Fault Detection by a Seismic Scanning Tunneling Macroscope

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Fault Detection by a Seismic Scanning Tunneling Macroscope Sherif M. Hanafy

description

Fault Detection by a Seismic Scanning Tunneling Macroscope. Sherif M. Hanafy. Outline. Introduction Motivation. Get super resolution by TRM Method. TRM & mute-window test Synthetic Test. 2D elastic simulation Field Test. 3D fault test Conclusions. Outline. - PowerPoint PPT Presentation

Transcript of Fault Detection by a Seismic Scanning Tunneling Macroscope

Page 1: Fault Detection by a Seismic Scanning Tunneling  Macroscope

Fault Detection by a Seismic Scanning Tunneling Macroscope

Sherif M. Hanafy

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Outline

• Introduction• Motivation. Get super resolution by TRM• Method. TRM & mute-window test• Synthetic Test. 2D elastic simulation• Field Test. 3D fault test• Conclusions

Page 3: Fault Detection by a Seismic Scanning Tunneling  Macroscope

Outline

• Introduction• Motivation. Get super resolution by TRM• Method. TRM & The mute-window test• Synthetic Test. 2D elastic simulation• Field Test. 3D fault test• Conclusions

Page 4: Fault Detection by a Seismic Scanning Tunneling  Macroscope

Introduction: Resolution

L

Z

Δx

X

Depth

Rayleigh resolutionLZx

2

Abbe resolution2

x

Super resolution2

x

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Outline

• Introduction• Motivation. Get super resolution by TRM• Method. TRM & The mute-window test• Synthetic Test. 2D elastic simulation• Field Test. 3D fault test• Conclusions

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Motivation

Motivation: Achieve super resolution

IBM, 1986, Scanning Tunneling Microscope

Problem: Source and receiver need to be in the near-field

Solution: Use scatterer points

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Outline

• Introduction• Motivation. Get super resolution by TRM• Method. TRM & The mute-window test• Synthetic Test. 2D elastic simulation• Field Test. 3D fault test• Conclusions

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Post-stack Migration

𝑮(𝒈∨𝒔𝒐)

ZO Migration Formula

𝒎 (𝒔′ )=∑𝒈𝑮∗(𝒈∨𝒔′ )𝑮(𝒈∨𝒔𝒐 )  

𝒔 ′ImagePlane

𝒔𝒐

MeasuredData

CalculatedData

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Post-stack Migration with Point Scatterer

𝑮(𝒈∨𝒔𝒐) ZO Migration Formula

𝒎 (𝒔′ )=∫−𝝎

𝝎

∫−𝑳

𝑳

𝑮 (𝒔𝒐|𝒔 )𝑮 (𝒈|𝒔𝒐 )𝑮∗ (𝒔𝒐|𝒔 ′ )𝑮∗ (𝒈|𝒔𝒐 )𝒅𝒈𝒅𝝎

𝒔 ′ImagePlane

𝒔𝒐

𝒔𝑮(𝒔𝒐∨𝒔)

MeasuredData

CalculatedData

Page 10: Fault Detection by a Seismic Scanning Tunneling  Macroscope

Post-stack Migration with Point Scatterer𝒎 (𝒔′ )=∫

−𝝎

𝝎

∫−𝑳

𝑳

𝑮 (𝒔𝒐|𝒔 )𝑮 (𝒈|𝒔𝒐 )𝑮∗ (𝒔𝒐|𝒔 ′ )𝑮∗ (𝒈|𝒔𝒐 )𝒅𝒈𝒅𝝎

𝑮 ( 𝒙|𝒙′ )= 𝒆𝒊𝝎|𝒙−𝒙′|/𝒄

¿ 𝒙−𝒙 ′∨¿¿

𝒎 (𝒔′ )=∫−𝝎

𝝎 𝒆𝒊 𝝎(|𝒔−𝒔𝒐❑|−|𝒔 ′−𝒔𝒐

❑|)/𝒄

(|𝒔−𝒔𝒐❑||𝒔 ′−𝒔𝒐

❑|)𝒅𝝎∫

−𝑳

𝑳 𝟏¿𝒈−𝒔𝒐¿

𝟐 𝒅𝒈

𝒎 (𝒔′ )=𝒔𝒊𝒏 ¿¿

𝒎 (𝒔′ )=𝑨 .𝑩

0.2 0.7S’

|s-s0| ~

S’0.2 0.7

|s-s0| ~ /40

Near-field->super-resolution Far-field->Rayleigh resolution

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Time Reversal Mirror(TRM)

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Time Reversal Mirrors (TRM)

𝑮(𝒈∨𝒔𝒐)

ZO Migration Formula

𝒎 (𝒔′ )=∑𝒈𝑮∗(𝒈∨𝒔′ )𝑮(𝒈∨𝒔𝒐 )  

𝒔 ′ImagePlane

𝒔𝒐

MeasuredData

CalculatedData

Page 13: Fault Detection by a Seismic Scanning Tunneling  Macroscope

Time Reversal Mirrors (TRM)

𝑮(𝒈∨𝒔𝒐)

ZO Migration Formula

𝒎 (𝒔′ )=∑𝒈𝑮∗(𝒈∨𝒔′ )𝑮(𝒈∨𝒔𝒐 )  

𝒔 ′ImagePlane 𝒔𝒐

MeasuredData

CalculatedData

𝒔 ′

MeasuredData

TRM Profile

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Summary

0.2 0.7S’

|s-s0| ~

S’0.2 0.7

|s-s0| ~ /40

Near-field->super-resolution Far-field->Rayleigh resolution

ImagePlane 𝒔𝒐𝒔 ′

TRM Profile

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Outline

• Introduction• Motivation. Get super resolution by TRM• Method. The mute-window test• Synthetic Test. 2D elastic simulation• Field Test. 3D fault test• Conclusions

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Velocity Model

120 receivers at 1 m receiver interval120 shots at 1 m shot interval

Dep

th (m

)

X (m)

0

400 120

Vp (m/s)500 3500Vs (m/s)250 1750Density (gm/cc)2.0 2.6

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TRM ProfilesSource # 34 Source # 80A

mpl

itude

Trial Source

1

-0.21 120

TRM ProfileNo traces are muted

Am

plitu

de

Trial Source

1

-0.21 120

TRM Profile21 traces are muted

Am

plitu

de

Trial Source

1

-0.21 120

TRM Profile101 traces are muted

Am

plitu

de

Trial Source

1

-0.21 120

TRM ProfileNo traces are muted

Am

plitu

de

Trial Source

1

-0.21 120

TRM Profile21 traces are muted

Am

plitu

de

Trial Source

1

-0.21 120

TRM Profile101 traces are muted

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TRM ImagesSource # 34 Source # 80M

ute-

win

dow

Siz

e

Trial Source

0

1111 120

Source Location

a) TRM Image of Shot # 34

Mut

e-w

indo

w S

ize

Trial Source

0

1111 120

Source Location

b) TRM Image of Shot # 80

Scatterers in the near-field of the sourceReceiver are only at far-field

Scatterers in the far-field of the sourceReceiver are only at far-field

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Outline

• Introduction• Motivation. Get super resolution by TRM• Method. TRM & The mute-window test• Synthetic Test. 2D elastic simulation• Field Test. 3D fault test• Summary

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Field Test

• Data Collected at Washington Fault Area, north of Arizona, USA.

• 6 Lines of receivers/shots• 80 receivers/line at 1 m

receiver interval• 40 shots/line at 2 m shot

interval

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Data Collection

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Tomography and Ground Truth

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Super Resolution Test

Pixel size: 2 x 1.5 m2

Wavelength: 10 m

Fault

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Migration Image – Traces within 0.8 λ are mutedMigration Image – Traces within 0.4 λ are muted

Super Resolution Results

Migration Image – Traces within 0.1 λ are mutedMigration Image using All TracesFault

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Outline

• Introduction• Motivation. Get super resolution by TRM• Method. TRM & The mute-window test• Synthetic Test. 2D elastic simulation• Field Test. 3D fault test• Conclusions

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Conclusions• TRM profiles have the shape of

a sink curve if no scatterer in the near-field of the shot point

• TRM profiles have the shape of a spike if scatterer exists in the near-field of the shot point

• Muting the near-field traces tends to decrease the amplitude of the TRM profile and its resolution

0.2 0.7S’

|s-s0| ~

S’0.2 0.7

|s-s0| ~ /40

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Possible Applications

Find local anomalies, faults, and scatterer points around boreholes in VSP data

Ground

Borehole

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Thank You