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[email protected]. edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC Berkeley)

[email protected] Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

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Page 1: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Wave-equation migration velocity analysis

beyond the Born approximation

Paul Sava* Stanford University

Sergey Fomel UT Austin (UC Berkeley)

Page 2: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Imaging=MVA+Migration

• Migration• wavefield based

• Migration velocity analysis (MVA)• traveltime based

• Compatible migration and MVA methods

Page 3: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Imaging: the “big picture”

• Kirchhoff migration

• traveltime tomography

wavefronts

• wave-equation migration

• wave-equation MVA (WEMVA)

wavefields

Page 4: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Agenda

Theoretical background

WEMVA methodology

Scattering

Imaging

Image perturbations

Wavefield extrapolation

Born linearization

Alternative linearizations

Page 5: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Wavefields or traveltimes?

Page 6: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Wavefields or traveltimes?

Page 7: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Scattered wavefield

Medium perturbation

Wavefield perturbation

Page 8: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Agenda

Theoretical background

WEMVA methodology

Scattering

Imaging

Image perturbations

Wavefield extrapolation

Born linearization

Alternative linearizations

Page 9: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Imaging: Correct velocity

Background velocity

Migrated image

Reflectivity model

What the data tell us...What migration does...

location

depth

location

depth

depthdepth

depth

Page 10: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Imaging: Incorrect velocity

Perturbed velocity

Migrated image

Reflectivity model

What the data tell us...What migration does...

location

depth

location

depth

depthdepth

depth

Page 11: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Wave-equation MVA: Objective

Velocity perturbation

Image perturbation

slownessperturbation(unknown)

WEMVAoperator

imageperturbation

(known)

sLΔRminΔs

location

depth

location

depth

Page 12: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

– migrated images

– moveout and focusing– use amplitudes

– parabolic wave equation– multipathing

– slow

– picked traveltimes

– moveout– ignore amplitudes

– eikonal equation

– fast

Comparison of MVA methods

• Wave-equation MVA • Traveltime tomography

Page 13: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Agenda

Theoretical background

WEMVA methodology

Scattering

Imaging

Image perturbations

Wavefield extrapolation

Born linearization

Alternative linearizations

Page 14: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

What is the image perturbation?

Focusing Flatness Residual process:• moveout• migration• focusing

slownessperturbation(unknown)

WEMVAoperator

imageperturbation

(known)

sLΔRminΔs

location

depth

angle

Page 15: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Agenda

Theoretical background

WEMVA methodology

Scattering

Imaging

Image perturbations

Wavefield extrapolation

Born linearization

Alternative linearizations

Page 16: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Double Square-Root Equation

Wikdz

dWz

Δsds

dkkk

0

0

ss

zzz

Fourier Finite DifferenceGeneralized Screen Propagator

Δzikz

Δzzze

W

W

Wavefield extrapolation

βΔsΔzz

0

Δzz

eW

W

βΔsΔzikΔzik0zz

Page 17: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

“Wave-equation” migration

z

Δzz0s

Δzz0W

Page 18: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Slowness perturbation

0s Δss0

Δzz0W

z

Δzz

βΔsΔzz0 eW

Page 19: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

1eWΔW βΔs0

slownessperturbation

backgroundwavefield

wavefieldperturbation

ΔW

Δs

Wavefield perturbation

z

Δzz0s Δss0

Page 20: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Agenda

Theoretical background

WEMVA methodology

Scattering

Imaging

Image perturbations

Wavefield extrapolation

Born linearization

Alternative linearizations

Page 21: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Born approximation

iei 1

ie

Small perturbations!

Born linearization

Non-linear WEMVA

1eWΔW βΔs0

βΔsWΔW 0slowness

perturbation(unknown)

WEMVAoperator

imageperturbation

(known)

sLΔRminΔs

Unit circle

Page 22: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

sLΔRminΔs

Does it work?What if the perturbations are not small?

Location [km]

Depth [km

]

Page 23: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Synthetic example

Page 24: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Born approximation

1% 10%

Page 25: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Agenda

Theoretical background

WEMVA methodology

Scattering

Imaging

Image perturbations

Wavefield extrapolation

Born linearization

Alternative linearizations

Page 26: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Wavefield continuation

Wikdz

dWz βΔs

0

eW

W

Bilinear

Implicit

βΔs2

βΔs2

W

W

0

βΔs1

1

W

W

0

Explicit βΔs1W

W

0

(Born approximation)

Page 27: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Exponential approximations

ξβΔs1

βΔsξ11eβΔs

0,1ξ

0.5ξ

Wikdz

dWz βΔs

0

eW

W

Unit circle

Page 28: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

1eWΔW βΔs0

A family of linearizations

ξβΔs1

βΔsξ11eβΔs

0,1ξ

βΔsξΔWWΔW 0Linear WEMVA

slownessperturbation(unknown)

WEMVAoperator

imageperturbation

(known)

sLΔRminΔs

Page 29: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Improved linearizations

1% 10%40%

Page 30: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Agenda

Theoretical background

WEMVA methodology

Scattering

Imaging

Image perturbations

Wavefield extrapolation

Born linearization

Alternative linearizations

Page 31: Paul@sep.stanford.edu Wave-equation migration velocity analysis beyond the Born approximation Paul Sava* Stanford University Sergey Fomel UT Austin (UC

[email protected]

Summary

• Wave-equation MVA• wavefield-continuation• improved focusing • image space (improve the image)• interpretation guided

• Improved WEMVA• better approximations• no additional cost• further refinement