
Time Reversal CavityElectromagnetic Scattering
ProblemSuppose we are given the tangential component of E on a sphere S for t ∈ [0, t0]. Let Etr bethe field obtained by re-emitting time reversed data. Find Etr and the location z of D.
Theorem
Etr(x, t) ' −δ3
∫RqT (z, τ) ·
∂
∂t
[Sωc [Gee(x− z, t0 − τ − t)−Gee(x− z, t− t0 + τ)]
]dτ,
Etr(x, ω) ∝ δ3qT (z, τ) ·(ω2
c2I +∇∇
)sinc
(ωc|x− z|
),
where
q(z, τ) = ε0M(ε, B) ·∂
∂tSωc [Ey ](z, τ).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 53 / 57
Time Reversal CavityElectromagnetic Scattering
ProblemSuppose we are given the tangential component of E on a sphere S for t ∈ [0, t0]. Let Etr bethe field obtained by re-emitting time reversed data. Find Etr and the location z of D.
Theorem
Etr(x, t) ' −δ3
∫RqT (z, τ) ·
∂
∂t
[Sωc [Gee(x− z, t0 − τ − t)−Gee(x− z, t− t0 + τ)]
]dτ,
Etr(x, ω) ∝ δ3qT (z, τ) ·(ω2
c2I +∇∇
)sinc
(ωc|x− z|
),
where
q(z, τ) = ε0M(ε, B) ·∂
∂tSωc [Ey ](z, τ).
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 53 / 57
Conclusion, Perspectives and Open Questions
Conclusion, Perspectives andOpen Questions
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 54 / 57
Conclusion, Perspectives and Open Questions
- Presented time reversal techniques for wave imaging.
- Proposed and analysed, adjoint, pre-processing and weighted TR techniques tocompensate for the attenuation effects.
- Derived Helmholtz-Kirchhoff identities for elastic, visco-elastic and attenuatingacoustic media.
- Variable attenuation correction.
- Time reversal in composite and inhomogeneous media.
- Limited view problem and virtual sources in scattering media.
- Time reversal with a few transducers : lower bound on the number oftransducers for stable reconstructions.
- Coherent interferometric techniques for clutter media and imaging in thepresence of measurements noise (elasticity case).
- Topological derivative based imaging techniques and their analogy with TR.
- Universe of applications.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 55 / 57
Conclusion, Perspectives and Open Questions
- Presented time reversal techniques for wave imaging.
- Proposed and analysed, adjoint, pre-processing and weighted TR techniques tocompensate for the attenuation effects.
- Derived Helmholtz-Kirchhoff identities for elastic, visco-elastic and attenuatingacoustic media.
- Variable attenuation correction.
- Time reversal in composite and inhomogeneous media.
- Limited view problem and virtual sources in scattering media.
- Time reversal with a few transducers : lower bound on the number oftransducers for stable reconstructions.
- Coherent interferometric techniques for clutter media and imaging in thepresence of measurements noise (elasticity case).
- Topological derivative based imaging techniques and their analogy with TR.
- Universe of applications.
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 55 / 57
Related Publications 1
H. Ammari, E. Bretin, J. Garnier, A. Wahab, Noise source localization inan attenuating medium, SIAM Journal on Applied Mathematics,72(1) :(2012), pp. 317-336.
H. Ammari, E. Bretin, J. Garnier, A. Wahab, Time reversal algorithms inviscoelastic media, Submitted to European Journal of Applied Mathematics,(33 pages).
H. Ammari, E. Bretin, J. Garnier, A. Wahab, Time reversal in attenuatingacoustic media, Contemporary Mathematics, vol. 548, pp. 151-163 AmericanMathematical Society 2011.
S. Gdoura, D. Lesselier, A. Wahab, Time reversal and scattering by asmall 3-D dielectric inclusion in lossy media, in preparation
1. Preprints are available at www.cmap.polytechnique.fr/∼wahab
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 56 / 57
Thank You !
Questions ?
A. Wahab (CMAP, LPMA) Time Reversal in Wave Imaging NUST, April 18, 2012 57 / 57