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The Elastic Wave Equation

 Elastic waves in infinite homogeneous isotropic media

Numerical simulations for simple sources

 Plane wave propagation in infinite media

Frequency, wavenumber, wavelength

 Conditions at material discontinuities

Snell’s Law

Reflection coefficients

Free surface

 Reflection Seismology: an example from the Gulf of Mexico

(2)

Equations of motion

What are the solutions to this equation? At first we look at infinite homogeneous isotropic media, then:

ij j i

i

t

u f

 

2

  

ij ij

ij

 

   2

) (

i j j i

ij k k

ij

   u     u   u

( )

2

i j j

i ij

k k j

i

i

f u u u

t

u        

   

u u

u f

u

2

2

        

   

(3)

Equations of motion – homogeneous media

We can now simplify this equation using the curl and div operators

2 2

2 2

z y

x

   

i j

j i k

k i i

i

f u u u

u

j

t

2

2

        

   

u -

u f

u         

   

2

( 2 )

t

i i

u u  

and  u    u -     u

… this holds in any coordinate system …

This equation can be further simplified, separating the wavefield into curl

free and div free parts

(4)

Equations of motion – P waves u -

u

u        

   

2

( 2 )

t

Let us apply the div operator to this equation, we obtain

 

2

 (  2 ) 

t

where

u

i

u  

i

 

or

  

2t 2

   2

P wave velocity Acoustic wave

equation

(5)

Equations of motion – shear waves u -

u

u        

   

2

( 2 )

t

Let us apply the curl operator to this equation, we obtain

) (

)

2

(

i

i

u

t

  u         

    

we now make use of      0 and define to obtain

  

2 2

t

  

i

u

i

 

Shear wave

velocity Wave equation for

shear waves

(6)

Elastodynamic Potentials

Any vector may be separated into scalar and vector potentials

u



 

Shear waves have no change in volume

  

2 2

t

P-waves have no rotation

where F is the potential for P waves and Y the potential for shear waves



  u

  

2 2

t

(7)

Seismic Velocities

Material and Source P-wave velocity (m/s) shear wave velocity (m/s)

Water 1500 0

Loose sand 1800 500

Clay 1100-2500

Sandstone 1400-4300

Anhydrite, Gulf Coast 4100

Conglomerate 2400

Limestone 6030 3030

Granite 5640 2870

Granodiorite 4780 3100

Diorite 5780 3060

Basalt 6400 3200

Dunite 8000 4370

Gabbro 6450 3420

(8)

Solutions to the wave equation - general

Let us consider a region without sources

Where n could be either dilatation or the vector potential and c is either P- or shear-wave velocity. The general solution to this equation is:

  

2

c

2

t

Let us take a look at a 1-D example

) (

) ,

( x

i

tG a

j

x

j

ct

(9)

Solutions to the wave equation - harmonic

Let us consider a region without sources

  

2

c

2

t

The most appropriate choice for G is of course the use of harmonic functions:

)]

( exp[

) ,

( x t A ik a x ct

u

i i

i j j

(10)

Solutions to the wave equation - harmonic

… taking only the real part and considering only 1D we obtain

)]

( cos[

) ,

( x t A k x ct

u  

T t x

t x

kct kx

ct x

k

 

 2 2

) 2

(       

c wave speed

k wavenumber

l wavelength

T period

w frequency

A amplitude

(11)

Spherical Waves

Let us assume that h is a function of the distance from the source

where we used the definition of the Laplace operator in spherical coordinates

let us define

to obtain

  

2

c

2

t

r r t

c

r

2 2

2

 2   1 

r 

r

  

  

2

c

2

t

with the known solution   f ( r   t )

(12)

Geometrical spreading

so a disturbance propagating away with spherical wavefronts decays like

... this is the geometrical spreading for spherical waves, the amplitude decays proportional to 1/r.

r

If we had looked at cylindrical waves the result would have been that the waves decay as (e.g. surface waves)

t r r

r f

) 1 1 (

  

r

 1

(13)

Plane waves

... what can we say about the direction of displacement, the polarization of seismic waves?

uuPS

P S    

... we now assume that the potentials have the well known form of plane harmonic waves

) (

exp i t

A   

k x   B exp i ( kx   t ) )

(

exp i t

A   

k k x

P SkB exp i ( kx   t )

shear waves are transverse because S is normal to the wave vector k P waves are longitudinal as P is

parallel to k

(14)

Heterogeneities

.. What happens if we have heterogeneities ?

Depending on the kind of reflection part or all of the signal is reflected or transmitted.

 What happens at a free surface?

 Can a P wave be converted in an S wave

 or vice versa?

 How big are the amplitudes of the

 reflected waves?

(15)

Wavenumber, slowness, phase velocity

(16)

Reflection at an interface

(17)

Boundary Conditions

... what happens when the material parameters change?

r

1

v

1

r

2

v

2

welded interface

At a material interface we require continuity of displacement and

traction

A special case is the free surface condition, where the surface tractions

are zero.

(18)

Reflection and Transmission – Snell’s Law

What happens at a (flat) material discontinuity?

Medium 1: v

1

Medium 2: v

2

i

1

i

2

2 1 2

1

sin sin

v v i

i

But how much is reflected, how much transmitted?

(19)

Reflection and Transmission coefficients

Medium 1: r1,v1

Medium 2: r2,v2

T

Let’s take the most simple example: P-waves with normal incidence on a material interface

A R

1 1 2

2

1 1 2

2

  A R

1 1 2

2

1

2 1

  A T

At oblique angles conversions from S-P, P-S have to be

considered.

(20)

Reflection and Transmission – Ansatz

How can we calculate the amount of energy that is transmitted or reflected at a material discontinuity?

We know that in homogeneous media the displacement can be described by the corresponding potentials

u

in 2-D this yields

y x z

z

z x x

z y

z y x

x

u u u

an incoming P wave has the form

) (

0

exp i a x t

A

j j

(21)

Reflection and Transmission – Ansatz

... here a

i

are the components of the vector normal to the wavefront : a

i

=(cos e, 0, -sin e), where e is the angle between surface and ray direction, so that for the free surface

where

) ' tan

( ' exp

) tan

( exp )

tan (

exp

3 1

3 1

3 1

0

t c f

x x

ik B

ct e

x x

ik A

ct e

x x

ik A

e c k

c e

cos cos

f k

c f

cos '

' cos

P

P

r

SV

r

e f

what we know is that

0 0

zz xz

(22)

Reflection and Transmission – Coefficients

... putting the equations for the potentials (displacements) into these equations leads to a relation between incident and reflected

(transmitted) amplitudes

2 2

2 0

2 2

2 2

0

) tan

1 ( tan

tan 4

) tan

1 ( tan

4

) tan

1 ( tan

tan 4

) tan

1 ( tan

tan 4

f f

e

f e

A R B

f f

e

f f

e A

R A

PS PP

 

 

These are the reflection coefficients for a plane P wave incident

on a free surface, and reflected P and SV waves.

(23)

Case 1: Reflections at a free surface

A P wave is incident at the free surface ...

P P

SV i j

The reflected amplitudes can be described by the scattering matrix S

 

 

  u d u d S S S

P

P S P

S P

(24)

Example

(25)

Case 2: SH waves

For layered media SH waves are completely decoupled from P and SV waves

There is no conversion only SH waves are reflected or transmitted

 

 

 

d u d

u

d u d

u

S S S

S

S S S

S S

SH

(26)

Example

(27)

Case 3: Solid-solid interface

To account for all possible reflections and transmissions we need 16 coefficients, described by a 4x4 scattering matrix.

P SV

r

P

r

P

t

SV

t

(28)

Case 4: Solid-Fluid interface

At a solid-fluid interface there is no conversion to SV in the lower medium.

P SV

r

P

r

P

t

(29)

Reflection coefficients - example

(30)

Refractions – waveform effects

(31)

Reservoir example

(32)

Example: Gulf of Mexico

(33)

Summary

 Reflection and transmission coefficients can be derived using plane waves and boundary conditions

 Cases include:

 solid-solid

 solid-fluid

 fluid-solid

 solid-free surface

 fluid-free surface

 The angular dependence of R-T coefficients is complex.

Their behaviour allows constraining the change of

physical properties.

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