Pcube+ - high resolution horizon update by prestack inversion · Pcube . Gas Gas sand Brine...
Transcript of Pcube+ - high resolution horizon update by prestack inversion · Pcube . Gas Gas sand Brine...
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Pcube+ - high resolution horizon update by prestack inversion Øyvind M. Skjæveland and Richard William Metcalfe, Statoil. Odd Kolbjørnsen, Lundin (formerly NR). Per Røe and Ragnar Hauge, Norwegian Computing Centre (NR).
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Outline
• Motivation
• Simplified example – thin gas sand – achieving a detailed interpretation
− Classical detuning
− Rock physics inversion walk-through
• Real case with several layers in tuning (Statfjord East flank)
• Concluding remarks
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Horizon interpretation - customary practice:
Pick one substack.
Interpret horizons in max peak and max trough.
Thin layers - tuning and AVO issues:
Real layer boundaries not in max peak or max trough
Amplitudes and AVO carry information – not used.
Horizons update by prestack inversion:
Using rock physics knowlegde.
Moving horizons away from peaks and troughs.
Quantifying the uncertainty.
Resulting in:
Better volumetrics.
More accurate well placement.
Better understanding of uncertainty.
Horizon consistency check by prestack data.
Motivation – horizon update by inversion Horizons are widely used
• Volumetrics
• Well prognoses
• Geomodels
One of the most important
deliveries from geophysics.
Vp/V
s
AI
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Simple case - Thin gas sand in tuning How to achieve a more detailed horizon placement
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Well
gas
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Below 0 and λ/2 the amplitude is affected by thickness
Well
position
Input horizons
Output horizons
True thick.
= f(amp, int.thick.)
The quick and easy way – detuning
Int.thick. True thick.
amp
True thickness
Knowledge of properties and assumption of blocky sand
enables detailed horizon prediction below tuning thickness
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Simple case - Rock physics inversion AI and near stack only. 3 possible Lithology fluid classes (LFC’s)
6
4ms
LFC
grid
Elastic
properties and
wavelet known
from well.
Young shale
AI = 8000
Old shale
AI = 8000
Gas sand
AI = 5000
wavelet
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Model 1 – very poor match
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AI
Synthetic
Young shale
AI = 8000
Old shale
AI = 8000
Gas sand
AI = 5000
wavelet
LFC
configuration
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Model 2 – very poor match
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AI
Synthetic
Young shale
AI = 8000
Old shale
AI = 8000
Gas sand
AI = 5000
wavelet
LFC
configuration
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Model 3 poor match
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AI
Synthetic
Young shale
AI = 8000
Old shale
AI = 8000
Gas sand
AI = 5000
wavelet
LFC
configuration
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Model 4 good match
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AI
Synthetic
Young shale
AI = 8000
Old shale
AI = 8000
Gas sand
AI = 5000
wavelet
LFC
configuration
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Some good-match models P(y.s) P(o.s.)
Young shale
AI = 8000
Old shale
AI = 8000
Gas sand
AI = 5000
wavelet
Probability: match-weighted sum of all models
P(gas)
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Probability: match-weighted sum of all models
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Some good-match models P(all)
Young shale
AI = 8000
Old shale
AI = 8000
Gas sand
AI = 5000
wavelet
Buland et al 2008
Pcube
0.3 0.4 0.3
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Old shale
over
young shale
Old shale
over
gas sand
Gas sand
over
young shale
Extra:
Illegal
combinations
Young shale
AI = 8000
Old shale
AI = 8000
Gas sand
AI = 5000
wavelet
Probability: match-weighted sum of all models
Some good-match models P(all)
Buland et al 2008
Pcube
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Young shale
AI = 8000
Old shale
AI = 8000
Gas sand
AI = 5000
wavelet
Old shale
over
young shale
Old shale
over
gas sand
Gas sand
over
young shale
Illegal
combinations
Probability: match-weighted sum of all legal models
Pcube+
Illegal combinations
impose blocky sand
Buland et al 2008
Pcube
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Gas
sand
Brine
sand
Zone 1
Zone 2
Zone 3
Actual setup – prestack case
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Smoothed model
=Prior model
Inversion
result
wavelets
AI
Vp/V
s
AI
Angle stacks
Old
shale
Young
shale
Gas
sand
Concept
Input horizons Inp
ut
ho
rizo
n u
nce
rtain
ty
Output horizons
w/uncertainty
Inve
rsio
n
Illegal
combinations
-per zone
Knowledge of properties and assumption of blocky sand
enables detailed horizon prediction below tuning thickness
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Statfjord East flank
Brent Gp.
Statfjord Fm.
Dunlin Gp.
East flank
slump block C
SFC
SFB
SFA
Prod. start
1979
300+ wells
Partners:
Statoil
Centrica
ExxonMobil
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Draupne
Mime
Cook/Amundsen
shale
Shetland
Sand
Drake/Burton
shale
AI
Vp/v
s
LFC properties
Shetland
Mime
Draupne
Reworked Brent
Intra-reservoir Dunlin
Isolated Brent
Dunlin Group
BCU
TIB
BCU + 35ms
TIB + 30ms
(BIB)
BCU – 5 ms
BCU + 10ms
Statfjord – model setup
BCU
T IB
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Shetland
Mime
Draupne
Reworked Brent
Intra-reservoir Dunlin
Isolated Brent
Dunlin Group
BCU
TIB
BCU + 35ms
TIB + 30ms
(BIB)
BCU – 5 ms
BCU + 10ms
Statfjord – model setup
Seismic section with interpretation
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Shetland
Mime
Draupne
Reworked Brent
Intra-reservoir Dunlin
Isolated Brent
Dunlin Group
BCU
TIB
BCU + 35ms
TIB + 30ms
(BIB)
BCU – 5 ms
BCU + 10ms
Seismic section with interpretation
and slave horizons
Statfjord – model setup – slave horizons
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Shetland
Mime
Draupne
Reworked Brent
Intra-reservoir Dunlin
Isolated Brent
Dunlin Group
BCU
TIB
BCU + 35ms
TIB + 30ms
(BIB)
BCU – 5 ms
BCU + 10ms
Seismic section with interpretation
and sand concept model
Statfjord – model setup – slave horizons
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Shetland
Isolated Brent
Dunlin Group
Shetland
Mime
Draupne
Reworked Brent
Intra-reservoir Dunlin
Isolated Brent
Dunlin Group
BCU
TIB
BCU + 35ms
TIB + 30ms
(BIB)
BCU – 5 ms
BCU + 10ms
BCU ± 10ms
TIB ± 25ms
BIB ± 25ms
Sand smoothed model section
= prior distribution for sand
Probability 0 1
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Statfjord – model setup – sand prior section
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BCU ± 10ms
TIB ± 25ms
BIB ± 25ms
Sand smoothed model section
= prior distribution for sand
Probability 0 1
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Statfjord – model setup – sand prior section
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BCU ± 4ms
TIB ± 11ms
BIB ± 8ms
Posterieor
uncertainty
(2σ ≈ P(95))
Sand inversion result section
= posterior distribution for sand
Probability 0 1
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Statfjord – model setup – sand post. section
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Inversion process – one trace
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Isolated Brent
TIB ± 11ms
TIB
Deterministic
model
TIB ± 25ms
Human estimate
of uncertainty
Updated to match
prestack data
inversion
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near, input horizons
far, input and slave horizons
sand prior model, input horizons
sand posterior, output horizons
far, output horizons
A B C
A B C
A B C
A B C
A B C
A B C
Input data, sand probability and horizons
25 m
i
Mid stack also used as input but not shown
Probability 0 1
Concept model from horizons
250m Probability 0 1
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A
B
C
Input (prior
expected
isochrone)
(constant 30ms) A B C
A B C
Isochrone Isolated Brent sand
A
B
C
Output
(posterior
expected
isochrone)
0 65 Isolated Brent thickness, ms
40 20
sand prior model, input horizons
sand posterior, output horizons
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500m
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0 65 Isolated Brent thickness, ms
40 20
A
B
C
A
B
C
A B C
Isochrone prediction vs well result
0 50 Intra-Reservoir Dunlin thickness, ms
30 20 10 40
Formation TVT est.
pre-inv (m)
TVT est.
post-inv(m)
TVT well
obs. (m)
Mime 3 4 4
Draupne 9 10 12
Reworked
Brent
20 18 8
Intra-res
Dunlin
17 7 7
Isolated
Brent
36 58 55
Intra-reservoir
Dunlin shale
expected
thickness
Isolated Brent
sand
expected
thickness
Well B result (Jan 2016)
27
500m
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A
B
C
A
B
C
A
B
C
Mean
(P50)
Maximum
(P10)
Minimum
(P90)
Isochrone Isolated Brent sand - uncertainty
0 65 Isolated Brent thickness, ms
40 20 28
500m
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Concluding remarks
• Working with sand probability and uncertain horizons as input and output:
− Facilitates integration of geoscience.
− Easy to relate to for all disciplines compared to AI and vp/vs input/output
• Accurate horizon placement - below tuning, away from peak and trough is valuable
− Horizons with uncertainty are often what we want
− Volumetrics, well planning, geomodels, instant isochrones
• Constraining the inversion is key to achieving sub-tuning detail
− Limited number of lithologies – limited combinations of vp,vs,ρ allowed
− Limiting where the lithologies can be – based on geological input
− Excluding non-geological and non-physical layering (e.g. brine just above gas)
• Making amplitudes move horizons is making amplitudes matter.
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Thanks
• to the Statfjord partnership for the permission to show the Statfjord results.
• to co-authors for
− doing the Statfjord work (Richard)
− developing the technique and setting up a JIP to take it further (NR)
• to you for listening
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