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Page 1: PS, SSP, PSPI, FFD

PS, SSP, PSPI, FFDPS, SSP, PSPI, FFDSSPSSP

FFDFFD

KMKM

PSPIPSPI

Page 2: PS, SSP, PSPI, FFD

k

k z

x

k = k 1 – k z

2

k 2x ~ k (1 – k + ..)

2x

k 22

P(x,z,) = P(x,0 ,) e zik(x) z

Page 3: PS, SSP, PSPI, FFD

PS, SSP, PSPI, FFDPS, SSP, PSPI, FFDk = k 1 – k z

2

k 2x

-1 1.2

1

k z ~ k(1 – k ) 2x

k 22

k z ~ k (1 – .43 ) 2

21 -.5

= k 2x

k 2

P(x,z,) = P(x,0 ,) e zik(x)z

k

k

x

z

Page 4: PS, SSP, PSPI, FFD

SSP MigrationSSP Migration

k = k(x) 1 – k z

2

k(x)2x = k 1 – k

2

k 2x - k

0

0

Thin lens

P(x,z,) = P(x,0 ,) e zik(x)z

Page 5: PS, SSP, PSPI, FFD

FFD MigrationFFD Migration

k = k(x) 1 – k z

2

k(x)2x = k 1 – k

2

k 2x - k

0

0

Thin lens

P(x,z,) = P(x,0 ,) e zik(x)z

Page 6: PS, SSP, PSPI, FFD

k = k(x) 1 – k z

2

k(x)2x = k 1 – k

2

k 2x - k

0

0

Thin lens

FFD MigrationFFD MigrationP(x,z,) = P(x,0 ,) e zik(x)z

Page 7: PS, SSP, PSPI, FFD

FFD MigrationFFD MigrationP(x,z,) = P(x,0 ,) e zik(x)z

Page 8: PS, SSP, PSPI, FFD

FFD MigrationFFD Migrationother term

P(x,z,) = P(x,0 ,) e zik(x)z

Page 9: PS, SSP, PSPI, FFD

FFD MigrationFFD Migration

PDE associated withother term

other term

Rearrange PDE

P(x,z,) = P(x,0 ,) e zik(x)z

Page 10: PS, SSP, PSPI, FFD

FFD MigrationFFD Migration

Substitute FD approximations into above

P(x,z,) = P(x,0 ,) e zik(x)z

Page 11: PS, SSP, PSPI, FFD

FFD MigrationFFD Migration

Substitute FD approximations into above

P(x,z,) = P(x,0 ,) e zik(x)z

Page 12: PS, SSP, PSPI, FFD

FFD MigrationFFD Migration

k = k(x) 1 – k z

2

k(x)2x = k 1 – k

2

k 2x - k

0

0

Thin lens

P(x,z,) = P(x,0 ,) e zik(x)z

Page 13: PS, SSP, PSPI, FFD

PS, SSP, PSPI, FFDPS, SSP, PSPI, FFD

Page 14: PS, SSP, PSPI, FFD

PS, SSP, PSPI, FFDPS, SSP, PSPI, FFD

Page 15: PS, SSP, PSPI, FFD

SummarySummaryCost:Cost:

Accuracy:Accuracy: KMKM SSPSSP

PSPIPSPI FFDFFD

Page 16: PS, SSP, PSPI, FFD

Course SummaryCourse Summary

m(x)= (g,s,x) G(g|x)d(g|x)G(x|s)dgdsg,s,

G(g|x) = G(g|x) + G(g|x) d(g|x) = d(g|x) + d(x|g)

G(g|x) = G(g|x) d(g|x) = d(g|x)

Filter

RTM

Asymptotic G

KM Phase Shift Beam

1-way G Asymptotic G+ Fresnel Zone

Page 17: PS, SSP, PSPI, FFD

1980

Multisource SeismicMultisource SeismicImagingImaging

vs

copper

VLIW

Superscalar

RISC

1970 1990 2010

1

100

100000

10

1000

10000

Aluminum

Year

202020001980

CPU Speed vs Year

Page 18: PS, SSP, PSPI, FFD

OUTLINEOUTLINE

Theory ITheory I

Theory IITheory II

Numerical ResultsNumerical Results

Page 19: PS, SSP, PSPI, FFD

RTM Problem & Possible Soln.RTM Problem & Possible Soln.

• Problem:Problem: RTM computationally costly RTM computationally costly

• Solution:Solution: Multisource LSM RTM Multisource LSM RTM

1919

Preconditioning speeds up by factor 2-3Preconditioning speeds up by factor 2-3

LSM reduces crosstalkLSM reduces crosstalk

5

Page 20: PS, SSP, PSPI, FFD

Multisource Migration:Multisource Migration: mmmigmig=L=LTTdd

Forward Model:Forward Model:

Multisource Least Squares Migration Multisource Least Squares Migration

d +d +dd =[ =[L +L +LL ]m ]m11 222211

LL{dd{

=[=[L +L +LL ]( ](dd + + dd ) ) 11 222211

TT TT

= = L d +L d +L dL d + + 11 222211

TT TT

LL dd + +L L dd22 112211

Crosstalk noiseCrosstalk noiseStandard migrationStandard migration

TT TT

Page 21: PS, SSP, PSPI, FFD

Multisource Least Squares Phase-encoded Multisource Least Squares Phase-encoded Migration Migration

=[=[NN L +L +N LN L ](N ](N dd + + NN dd ) ) 11 222211 22 221111

mmmigmig

==N*NN*N L d +L d +N*N L dN*N L d + N* + N*NN L L dd + + N*N*NN L L dd 11 2211 22 221111 11 11 11 22 1122 22 22 22

TT TT

TT TT TT TT

** **

= = L d +L d + L d L d11 11 22 22

Standard migrationStandard migration

If <N N > = If <N N > = (i-j)(i-j)i j

Crosstalk noiseCrosstalk noise

Orthogonal phase encoding s.t. <Orthogonal phase encoding s.t. <N* N* N >=0N >=01 1 22

Page 22: PS, SSP, PSPI, FFD

Key AssumptionKey Assumption

d(t) =d(t) =

Zero-mean white noise: <N(t)>=0; <N(t) N(t’) >=0

++ M= Stack Number

Am

plit

ude

k=1k=1

MM

N(t )N(t )(k)(k)

<N(t)> ~<N(t)> ~

k=1k=1

MM

[ S(t) ][ S(t) ]22

M1

SNR SNR

M

M vs M

k=1k=1

MM

[ N(t) ][ N(t) ]22

~

(k)(k)

(k)(k)

[ S(t) ][ S(t) ]22

k=1k=1

MM

[ N(t) ][ N(t) ]22 22

~(k)(k)

MM22

[ S(t) ][ S(t) ]22

~MM

22

M M

k=1k=1

MM

[S(t) +N(t) ][S(t) +N(t) ]

Page 23: PS, SSP, PSPI, FFD

Multisource S/N RatioMultisource S/N Ratio

# geophones/CSG# geophones/CSG

# CSGs# CSGs

L [d + d +.. ]1 221

d +d T d , d 2211

L [d + d + … ]1 2

T , …. +….

Page 24: PS, SSP, PSPI, FFD

Multisrc. Migration vs Standard Migration

# iterations# iterations

Iterative Multisrc. Migration vs Standard Migration

vs

vs

MSMSS-1

M~~

# geophones/CSG# geophones/CSG # CSGs# CSGs

MSMI

Page 25: PS, SSP, PSPI, FFD

SummarySummary

Time Statics

Time+Amplitude Statics

QM Statics

1. Multisource crosstalk term analyzed analytically1. Multisource crosstalk term analyzed analytically

2. Crosstalk decreases with increasing 2. Crosstalk decreases with increasing , randomness, , randomness, dimension, iteration #, and decreasing depthdimension, iteration #, and decreasing depth

3. Crosstalk decrease can now be tuned3. Crosstalk decrease can now be tuned

4. Some detailed analysis and testing needed to refine 4. Some detailed analysis and testing needed to refine predictions.predictions.

LL dd + +L L dd22 112211

TT TT

Page 26: PS, SSP, PSPI, FFD

OUTLINEOUTLINE

Theory ITheory I

Theory IITheory II

Numerical ResultsNumerical Results

Page 27: PS, SSP, PSPI, FFD

0Z

k(m

)3

0 X (km) 16

The Marmousi2 Model

The area in the white box is used for S/N calculation.

Page 28: PS, SSP, PSPI, FFD

0 X (km) 16

0Z

k(m

)3

0Z

(k

m)

3

0 X (km) 16

Conventional Source: KM vs LSM (50 iterations)

Page 29: PS, SSP, PSPI, FFD

0 X (km) 16

0Z

k(m

)3

0Z

(k

m)

3

0 X (km) 16

200-source Supergather: KM vs LSM (300 its.)

Page 30: PS, SSP, PSPI, FFD

S/N

0

1 Number of Iterations 300

S/N =7

The S/N of MLSM image grows as the square root of the number of iterations.

I

Page 31: PS, SSP, PSPI, FFD

• Fast Multisource Least Squares Fast Multisource Least Squares Phase Shift.Phase Shift.

• Multisource Waveform Inversion (Ge Zhan)Multisource Waveform Inversion (Ge Zhan)

• Theory of Crosstalk Noise (Schuster)Theory of Crosstalk Noise (Schuster)

8

Multisource TechnologyMultisource Technology

Page 32: PS, SSP, PSPI, FFD

The True Model

• use constant velocity model with c = 2.67 km/s

• center frequency of source wavelet f = 20 Hz

X (km)

Z (

km)

Reflectivity, SEG/EAGE Salt Model

0 1 2 3 4 5

0

0.2

0.4

0.6

0.8

1

1.2

Page 33: PS, SSP, PSPI, FFD

Multi-source PSLSM

X (km)

Z (k

m)

Reflectivity, Ten 10-source supergathers

0 1 2 3 4 5

0

0.2

0.4

0.6

0.8

1

1.2

• 645 receivers and 100 sources, equally spaced 10 sets of sources, staggered; each set constitutes a supergather

• 50 iterations of steepest descent

Page 34: PS, SSP, PSPI, FFD

Single-source PSLSM

• 645 receivers and 100 sources, equally spaced 100 individual shots

• 50 iterations of steepest descent

X (km)

Z (k

m)

Reflectivity, 100 single source gathers

0 1 2 3 4 5

0

0.2

0.4

0.6

0.8

1

1.2

Page 35: PS, SSP, PSPI, FFD

Multi-Source Waveform Inversion StrategyMulti-Source Waveform Inversion Strategy(Ge Zhan) (Ge Zhan)

Generate multisource field data with known time shift

Generate synthetic multisource data with known time shift from estimated

velocity model

Multisource deblurring filter

Using multiscale, multisource CG to update the velocity model with

regularization

Initial velocity model

144 shot gathers144 shot gathers

Page 36: PS, SSP, PSPI, FFD

3D SEG Overthrust Model(1089 CSGs)

15 km

3.5 km

15 km

Page 37: PS, SSP, PSPI, FFD

3.5 km

Dynamic QMC TomogramDynamic QMC Tomogram (99 CSGs/supergather)(99 CSGs/supergather)

Static QMC TomogramStatic QMC Tomogram(99 CSGs/supergather)(99 CSGs/supergather)

15 km

Dynamic Polarity TomogramDynamic Polarity Tomogram(1089 CSGs/supergather)(1089 CSGs/supergather)

Numerical ResultsNumerical Results

Page 38: PS, SSP, PSPI, FFD

OUTLINEOUTLINE

Theory ITheory I

Theory IITheory II

Numerical ResultsNumerical Results

Page 39: PS, SSP, PSPI, FFD

Multisource Least Squares Migration Multisource Least Squares Migration Crosstalk term

Time Statics

Time+Amplitude Statics

QM Statics

36

Page 40: PS, SSP, PSPI, FFD

SummarySummaryCrosstalk term

Time Statics

Time+Amplitude Statics

QM Statics

1. Multisource crosstalk term analyzed analytically1. Multisource crosstalk term analyzed analytically

2. Crosstalk decreases with increasing 2. Crosstalk decreases with increasing , randomness, , randomness, dimension, and decreasing depthdimension, and decreasing depth

3. Crosstalk decrease can now be tuned3. Crosstalk decrease can now be tuned

4. Some detailed analysis and testing needed to refine 4. Some detailed analysis and testing needed to refine predictions.predictions.

37

Page 41: PS, SSP, PSPI, FFD

Multisource Migration:Multisource Migration: mmmigmig=L=LTTdd

Forward Model:Forward Model:

Multisource Least Squares Migration Multisource Least Squares Migration

d +d =[d +d =[L +L ]mL +L ]m11 222211

LL{dd{Standard migration

Crosstalk term

Phase encodingPhase encoding

Kirchhoff kernelKirchhoff kernel

34

Page 42: PS, SSP, PSPI, FFD

Multisource Least Squares Migration Multisource Least Squares Migration Crosstalk term

35

Page 43: PS, SSP, PSPI, FFD

Multisource Least Squares Migration Multisource Least Squares Migration Crosstalk term

Time Statics

Time+Amplitude Statics

QM Statics

36

Page 44: PS, SSP, PSPI, FFD

Crosstalk TermCrosstalk Term

Time Statics

Time+Amplitude Statics

QM Statics

LL dd + +L L dd22 112211

TT TT

Page 45: PS, SSP, PSPI, FFD

SummarySummaryCrosstalk term

Time Statics

Time+Amplitude Statics

QM Statics

1. Multisource crosstalk term analyzed analytically1. Multisource crosstalk term analyzed analytically

2. Crosstalk decreases with increasing 2. Crosstalk decreases with increasing , randomness, , randomness, dimension, and decreasing depthdimension, and decreasing depth

3. Crosstalk decrease can now be tuned3. Crosstalk decrease can now be tuned

4. Some detailed analysis and testing needed to refine 4. Some detailed analysis and testing needed to refine predictions.predictions.

37

Page 46: PS, SSP, PSPI, FFD

Multisource FWI SummaryMultisource FWI Summary(We need faster migration algorithms & better velocity models)(We need faster migration algorithms & better velocity models)

IO 1 vs 1/20

Cost 1 vs 1/20 or better

Resolution dx 1 vs 1

Sig/MultsSig ?

Stnd. FWI Multsrc. FWIStnd. FWI Multsrc. FWI

Page 47: PS, SSP, PSPI, FFD

Key AssumptionKey Assumption

<d(t)>= <S(t)> + <N(t)><d(t)>= <S(t)> + <N(t)>

Zero-mean white noise: <N>=0; <N N >=0i j

++ n= Stack Number

Am

plit

ude

<N(t)> ~ <N(t)> ~ 22 n <S(t)> ~ <S(t)> ~

22 n 22

k=1k=1

nn

N(t )N(t )(k)(k)

<N(t)> ~<N(t)> ~1/n

<N(t) > ~<N(t) > ~ 22

k=1k=1

nn

[ N(t ) ][ N(t ) ](k)(k) 22

1/n

<N(t) > ~<N(t) > ~ 22

k=1k=1

nn

[ N(t ) ][ N(t ) ](k)(k) 22

1/n


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