modelling electromagnetic responses from seismic datamodelling electromagnetic responses from...

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Modelling electromagnetic responses from seismic data Dieter Werthmüller [[email protected]], Anton Ziolkowski, and David Wright Introduction Good estimates of background resistivit- ies are often crucial in controlled-source elec- tromagnetic (CSEM) feasibility studies and in- versions. Seismic data and well logs are of- ten available prior to CSEM acquisition, but elastic waves and electromagnetic waves share no physical parameter. Contributions We present a methodology to estimate res- istivities from seismic velocities. We apply known methods, including rock physics, depth trends, structural in- formation, and uncertainty analysis. We show an example of the methodology with data from the North Sea Harding field. Rock Physics We use a Gassmann-based relation (f G ) for the transformation from P-wave velocity v to porosity φ, and the self-similar model (f s ) for the transformation from porosity φ to resistiv- ity ρ (e.g. Carcione et al., 2007): ρ = f s (ρ s f , m) , where φ = f G (K s ,K f ,G s ,% s ,% f , κ, v ) , m is the cementation exponent, K and G are bulk and shear moduli, % is density, κ is the Krief exponent, and subscripts s and f stand for solid and fluid fraction (see Fig. 5). EM-Line b-7 a-3 b-11 b-A01 b-8 6570000 6575000 412500 417500 4 0.0 0.1 0.2 0.3 0.4 Porosity (-) 1.5 2.5 3.5 4.5 Velocity (km/s) Gassmann 10 -1 10 0 10 1 Resistivity (Ωm) self-similar 5 The transform is done in three steps: 1) Calibrate transform (incl. depth trend, box below) with a well log nearby (b-8). 2) Apply to seismic velocity in area of in- terest (including uncertainty, box left). 3) Check transform with well log in area of interest (if available). 1 10 1 2 3 Depth (km) b-8 1 10 b-7 1 10 Resistivity (Ωm) b-11 1 10 b-A01 1 10 a-3 ρ s mode ±2σ 6 Start EM-Line End 1 2 3 Depth (km) Grid Sandstone Seabed Balder Formation Base Cretaceous Background resistivity model [Mode (Ωm)] 0.4 0.7 1.3 2.3 4.1 7 1D Modelling 1200 1300 1400 1500 CMP Position 0 0.2 0.4 0.6 Depth (km) Start model ρ m (Ωm) 1 2 3 4 5 9a 1200 1300 1400 1500 CMP Position 0 0.2 0.4 0.6 Depth (km) Final model ρ m (Ωm) 9b This resistivity model (box left) has two weak- nesses: 1) anisotropy (λ = p ρ v h , ρ m = ρ v ρ h ), 2) resistivities outside well control. CSEM impulse (IR) and step (SR) responses have different sensitivities to anisotropy (Fig. 10). Only if the anisotropy factor is cor- rect, inversion of IR and SR yield the same res- ult (Fig. 11). Short offset 1D inversions of measured CSEM data, with correct aniso- tropy factor, improve the background resistivity model in the shallow section, were we have no well control (Fig. 9); the resulting resistivities are in this case lower. 0.0 0.5 1.0 1.5 2.0 2.5 Time (s) 0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 Amplitude (Ω/(m 2 s)) ×10 -10 ρ m = 1.0 ρ m = 2.0 ρ m = 3.0 λ = 1.0 λ = 1.5 λ = 2.0 10a 0.0 0.5 1.0 1.5 2.0 2.5 Time (s) 0 1 2 3 4 5 6 7 Amplitude (Ω/m 2 ) ×10 -11 10b 1.0 1.5 2.0 2.5 Anisotropy (-) 0 2 4 6 8 10 NRMSD (%) NRMSD IR NRMSD SR Model (SR - IR) 0 2 4 6 8 10 Δ Model IR-SR (Ωm) 11 Uncertainty Analysis 0.4 0.6 0.8 1.0 2 6 10 14 Prob. density (-) Parameter 0.4 0.6 0.8 1.0 Resistivity (Ωm) Model 0.4 0.6 0.8 1.0 2 6 10 14 Prob. density (-) Parameter & Model 1a 1b 1c 2 Data, rock physics model, and rock phys- ics parameter have errors. Chen and Dick- ens (2009) describe a methodology to account for the uncertainties related to rock physics parameters and the rock physics model it- self. They describe the rock physics model as gamma distribution in a Bayesian frame- work, with a defined error E , and the rock physics parameters as distributions, f (ρ|θ )= β α x α-1 Γ(α) exp (-βx) , where θ is a vector containing all model para- meter distributions, α =1/E 2 , and β =(α - 1)rp . Here, ρ rp is one realization of the rock physics model with a random set of model para- meters. We define the distribution of the velo- city from the data themselves (see Fig. 2). The distribution is defined as the difference between the measured log values and the val- ues of the smoothed log, v (z ) - v s (z ). This yields resistivity as a probability density function, instead of a deterministic resistivity value (Fig. 3c). 1 10 Resistivity (Ωm) 0.6 1.0 1.4 1.8 Depth (km) Grid Sandstone ρ s mode ±σ ±2σ 3a v f 2.0 3.0 4.0 v s Velocity (km/s) ρ f 1 10 ρ s Resistivity (Ωm) deterministic 0.6 0.8 1.0 1.2 Resistivity (Ωm) 1 3 5 Prob. density (-) 3b 3c Depth Trend Rock parameters are a function of, e.g., litho- logy and depth. We include the following dependences in our model: Depth: K s ,G s , κ, ρ s Temperature: ρ f Porosity : m Lithology: Grid Sandstones (delineated with seismic horizons) 1 10 Resistivity (Ωm) ρ ρ s ρ(φ[v ]) 2 3 4 Vel. (km/s) 0.6 1.0 1.4 1.8 Depth (km) v v s 10 30 (GPa) K s G s 1 10 (GPa) ρ f ρ s 2 3 (-) m κ Grid Sandstone 8 Acknowledgment We thank PGS for funding the research and the Harding partners, BP and Maersk, for per- mission to use the data. References Carcione, J. M., B. Ursin, and J. I. Nordskag, 2007, Cross-property relations between electrical conductivity and the seismic velocity of rocks: Geophysics, 72, E193–E204, doi: 10.1190/1.2762224. Chen, J., and T. A. Dickens, 2009, Effects of uncertainty in rock-physics models on reservoir parameter estimation using seismic amplitude variation with angle and controlled-source electromagnetics data: Geophysical Prospecting, 57, 61–74, doi: 10.1111/j.1365-2478.2008.00721.x. Werthmüller, D., A. Ziolkowski, and D. Wright, 2012, Background resistivity model from seismic velocities: SEG Technical Program Expanded Abstracts, 31, doi: 10.1190/segam2012-0696.1. Conclusions This method yields the range of back- ground resistivity models, consistent with the known seismic velocities. This model provides an additional data set, which can be used for integrated ana- lysis, or as a starting point for a detailed CSEM feasibility study or inversion. We will use this background resistivity model for 3D CSEM modelling for comparison with measured data.

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Page 1: Modelling electromagnetic responses from seismic dataModelling electromagnetic responses from seismic data Dieter Werthmüller [Dieter.Werthmuller@ed.ac.uk], ... 2 :5 3 :5 4 :5 Velocity

Modelling electromagnetic responses from seismic dataDieter Werthmüller [[email protected]], Anton Ziolkowski, and David Wright

IntroductionGood estimates of background resistivit-ies are often crucial in controlled-source elec-tromagnetic (CSEM) feasibility studies and in-versions. Seismic data and well logs are of-ten available prior to CSEM acquisition, butelastic waves and electromagnetic wavesshare no physical parameter.

Contributions• We present a methodology to estimate res-istivities from seismic velocities.

• We apply known methods, including rockphysics, depth trends, structural in-formation, and uncertainty analysis.

• We show an example of the methodologywith data from the North Sea Harding field.

Rock PhysicsWe use a Gassmann-based relation (fG) forthe transformation from P-wave velocity v toporosity φ, and the self-similar model (fs) forthe transformation from porosity φ to resistiv-ity ρ (e.g. Carcione et al., 2007):

ρ = fs(ρs, ρf,m, φ) , where

φ = fG(Ks,Kf, Gs, %s, %f, κ, v) ,

m is the cementation exponent, K and G arebulk and shear moduli, % is density, κ is theKrief exponent, and subscripts s and f standfor solid and fluid fraction (see Fig. 5).

EM-Line

b-7a-3

b-11

b-A01

b-86570000

6575000

412500

417500

4

0.0 0.1 0.2 0.3 0.4

Porosity (-)

1.5

2.5

3.5

4.5

Vel

oci

ty(k

m/s)

Gassmann

10−1

100

101

Res

isti

vit

y(Ω

m)

self-similar

5

The transform is done in three steps:1) Calibrate transform (incl. depth trend,box below) with a well log nearby (b-8).2) Apply to seismic velocity in area of in-terest (including uncertainty, box left).3) Check transform with well log in area ofinterest (if available).

1 10

1

2

3

Dep

th(k

m)

b-8

1 10

b-7

1 10

Resistivity (Ωm)

b-11

1 10

b-A01

1 10

a-3

ρs

mode

±2σ

6

Start – EM-Line – End

1

2

3

Dep

th(k

m)

Grid Sandstone

Seabed

Balder Formation

Base Cretaceous

Background resistivity model [Mode (Ωm)]

0.4

0.7

1.3

2.3

4.17

1D Modelling

1200 1300 1400 1500CMP Position

0

0.2

0.4

0.6Dep

th(k

m)

Start model ρm (Ωm)

1

2

3

4

59a

1200 1300 1400 1500CMP Position

0

0.2

0.4

0.6 Dep

th(k

m)

Final model ρm (Ωm)9b

This resistivity model (box left) has two weak-nesses:1) anisotropy (λ =

√ρv/ρh, ρm =

√ρvρh),

2) resistivities outside well control.CSEM impulse (IR) and step (SR) responseshave different sensitivities to anisotropy(Fig. 10). Only if the anisotropy factor is cor-

rect, inversion of IR and SR yield the same res-ult (Fig. 11). Short offset 1D inversions ofmeasured CSEM data, with correct aniso-tropy factor, improve the background resistivitymodel in the shallow section, were we have nowell control (Fig. 9); the resulting resistivitiesare in this case lower.

0.0 0.5 1.0 1.5 2.0 2.5

Time (s)

0.0

0.2

0.4

0.6

0.8

1.0

1.2

1.4

Am

pli

tud

e(Ω/(m

2s)

)

×10−10

ρm = 1.0

ρm = 2.0

ρm = 3.0

λ = 1.0

λ = 1.5

λ = 2.0

10a

0.0 0.5 1.0 1.5 2.0 2.5

Time (s)

0

1

2

3

4

5

6

7

Am

plitu

de

(Ω/m

2)

×10−11

10b

1.0 1.5 2.0 2.5

Anisotropy (−)

0

2

4

6

8

10

NR

MSD

(%)

NRMSD IR

NRMSD SR

Model (SR - IR)

0

2

4

6

8

10

∆M

odel

IR-S

R(Ω

m)

11

Uncertainty Analysis

0.4 0.6 0.8 1.0

2

6

10

14

Pro

b.

den

sity

(-) Parameter

0.4 0.6 0.8 1.0

Resistivity (Ωm)

Model

0.4 0.6 0.8 1.0

2

6

10

14

Pro

b.

den

sity

(-)Parameter & Model

1a 1b 1c

-1 0 1∆v : v(z)−vs (z)

pdf

data

0

1

2

3

4

5

Pro

b.

den

sity

(-)

2 3 4Vel. (km/s)

0.6

1.0

1.4

1.8D

ep

th (

km

)

v

vs

2

Data, rock physics model, and rock phys-ics parameter have errors. Chen and Dick-ens (2009) describe a methodology to accountfor the uncertainties related to rock physicsparameters and the rock physics model it-self. They describe the rock physics model asgamma distribution in a Bayesian frame-work, with a defined error E, and the rockphysics parameters as distributions,

f(ρ|θ) =βαxα−1

Γ(α)exp (−βx) ,

where θ is a vector containing all model para-meter distributions, α = 1/E2, and β = (α −1)/ρrp. Here, ρrp is one realization of the rockphysics model with a random set of model para-meters.

We define the distribution of the velo-city from the data themselves (see Fig. 2).The distribution is defined as the differencebetween the measured log values and the val-ues of the smoothed log, v(z) − vs(z). Thisyields resistivity as a probability densityfunction, instead of a deterministic resistivityvalue (Fig. 3c).

1 10

Resistivity (Ωm)

0.6

1.0

1.4

1.8

Dep

th(k

m)

Grid Sandstone

ρs

mode

±σ±2σ3a

vf 2.0 3.0 4.0 vs

Velocity (km/s)

ρf

1

10

ρs

Res

isti

vit

y(Ω

m) deterministic

0.6 0.8 1.0 1.2

Resistivity (Ωm)

1

3

5

Pro

b.

den

sity

(-)

3b

3c

Depth TrendRock parameters are a function of, e.g., litho-logy and depth. We include the followingdependences in our model:• Depth: Ks, Gs, κ, ρs

• Temperature: ρf• Porosity: m• Lithology: Grid Sandstones(delineated with seismic horizons)

1 10

Resistivity (Ωm)

ρ

ρs

ρ(φ[v])

2 3 4

Vel. (km/s)

0.6

1.0

1.4

1.8

Dep

th(k

m)

v

vs

10 30

(GPa)

Ks

Gs

1 10

(GPa)

ρf

ρs

2 3

(-)

m

κ

Grid Sandstone

8

AcknowledgmentWe thank PGS for funding the research andthe Harding partners, BP and Maersk, for per-mission to use the data.

ReferencesCarcione, J. M., B. Ursin, and J. I. Nordskag, 2007, Cross-property

relations between electrical conductivity and the seismic velocityof rocks: Geophysics, 72, E193–E204, doi: 10.1190/1.2762224.

Chen, J., and T. A. Dickens, 2009, Effects of uncertainty inrock-physics models on reservoir parameter estimation usingseismic amplitude variation with angle and controlled-sourceelectromagnetics data: Geophysical Prospecting, 57, 61–74,doi: 10.1111/j.1365-2478.2008.00721.x.

Werthmüller, D., A. Ziolkowski, and D. Wright, 2012, Backgroundresistivity model from seismic velocities: SEG Technical ProgramExpanded Abstracts, 31, doi: 10.1190/segam2012-0696.1.

Conclusions• This method yields the range of back-ground resistivity models, consistentwith the known seismic velocities.• This model provides an additional dataset, which can be used for integrated ana-lysis, or as a starting point for a detailedCSEM feasibility study or inversion.• We will use this background resistivity model

for 3D CSEM modelling for comparison withmeasured data.