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CROSSWELL IMAGING BY 2-D CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION PRESTACK WAVEPATH MIGRATION H. Sun H. Sun Geology and Geophysics Department Geology and Geophysics Department University of Utah University of Utah
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CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Dec 20, 2015

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Page 1: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

CROSSWELL IMAGING BY 2-D CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH PRESTACK WAVEPATH

MIGRATIONMIGRATION

H. SunH. Sun

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

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

Offset (km)Offset (km)44 1010

De

pth

(k

m)

De

pth

(k

m)

0.50.5

2.52.5

44 Offset (km)Offset (km) 1010 44 Offset (km)Offset (km) 1010

KM ImageKM Image WM ImageWM ImageModelModel

SEG 2-D Overthrust DataSEG 2-D Overthrust Data

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

2-D Husky Field Data2-D Husky Field Data

Offset (km)Offset (km)2.52.5 5.55.5

2.52.5

5.05.0

De

pth

(k

m)

De

pth

(k

m)

KM Image (Zoom A)KM Image (Zoom A) WM Image (Zoom A)WM Image (Zoom A)

Offset (km)Offset (km)2.52.5 5.55.5

2.52.5

De

pth

(k

m)

De

pth

(k

m)

5.05.0

Page 4: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

WMWM

ModelModel

KM KM

SubSubWMWM

SEG 3-D Salt DataSEG 3-D Salt Data

Horizontal Slice (Depth=1.4 km)Horizontal Slice (Depth=1.4 km)

CPU:CPU:1/170 1/170

CPU:CPU:1/33 1/33

CPU:CPU:1 1

Page 5: CROSSWELL IMAGING BY 2-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 SSAA

AA

BB

BB

CC

CC

Page 6: CROSSWELL IMAGING BY 2-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

AABB

CC

Page 7: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Traveltime + Ray DirectionTraveltime + Ray Direction

TrueReflection point

SmallMigration Aperture

FewerFewerArtifactsArtifacts

LessLessExpensiveExpensive

Wavepath MigrationWavepath Migration

Page 8: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

OutlineOutline

• WM Crosswell ImagingWM Crosswell Imaging• Synthetic Crosswell Data Synthetic Crosswell Data • McElroy Crosswell DataMcElroy Crosswell Data• Synthetic Single Well DataSynthetic Single Well Data• ConclusionsConclusions

Page 9: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

KM Crosswell ImagingKM Crosswell ImagingReceiver Receiver

WellWell

Up-goingUp-going

Down-goingDown-going

Interface 2Interface 2

Source Source WellWell

Interface 1Interface 1

Page 10: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

KM Crosswell ImagingKM Crosswell ImagingReceiver Receiver

WellWell

Up-goingUp-going

Interface 2Interface 2

Source Source WellWell

Interface 1Interface 1

Page 11: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

KM Crosswell ImagingKM Crosswell ImagingReceiver Receiver

WellWellDown-goingDown-going

Interface 2Interface 2

Source Source WellWell

Interface 1Interface 1

Page 12: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

KM Crosswell ImagingKM Crosswell ImagingReceiver Receiver

WellWell

Up-goingUp-going

Down-goingDown-going

Interface 2Interface 2

Source Source WellWell

Interface 1Interface 1

Page 13: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Problems in KM Crosswell ImagingProblems in KM Crosswell Imaging

• Insufficient Stacking Leads to ArtifactsInsufficient Stacking Leads to Artifacts

• Complex Data Cause Difficulty inComplex Data Cause Difficulty in Up-going and Down-going SeparationUp-going and Down-going Separation

• Slow ComputationSlow Computation

Page 14: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

WM Crosswell ImagingWM Crosswell ImagingReceiver Receiver

WellWell

Up-goingUp-going

Down-goingDown-going

Interface 2Interface 2

Source Source WellWell

Interface 1Interface 1

Page 15: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Advantages of WM Crosswell ImagingAdvantages of WM Crosswell Imaging

• Avoid Artifacts by Migrating to theAvoid Artifacts by Migrating to the Primary Reflection PointPrimary Reflection Point

• Handle Complex Data by MigratingHandle Complex Data by Migrating Up-going and Down-going togetherUp-going and Down-going together

• No Constraints NeededNo Constraints Needed

• Fast ComputationFast Computation

Page 16: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Shortcomings of WMShortcomings of WM

• Weaker EventsWeaker Events

• Worse Interface ContinuityWorse Interface Continuity

Page 17: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

OutlineOutline

• WM Crosswell ImagingWM Crosswell Imaging• Synthetic Crosswell Data Synthetic Crosswell Data • McElroy Crosswell DataMcElroy Crosswell Data• Synthetic Single Well DataSynthetic Single Well Data• ConclusionsConclusions

Page 18: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Fault ModelFault Model A Common Shot GatherA Common Shot Gather

00 0000

9090

210210

210210

0.20.2

00Offset (m)Offset (m)

De

pth

(m

)D

ep

th (

m)

Tim

e (

s)T

ime

(s)

Geophone Depth (m)Geophone Depth (m)

Page 19: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

ModelModel

Crosswell Imaging of Synthetic Fault Data Crosswell Imaging of Synthetic Fault Data

Offset: 0~90 m, Depth: 0~210 mOffset: 0~90 m, Depth: 0~210 m

WMWMKM KM WM (no separation)WM (no separation)

Better ImageBetter ImageBetter ResolutionBetter Resolution

Page 20: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

OutlineOutline

• WM Crosswell ImagingWM Crosswell Imaging• Synthetic Crosswell Data Synthetic Crosswell Data • McElroy Crosswell DataMcElroy Crosswell Data• Synthetic Single Well DataSynthetic Single Well Data• ConclusionsConclusions

Page 21: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

A Common Shot GatherA Common Shot Gather

811811 963963

0.050.05

00

Tim

e (

s)T

ime

(s)

Hydrophone Depth (m)Hydrophone Depth (m)

Traveltime TomogramTraveltime Tomogram

00

8118115656

963963

Offset (m)Offset (m)

De

pth

(m

)D

ep

th (

m)

6.76.7

4.74.7

(k

m /s

)(k

m /s

)

Page 22: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

De

pth

(m

)D

ep

th (

m)

KM ImageKM Image

00 5656Offset (m)Offset (m)

Receiver WellReceiver WellSource WellSource Well

811811

963963SyntheticSyntheticSyntheticSynthetic

Up-goingUp-going

Down-goingDown-going

SeparationSeparation

??

??

Page 23: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

De

pth

(m

)D

ep

th (

m)

Receiver WellReceiver WellSource WellSource Well

811811

963963SyntheticSyntheticSyntheticSynthetic

Up-goingUp-going

Down-goingDown-going

SeparationSeparation

WM ImageWM Image

00 5656Offset (m)Offset (m)

Page 24: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

WM ImageWM Image

00 5656Offset (m)Offset (m)

De

pth

(m

)D

ep

th (

m)

Receiver WellReceiver WellSource WellSource Well

811811

963963SyntheticSyntheticSyntheticSynthetic

Up-goingUp-going

Down-goingDown-going

NO SeparationNO Separation

Page 25: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

Receiver WellReceiver Well

SyntheticSynthetic

Source WellSource Well

SyntheticSynthetic

WM (up+down)WM (up+down)WM(CPU=1)WM(CPU=1)KM(CPU=2.5)KM(CPU=2.5)

Offset: 0~56 m, Depth: 811~963 mOffset: 0~56 m, Depth: 811~963 m

Page 26: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

OutlineOutline

• WM Crosswell ImagingWM Crosswell Imaging• Synthetic Crosswell Data Synthetic Crosswell Data • McElroy Crosswell DataMcElroy Crosswell Data• Synthetic Single Well DataSynthetic Single Well Data• ConclusionsConclusions

Page 27: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

OYO Salt ModelOYO Salt Model

9900

Velocity (km/s)Velocity (km/s)

00

66

Offset (km)Offset (km)

De

pth

(k

m)

De

pth

(k

m)

WellWell

SaltSalt

? ? ? ?? ? ? ?

????

????

4.54.52.82.8

Page 28: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

KM imageKM image22

55

Dep

th (

km)

Dep

th (

km)

6.56.52.52.5 Offset (km)Offset (km) 6.56.52.52.5 Offset (km)Offset (km) 6.56.52.52.5 Offset (km)Offset (km)

OYO Salt ModelOYO Salt Model

Velocity ModelVelocity Model WM imageWM image

????

????

????? ?????

WellWell

Page 29: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

ConclusionsConclusions

Crosswell Synthetic DataCrosswell Synthetic Data• Fewer migration artifactsFewer migration artifacts• Slightly better image resolutionSlightly better image resolution• Better for dipping fault boundaryBetter for dipping fault boundary• No up- and down-going separationNo up- and down-going separation

Page 30: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

ConclusionsConclusions

Crosswell McElroy DataCrosswell McElroy Data• Similar image qualitySimilar image quality• No up- and down-going separationNo up- and down-going separation• 2.5 times faster than KM2.5 times faster than KM• Worse image continuityWorse image continuity• Structure details? Artificial events?Structure details? Artificial events?

Page 31: CROSSWELL IMAGING BY 2-D PRESTACK WAVEPATH MIGRATION H. Sun Geology and Geophysics Department University of Utah.

ConclusionsConclusions

Single Well Synthetic DataSingle Well Synthetic Data• Similar image qualitySimilar image quality• Fewer migration artifactsFewer migration artifacts

Page 32: CROSSWELL IMAGING BY 2-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