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Seismic velocity tomography with co-located soft data Mohammad Maysami Bob Clapp Stanford University SCRF Affiliate Meeting May 2009

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Page 1: Seismic velocity tomography with co-located soft data · 2009. 5. 29. · Seismic velocity tomography with co-located soft data Mohammad Maysami Bob Clapp ... ‣ resolution decreases

Seismic velocity tomography with co-located soft data

Mohammad Maysami Bob Clapp

Stanford University

SCRF Affiliate MeetingMay 2009

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SCRF Annual MeetingMohammad Maysami

Motivation

‣ soft data constrains flow simulation

2

model

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SCRF Annual MeetingMohammad Maysami

Outline

‣ Introduction

‣ Seismic tomography

‣ Geological constraints for velocity analysis

‣ Cross Gradients Function

• Accuracy in different frequency intervals

‣ Results

‣ Future work:

• Western Geco Dataset: Seismic & Resistivity

3

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Introduction

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SCRF Annual MeetingMohammad Maysami

Schematic of seismic imaging

5

s g

Model:v, ρ

Data

Image

Velocity Estimation

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SCRF Annual MeetingMohammad Maysami

Tomography Problem

6

Image

Velocity estimation

Data

traveltime-slowness operator

‣ Choice of constraints

• Soft data

• Training images

• Smoothness

Inverse Problem

Velocity update

Constraints

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SCRF Annual MeetingMohammad Maysami

Magnetotellurics (MT) data

‣ Natural-source (electromagnetic method)

‣ Insight into the resistivity structure as the main parameter

• Frequency: 0.001 -1 Hz

• Insensitive to thin resistors

7

Coils Hx Hy Hz

Computer

Amplifiers,digitizers, etc.

GPS antenna

Electrodes

E-Lines Ex Ey

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SCRF Annual MeetingMohammad Maysami

Field Data

‣ 3D cube inverted resistivity

8

‣ Seismic Data

Courtesy of WesternGeco Co.

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Seismic tomography

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SCRF Annual MeetingMohammad Maysami

Tomography

‣ Relate travel times and slowness

‣ Operator is model dependent

• Initial guess s0

• Ray paths are a function of slowness

10

2 CHAPTER 1. INTRODUCTION

TOMOGRAPHY

Tomography, or at least the definition of tomography I will be using in thesis, starts from the

idea that there is an operator Tnl that relates slowness s to travel times t,

t= Tnls (1.1)

One way to think of this operator is in terms of rays. Figure 1.1 shows a simple two layered

model with sources along top and left edges and receivers along all four edges. The simplest

way to think of the operator Tnl is that it simply integrates the slowness along the raypath.

Figure 1.1: A simple example of to-

mography with the sources and re-

ceivers every .2 km in depth and ev-

ery .5 km in x. Overlaid are the ray-

paths connecting the sources to the

receivers. intro-cor.overlay [CR]

This simplistic view of tomography has a number of inconsistencies with the reflection

tomography problem. The first is that we wouldn’t be doing tomography if we actually knew

the slowness field beforehand. What we actually have is some initial guess, s0, of the slow-

ness field. If for our initial model we assume a constant slowness field and find the raypaths

connecting the same source and receivers, Figure 1.2, we encounter another problem: the ray-

paths are significantly different. An alternate way to state this observation is that the operator

is model dependent and therefore non-linear.

t = Tnl(s)

Courtesy of Bob Clapp.

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SCRF Annual MeetingMohammad Maysami

Tomography

‣ Relate travel times and slowness

‣ Operator is model dependent

• Initial guess s0

• Ray paths are a function of slowness

10

2 CHAPTER 1. INTRODUCTION

TOMOGRAPHY

Tomography, or at least the definition of tomography I will be using in thesis, starts from the

idea that there is an operator Tnl that relates slowness s to travel times t,

t= Tnls (1.1)

One way to think of this operator is in terms of rays. Figure 1.1 shows a simple two layered

model with sources along top and left edges and receivers along all four edges. The simplest

way to think of the operator Tnl is that it simply integrates the slowness along the raypath.

Figure 1.1: A simple example of to-

mography with the sources and re-

ceivers every .2 km in depth and ev-

ery .5 km in x. Overlaid are the ray-

paths connecting the sources to the

receivers. intro-cor.overlay [CR]

This simplistic view of tomography has a number of inconsistencies with the reflection

tomography problem. The first is that we wouldn’t be doing tomography if we actually knew

the slowness field beforehand. What we actually have is some initial guess, s0, of the slow-

ness field. If for our initial model we assume a constant slowness field and find the raypaths

connecting the same source and receivers, Figure 1.2, we encounter another problem: the ray-

paths are significantly different. An alternate way to state this observation is that the operator

is model dependent and therefore non-linear.

t = Tnl(s)

3

Figure 1.2: The same recording ge-

ometry as Figure 1.1, with a con-

stant velocity field. Note that the

ray paths are significantly different.

intro-init.overlay [CR]

Non-linear problems

Non-linear problems are much more difficult to solve than linear problems. A method that is

often successful is to make some approximations that will turn the non-linear problem into a

linear problem. We can make this conversion by doing a Taylor expansion (ignoring second

and higher order terms) around the initial guess at the slowness field,

t ≈ Tnls0+∇Tnl!st ≈ t0+T0!s (1.2)

!t ≈ T0!s

where s0 is the initial guess at slowness, T0 is the Frechet derivative, a linear approximation

of Tnl at s0,!s is the change in slowness, t0 are the modeled travel times by applying T0 to s0,

!t are the differences between the modeled travel times, t0, and the measured travel times, t.

Reflection seismic tomography problems are too large to do direct matrix inversion so iterative

methods, such as conjugate gradient, are used instead. Once we have used an iterative method

Courtesy of Bob Clapp.

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SCRF Annual MeetingMohammad Maysami

Linearization

‣ Linearize operator

• Using Taylor’s expansion

• Iteratively update approximation of s ➙ s0

• Linearize the operator around new s0

11

3

Figure 1.2: The same recording ge-

ometry as Figure 1.1, with a con-

stant velocity field. Note that the

ray paths are significantly different.

intro-init.overlay [CR]

Non-linear problems

Non-linear problems are much more difficult to solve than linear problems. A method that is

often successful is to make some approximations that will turn the non-linear problem into a

linear problem. We can make this conversion by doing a Taylor expansion (ignoring second

and higher order terms) around the initial guess at the slowness field,

t ≈ Tnls0+∇Tnl!st ≈ t0+T0!s (1.2)

!t ≈ T0!s

where s0 is the initial guess at slowness, T0 is the Frechet derivative, a linear approximation

of Tnl at s0,!s is the change in slowness, t0 are the modeled travel times by applying T0 to s0,

!t are the differences between the modeled travel times, t0, and the measured travel times, t.

Reflection seismic tomography problems are too large to do direct matrix inversion so iterative

methods, such as conjugate gradient, are used instead. Once we have used an iterative method

4 CHAPTER 1. INTRODUCTION

to converge to an acceptable!s, we update the slowness estimate,

s1 = s0+!s. (1.3)

We can then re-linearize around this new model (s1), constructing a new tomography operator

T1 and repeating the process.

Unfortunately, the linearization does not share many of the properties of a truly linear

problem. First, the step length calculation that is valid in the linear problem is usually not

valid in the non-linear problem. Instead, we must take into account the linearization point

when calculating the step size. Second, and more importantly, the problem isn’t guaranteed to

converge. To see why, let’s return to the simple example. The operator is based on the initial

slowness estimate, which is in error. Explained in terms of rays we are back projecting along

the guess at the ray trajectories, not their true trajectories. As a result we will end up back

projecting the slowness changes to the wrong portions of the model space.

Figure 1.3 shows the velocity estimate after applying linearized tomography. Generally,

we have moved towards the correct velocity model (Figure 1.1) but we can also see the effects

of the linear approximation. In the upper right portion of Figure 1.3 the velocity has been

incorrectly increased. If we look at the ray connecting (z = 1.6, x = 0) and (z = 0, x = 9.5) in

Figures 1.2 and 1.1 we can begin to see why. The guess at the raypath indicates that 30% of the

ray length is spent in the lower layer while in fact 50% is traveling through this high velocity

layer. To account for the traveltime discrepancy, the inversion has increased the velocity in the

in the upper portion of the model.

A second inconsistency is that equation (1.2) is an example of transmission tomography

rather than reflection tomography. Reflection tomography attempts to invert the slowness field

from raypaths that go from a known source, to a unknown reflection point in the subsurface, to

a known receiver. Not knowing the reflection point introduces a whole new set of unknowns

into the inversion. Figure 1.4 shows a synthetic anticline model. Overlaid in solid lines are the

correct reflector positions and the correct raypaths to these reflector positions. The dashed lines

are the reflector positions and raypaths that would be estimated using a s(z) initial slowness

model. Note that the guess at the reflector position is in significant error, making the guess at

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SCRF Annual MeetingMohammad Maysami

Tomography and null space

‣ shadow zones

• lack of illumination or poor illumination

(especially sub-salt regions)

‣ limited angle coverage

• imposed by recording geometry

‣ resolution decreases with depth

• velocity information is revealed with reflection angle.

‣ under-determined problem

12

9

al., 1996) or reparameterizing the model in term of spline nodes (Biondi, 1990). The lay-

ered model approach is attractive because it allows a linking between an interpreter’s geologic

model (Guiziou et al., 1996). It also provides a fairly accurate description of velocity structure

in regions such as the North Sea. The spline node approach can also be beneficial. It can guar-

antee the velocity model will be smooth (necessary for ray based methods) and with selective

placement of nodes can allow less freedom in areas where the data provides less information

about the velocity field. The downside of both of these approaches is that the parameterization

must be chosen a priori. At early iterations the guess at the velocity model can be in signif-

icant error. If we do a poor job of parameterizing the model we could actually slow, or stop,

the problem from converging (Delprat-Jannaud and Lailly, 1992).

The second option is regularization. In the regularization approach we add a second term

to the objective function,

Q(!s)= ‖!t−T0!s‖2+ ε2‖A!s‖2, (1.4)

whereA penalizes some definition of roughness in the model. The regularization approach has

its own drawbacks. The most significant is that the resulting model space may no longer has

any direct connection with geology. In addition, choosing A is problematic and can introduce

unrealistic elements into the slowness estimate.

OVERVIEW OF THESIS

The goal of this thesis is to present two different techniques that can help overcome reflection

tomography’s problems with nonlinearity and null space.

Tau tomography

In Chapter ??, I introduce the concept of tau (vertical travel-time) tomography and derive

the operator relating changes in slowness to moveout errors in tau space. I show how tau

tomography is less sensitive to the initial guess at reflector position and slowness estimate.

source receiver

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Cross-gradients function

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SCRF Annual MeetingMohammad Maysami

‣ Structural similarity measurement

‣ simplified 2-D definition

• Considering the mesh below, we can linearize the cross-gradients function

Cross-gradients function

14

!t(x, y, z) = ∇mr ×∇ms

mr : resistivity field

ms : slowness field

x

z

t ≈ 4∆x∆z

(mrc(msb −msr) + mrr(msc −msb) + mrb(msr − nsc)

)

t(x, z) =(∂mr

∂z

∂ms

∂x

)−

(∂mr

∂x

∂ms

∂z

)

Xc Xr

Xb

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SCRF Annual MeetingMohammad Maysami

Cross-gradients vs. Frequency range

‣ Accuracy for field properties in different frequency intervals:

• Difference in frequency

• Structural complexity ?

‣ Velocity vs. resistivity

• smooth velocity as resistivity

15

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SCRF Annual MeetingMohammad Maysami 16

Marmousi model

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SCRF Annual MeetingMohammad Maysami 17

Auto cross-gradient

Cross-gradient values

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SCRF Annual MeetingMohammad Maysami 18

× =

Cross-gradient values

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SCRF Annual MeetingMohammad Maysami 19

× =

Cross-gradient values

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SCRF Annual MeetingMohammad Maysami

Velocity analysis with cross-gradient constraint

‣ Velocity analysis objective function

20

TL : linear approximation of tomography matrixA : regularization operatorG : linear cross-gradients operator

g : cross-gradients functions : seismic slownessr : resistivityt : travel time

9

al., 1996) or reparameterizing the model in term of spline nodes (Biondi, 1990). The lay-

ered model approach is attractive because it allows a linking between an interpreter’s geologic

model (Guiziou et al., 1996). It also provides a fairly accurate description of velocity structure

in regions such as the North Sea. The spline node approach can also be beneficial. It can guar-

antee the velocity model will be smooth (necessary for ray based methods) and with selective

placement of nodes can allow less freedom in areas where the data provides less information

about the velocity field. The downside of both of these approaches is that the parameterization

must be chosen a priori. At early iterations the guess at the velocity model can be in signif-

icant error. If we do a poor job of parameterizing the model we could actually slow, or stop,

the problem from converging (Delprat-Jannaud and Lailly, 1992).

The second option is regularization. In the regularization approach we add a second term

to the objective function,

Q(!s)= ‖!t−T0!s‖2+ ε2‖A!s‖2, (1.4)

whereA penalizes some definition of roughness in the model. The regularization approach has

its own drawbacks. The most significant is that the resulting model space may no longer has

any direct connection with geology. In addition, choosing A is problematic and can introduce

unrealistic elements into the slowness estimate.

OVERVIEW OF THESIS

The goal of this thesis is to present two different techniques that can help overcome reflection

tomography’s problems with nonlinearity and null space.

Tau tomography

In Chapter ??, I introduce the concept of tau (vertical travel-time) tomography and derive

the operator relating changes in slowness to moveout errors in tau space. I show how tau

tomography is less sensitive to the initial guess at reflector position and slowness estimate.

P(∆s) = ||∆t−TL∆s||2 + ε21 ||A∆s||2 + ε22 ||G(s0 + ∆s)||2,

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SCRF Annual MeetingMohammad Maysami

Synthetic model with semi-circular fault

21

Velocity model

V (K

m/s

)

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SCRF Annual MeetingMohammad Maysami

Initial velocity estimation

22

Initial velocity guess

V (K

m/s

)

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SCRF Annual MeetingMohammad Maysami 23

Velocity estimation without soft data

V (K

m/s

)

Updated velocity

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SCRF Annual MeetingMohammad Maysami 24

Velocity estimation with soft data

Updated velocity with soft data

V (K

m/s

)

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SCRF Annual MeetingMohammad Maysami

Observations

‣ Steering filters

• Smooth and continuous velocity anomalies

‣ Cross-gradient functions

• Sharp boundaries

• Salt structures

• Faults

25

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Next

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SCRF Annual MeetingMohammad Maysami

Future work

‣ Improved velocity-resistivity relations

‣ Apply to field data

‣ Integrate training images as a constraint to tomography problem

‣ Integrate statistical uncertainty analysis

27

?

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SCRF Annual MeetingMohammad Maysami

Acknowledgements

• Biondo Biondi (Stanford Exploration Project)

• Tapan Mukerji (SCRF)

• Olav Lindtjorn (WesternGeco company)

• WesternGeco company

28

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Thank you