seismic refraction method lec22

32
Seismic Refraction Method Overview (2) Prepared by Dr. Amin Khalil

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Page 1: Seismic refraction method lec22

Seismic Refraction Method

Overview (2)

Prepared byDr. Amin Khalil

Page 2: Seismic refraction method lec22

Overview

Types and Properties of seismic waves

Seismic waves at an interface

Basic laws for seismic refraction

T-X graph (travel time distance curve)

Interpretation & Modeling

Page 3: Seismic refraction method lec22

Travel time distance graph

T-x graph is made by picking the first onset of the first arrival seismic phases. The picked phase should be defined with great care. For refraction, which is an active source method, the first onset should generally be compressional, hence the polarity of the onset should be positive. We must take care because under certain circumstances the onset is masked due to noise and we may pick later arrivals that may be of –ve polarity.

Page 4: Seismic refraction method lec22

Travel time curve

When the picked data is plotted, it will be time versus distances, that’s why we call it T-X or travel time distance curve.

Page 5: Seismic refraction method lec22

Horizontal FlatInterface

Page 6: Seismic refraction method lec22

• Horizontal interfaces provide a simple introduction to the construction of T-X diagrams.

• Close to the source, the first arrival is due to the direct ray travelling in layer 1.

• This plots as a straight line on the T-X diagram.

• The slope of the line is the reciprocal of the layer 1 velocity (assuming distance is on the X-axis).

• The intercept is zero.

Page 7: Seismic refraction method lec22
Page 8: Seismic refraction method lec22

• When the critical distance is exceeded, refraction occurs and some energy enters layer 2. A refracted ray then travels at V2 sending return rays back to the surface as it does so.

• At some point (the cross-over distance) the refracted ray (being the faster) will overtake the direct ray and the return rays will become the first arrivals, despite their longer travel distance.

• It is these that are now plotted on the T-X diagram

Page 9: Seismic refraction method lec22
Page 10: Seismic refraction method lec22

• The T-X diagram thus develops an upper branch due to the refracted ray.

• This is again a straight line, whose slope is the reciprocal of V2 .

• There is now an intercept time (T1) whose value is determined by the layer 1 thickness and the two velocities

• The intercept time is an example of a delay time sum, composed of the separate times taken by the signal to descend to the interface and then to return to the surface.

Page 11: Seismic refraction method lec22
Page 12: Seismic refraction method lec22

11 /VxT

1212

Vdf

Vcd

VacT

)cos( cihdfac

)tan( cihdebc

)tan(2 cihxdebcxcd

2)(12

)tan(2cos2

Vihx

iVhT c

c

22)(12

)tan(2cos2

Vx

Vih

iVhT c

c

22)(12

)cos()sin(

cos12

Vx

iVi

iVhT

c

c

c

Page 13: Seismic refraction method lec22

Using Seismic Refraction to Map the Subsurface

Depth{

12

12

2 VVVVXcDepth

Page 14: Seismic refraction method lec22

Interpretation using intercept time• The intercept time is given by

• Since, in this case, the ray path is symmetrical, the intercept time is the sum of two equal delay times

12

21

222VVVV

zT

Page 15: Seismic refraction method lec22

15

3 layer case

Page 16: Seismic refraction method lec22

• By a similar argument, a third layer introduces a third branch into the T-X diagram.

• The slope is the reciprocal of V3 and the intercept is a composite of the layer 1 and layer 2 delay times.

12

21

22

213

21

23

12 22VVVV

zVVVV

zT

Page 17: Seismic refraction method lec22

Delay Time Method• Allows Calculation of Depth Beneath Each Geophone

• Requires refracted arrival at each geophone from opposite directions

• Requires offset shots

• Data redundancy is important

Page 18: Seismic refraction method lec22
Page 19: Seismic refraction method lec22
Page 20: Seismic refraction method lec22
Page 21: Seismic refraction method lec22
Page 22: Seismic refraction method lec22
Page 23: Seismic refraction method lec22

Delay Time Methodx

V1

V2

Page 24: Seismic refraction method lec22

x

V1

V2

)cos()tan()tan(

)cos( 12221 c

BcBcA

c

AAB

iVh

Vih

Vih

VAB

iVhT

Page 25: Seismic refraction method lec22

Delay Time Methodx

)cos()tan()tan(

)cos( 12221 c

PcPcB

c

BBP

iVh

Vih

Vih

VBP

iVhT

)cos()tan()tan(

)cos( 12221 c

PcPcA

c

AAP

iVh

Vih

Vih

VAP

iVhT

)cos()tan()tan(

)cos( 12221 c

BcBcA

c

AAB

iVh

Vih

Vih

VAB

iVhT

V1

V2

Page 26: Seismic refraction method lec22

Delay Time Methodx

t T T TAP BP AB0

Definition:

V1

V2

(7)

Page 27: Seismic refraction method lec22

ABBPAP TTTt 0

)cos(

)tan()tan()cos( 12221

0c

PcPcA

c

A

iVh

Vih

Vih

VAP

iVht

)cos(

)tan()tan()cos( 12221 c

PcPcB

c

B

iVh

Vih

Vih

VBP

iVh

)cos(

)tan()tan()cos( 12221 c

BcBcA

c

A

iVh

Vih

Vih

VAB

iVh

2120

)tan(2)cos(

2V

ihiV

hV

ABBPAPt cP

c

p

Page 28: Seismic refraction method lec22

But from figure above, BPAPAB . Substituting, we get

2120

)tan(2)cos(

2V

ihiV

hV

BPAPBPAPt cP

c

p

or

210

)tan(2)cos(

2V

ihiV

ht cP

c

p

Page 29: Seismic refraction method lec22

)cos(

)sin()cos(

1221

0c

c

cp

iVi

iVht

)cos(

)sin()cos(

221

1

21

20

c

c

cp

iVViV

iVVVht

)cos(

)sin()cos(

22121

1

2

10c

c

cp

iVVi

iVVVV

Vht

2

1sinVVicSubstituting from Snell’s Law,

)cos(

)sin()cos(

sin1

22121

10c

c

c

cp

iVVi

iVViVht

Page 30: Seismic refraction method lec22

)cos(

)sin()cos(

sin1

22121

10c

c

c

cp

iVVi

iVViVht

Multiplying top and bottom by sin(ic)

)cos()sin(

)(sin)cos()sin(

1221

2

2110

cc

c

ccp

iiVVi

iiVVVht

)cos()sin(

)(cos221

2

10cc

cp

iiVViVht

)sin(

)cos(22

0c

cp

iViht

)sin(

)cos(22

0c

cp

iViht

Page 31: Seismic refraction method lec22

2

1sinVVic

Substituting from Snell’s Law,

10

)cos(2V

iht cp (8)

We get

Page 32: Seismic refraction method lec22

11

)cos(2

)cos(22

Ppoint at Delay timeVih

VihtD cpcpo

TP (9)