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3-D PRESTACK WAVEPATH 3-D PRESTACK WAVEPATH MIGRATION MIGRATION H. Sun H. Sun Geology and Geophysics Department Geology and Geophysics Department University of Utah University of Utah
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3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Dec 21, 2015

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Page 1: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

3-D PRESTACK WAVEPATH 3-D PRESTACK WAVEPATH MIGRATIONMIGRATION

H. SunH. Sun

Geology and Geophysics Department Geology and Geophysics Department University of UtahUniversity of Utah

Page 2: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

OutlineOutline

Problems in 2-D WMProblems in 2-D WM• Objectives of 3-D WM Objectives of 3-D WM • Numerical ResultsNumerical Results• ConclusionsConclusions

Page 3: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

• Lower CPU EfficiencyLower CPU Efficiency only 1/3 faster than KMonly 1/3 faster than KM or even 2 times slower than KMor even 2 times slower than KM• Moderate CPU EfficiencyModerate CPU Efficiency 4~11 times faster than KM4~11 times faster than KM By Slant StackingBy Slant Stacking

Problems in 2-D WMProblems in 2-D WM

Page 4: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

2-D KM of a Single Trace2-D KM of a Single Trace

RR SS

NNNN

11

11CPU Count = NCPU Count = N 22

AA

AA

BB

BB

CC

CC

Page 5: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

2-D WM of a Single Trace2-D WM of a Single Trace

RR SSAA

BBCC

CPU Count = 3 * ( Tracing + Searching + Migrating )CPU Count = 3 * ( Tracing + Searching + Migrating ) = 3 * ( N + 2N + 7N) = 30N = 3 * ( N + 2N + 7N) = 30N

NNNN

11

11

AABB

CC

Page 6: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

OutlineOutline

• Problems in 2-D WMProblems in 2-D WM Objectives of 3-D WM Objectives of 3-D WM • Numerical ResultsNumerical Results• ConclusionsConclusions

Page 7: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

• To Achieve Higher CPU EfficiencyTo Achieve Higher CPU Efficiency Compared to 3-D KMCompared to 3-D KM • To Generate Comparable or BetterTo Generate Comparable or Better Image Quality than 3-D KMImage Quality than 3-D KM

Key Goals of 3-D WMKey Goals of 3-D WM

Page 8: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

OutlineOutline• Problems in 2-D WMProblems in 2-D WM• Objectives of 3-D WM Objectives of 3-D WM Numerical ResultsNumerical Results 3-D Point Scatterer Data3-D Point Scatterer Data 3-D SEG/EAGE Salt Data3-D SEG/EAGE Salt Data 3-D West Texas Field Data3-D West Texas Field Data• ConclusionsConclusions

Page 9: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

3-D Prestack KM Point Scatterer Response3-D Prestack KM Point Scatterer Response R

efle

ctiv

ity

Ref

lect

ivit

y

Y Offset (km)Y Offset (km) X Offset (km)X Offset (km)

11

-0.5-0.5

00

11

Ref

lect

ivit

yR

efle

ctiv

ity

Y Offset (km)Y Offset (km) X Offset (km)X Offset (km)

11

-0.01-0.01

00

0.020.02

Ref

lect

ivit

yR

efle

ctiv

ity

Y Offset (km)Y Offset (km) X Offset (km)X Offset (km)

11

-0.05-0.05

00

0.10.1

Ref

lect

ivit

yR

efle

ctiv

ity

Y Offset (km)Y Offset (km) X Offset (km)X Offset (km)

11

-0.2-0.2

00

0.40.4

11

1111

11

Z0Z0

Z0-1Z0-1Z0-9Z0-9

Z0+8Z0+8

Page 10: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Ref

lect

ivit

yR

efle

ctiv

ity

Y Offset (km)Y Offset (km) X Offset (km)X Offset (km)

11

-0.5-0.5

00

11

Ref

lect

ivit

yR

efle

ctiv

ity

Y Offset (km)Y Offset (km) X Offset (km)X Offset (km)

11

-0.01-0.01

00

0.020.02

Ref

lect

ivit

yR

efle

ctiv

ity

Y Offset (km)Y Offset (km) X Offset (km)X Offset (km)

11

-0.05-0.05

00

0.10.1

Ref

lect

ivit

yR

efle

ctiv

ity

Y Offset (km)Y Offset (km) X Offset (km)X Offset (km)

11

-0.2-0.2

00

0.40.4

11

1111

11

3-D Prestack WM Point Scatterer Response3-D Prestack WM Point Scatterer Response

Z0Z0

Z0-1Z0-1Z0-9Z0-9

Z0+8Z0+8

Page 11: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

OutlineOutline• Problems in 2-D WMProblems in 2-D WM• Objectives of 3-D WM Objectives of 3-D WM Numerical ResultsNumerical Results 3-D Point Scatterer Data3-D Point Scatterer Data 3-D SEG/EAGE Salt Data3-D SEG/EAGE Salt Data 3-D West Texas Field Data3-D West Texas Field Data• ConclusionsConclusions

Page 12: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

A Common Shot GatherA Common Shot GatherTrace NumberTrace Number11 390390

Tim

e (s

ec)

Tim

e (s

ec)

00

5.05.0

Page 13: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Receiver DistributionReceiver DistributionC

ross

line

(m)

Cro

sslin

e (m

)

44804480

23202320

19201920

19201920 Inline (m)Inline (m)

Page 14: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Inline Velocity ModelInline Velocity Model

Offset (km)Offset (km)00 9.29.2

Dep

th (

km)

Dep

th (

km)

00

3.83.8

SALTSALT

Page 15: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Inline KMInline KM ((CPU=1CPU=1)) Inline WMInline WM ((CPU=1/33CPU=1/33))

Offset (km)Offset (km)00 9.29.2

00

3.83.8

De

pth

(k

m)

De

pth

(k

m)

Offset (km)Offset (km)00 9.29.2

Page 16: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Receiver DistributionReceiver DistributionC

ross

line

(m)

Cro

sslin

e (m

)

44804480

23202320

19201920

19201920 Inline (m)Inline (m)

Page 17: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Inline KMInline KM ((CPU=1CPU=1)) Inline WMInline WM ((CPU=1/170CPU=1/170))

Offset (km)Offset (km)00 9.29.2

00

3.83.8

De

pth

(k

m)

De

pth

(k

m)

Offset (km)Offset (km)00 9.29.2

(subsample)(subsample)

Page 18: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Zoom Views of Inline Sections Zoom Views of Inline Sections

Offset: 3~6.5 km, Depth: 0.3~1.8 kmOffset: 3~6.5 km, Depth: 0.3~1.8 km

WMWM

ModelModel

KM KM

SubSubWMWM

Page 19: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Offset: 1.8~4 km, Depth: 0.6~2.1 kmOffset: 1.8~4 km, Depth: 0.6~2.1 km

WMWM

ModelModel

KM KM

SubSubWMWM

Zoom Views of Crossline Sections Zoom Views of Crossline Sections

Page 20: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Inline: 1.8~7.2 km, Crossline: 0~4 kmInline: 1.8~7.2 km, Crossline: 0~4 km

WMWM

ModelModel

KM KM

SubSubWMWM

Horizontal Slices (Depth=1.4 km) Horizontal Slices (Depth=1.4 km)

Page 21: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

OutlineOutline• Problems in 2-D WMProblems in 2-D WM• Objectives of 3-D WM Objectives of 3-D WM Numerical ResultsNumerical Results 3-D Point Scatterer Data3-D Point Scatterer Data 3-D SEG/EAGE Salt Data3-D SEG/EAGE Salt Data 3-D West Texas Field Data3-D West Texas Field Data• ConclusionsConclusions

Page 22: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

A Common Shot GatherA Common Shot GatherTrace NumberTrace Number5454 193193

Tim

e (s

ec)

Tim

e (s

ec)

00

3.43.4

Page 23: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Receiver DistributionReceiver DistributionC

ross

line

(km

)C

ross

line

(km

)

4.54.51.21.2

3.53.5

1.51.5 Inline (km)Inline (km)

Page 24: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Receiver DistributionReceiver DistributionC

ross

line

(km

)C

ross

line

(km

)

4.54.51.21.2

3.53.5

1.51.5 Inline (km)Inline (km)

Page 25: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Inline KM Inline KM ((CPU=1CPU=1)) Inline WMInline WM ((CPU=1/14CPU=1/14))

Offset (km)Offset (km)0.40.4 4.54.5

0.80.8

3.83.8

De

pth

(k

m)

De

pth

(k

m)

Offset (km)Offset (km)0.40.4 4.54.5

Page 26: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Inline KMInline KM ((CPU=1CPU=1)) Inline WMInline WM ((CPU=1/50CPU=1/50))

Offset (km)Offset (km)0.40.4 4.54.5

0.80.8

3.83.8

De

pth

(k

m)

De

pth

(k

m)

Offset (km)Offset (km)0.40.4 4.54.5

(subsample)(subsample)

Page 27: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Crossline KM Crossline KM ((CPU=1CPU=1)) Crossline WMCrossline WM ((CPU=1/14CPU=1/14))

Offset (km)Offset (km)0.30.3 3.53.5

0.80.8

3.33.3

De

pth

(k

m)

De

pth

(k

m)

Offset (km)Offset (km)0.30.3 3.53.5

Page 28: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Crossline KMCrossline KM ((CPU=1CPU=1)) Crossline WMCrossline WM ((CPU=1/50CPU=1/50))(subsample)(subsample)

Offset (km)Offset (km)0.30.3 3.53.5

0.80.8

3.33.3

De

pth

(k

m)

De

pth

(k

m)

Offset (km)Offset (km)0.30.3 3.53.5

Page 29: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Inline: 0~4.6 km, Crossline: 0~3.8Inline: 0~4.6 km, Crossline: 0~3.8

KM (KM (CPU=1CPU=1))

Horizontal Slices (Depth=2.5 km) Horizontal Slices (Depth=2.5 km)

WM (WM (CPU=1/14CPU=1/14)) WM (Sub, WM (Sub, CPU=1/50CPU=1/50))

Page 30: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

OutlineOutline

• Problems in 2-D WMProblems in 2-D WM• Objectives of 3-D WM Objectives of 3-D WM • Numerical ResultsNumerical Results ConclusionsConclusions

Page 31: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

ConclusionsConclusions

SEG/EAGE Salt DataSEG/EAGE Salt Data• Fewer Migration ArtifactsFewer Migration Artifacts• Better for Complex Salt BoundaryBetter for Complex Salt Boundary• Higher Computational EfficiencyHigher Computational Efficiency

CPUCPU KM: KM: 11 WM: WM: 1/331/33 Subsampled WM: Subsampled WM: 1/1701/170

Page 32: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

ConclusionsConclusions

West Texas Field DataWest Texas Field Data• Fewer Migration ArtifactsFewer Migration Artifacts• Similar Image QualitySimilar Image Quality• Higher Computational EfficiencyHigher Computational Efficiency

CPUCPU KM: KM: 11 WM: WM: 1/141/14 Subsampled WM: Subsampled WM: 1/501/50

Page 33: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

ConclusionsConclusions

• Trade-off:Trade-off: between Image Quality between Image Quality and CPU Costsand CPU Costs

• Caution:Caution: WM Angle Estimation WM Angle Estimation Sensitive to Recording Geometry Sensitive to Recording Geometry

Page 34: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

• More Robust Angle CalculationMore Robust Angle Calculation• Crossing-event CalculationCrossing-event Calculation• 3-D Marine Field Data3-D Marine Field Data• 3-D Iterative Velocity Analysis3-D Iterative Velocity Analysis

Future WorkFuture Work

Page 35: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Real-time Velocity UpdatingReal-time Velocity Updatingfor Target-oriented Migrationfor Target-oriented Migration

Possible ?Possible ?

QuestionQuestion

Page 36: 3-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

AcknowledgementsAcknowledgements

I thank UTAM sponsorsI thank UTAM sponsorsfor their financial supportfor their financial support