Geophysical Challenges at North Sea
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Transcript of Geophysical Challenges at North Sea
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010
Geophysical Challenges at the HP/HT Erskine Field, North Sea
Joerg Zaske, Caroline Pickles Chevron Upstream Europe
Stefano BagalaChevron Energy Technology Company
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010
Outline
Field Background
Subsurface Challenges
Geophysics
Seismic
Geomechanics
1D Model
Full Field Model
Reservoir Monitoring
4D Seismic
Microseismics
Conclusions
2
DOC ID© Chevron 2005 3
Erskine Field: Location
Located Western side of the East Central Graben, CNS.
150 miles East of Aberdeen.
300 ft Water Depth.
50% Chevron; 32% BG and 18% BP
DOC ID© Chevron 2005 4
Erskine Field Structure
Top Erskine E70 Reservoir Structure Map 2008 Interpretation, 2007 PSDM Re-processed Seismic
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6b
Machar Field boundary (above 12000’)
GW
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ine
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ck
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Machar Field boundary (above 12000’)
2STRE
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ine
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ck
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6b
Machar Field boundary (above 12000’)
GW
C
N2 kmSeveral fault blocks, formed by late Jurassic rifting.
Main Field :
Erskine & Pentland
Beta Terrace:
Erskine & Pentland
Alpha Terrace:
Heather Turbidites
Alpha Terrace
Beta Terrace
Main Field
A A’
Salt Dome
DOC ID© Chevron 2005 5
Exploration Wells
2STRE Northern Area
3RE - Main Field
19Y - Downthrown region adjacent to salt dome
Appraisal Wells
4 - Main Field
7 - Main Field
8 - Main Field
14 - Main Field
15 - Alpha Terrace
Producers
W1 - Main Field Pentland
W2 - Main Field Erskine
W3 - Main Field Erskine
W4 - Alpha Terrace Heather
W5 - Main Field Erskine
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Ersk
ine
Fiel
dP.0
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Ersk
ine
Fiel
d P.
264
Blo
ck
23/2
6b
Machar Field boundary (above 12000’)
GW
C
N2 km
-465
0
- 4650
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0
--47
50
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0
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0-4
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W1
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Ersk
ine
Fiel
dP.0
57
Ersk
ine
Fiel
d P.
264
Blo
ck
23/2
6b
Machar Field boundary (above 12000’)
2STRE
19Y
W1
W2
W3
W4
W5
8 4
3RE
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Ersk
ine
Fiel
dP.0
57
Ersk
ine
Fiel
d P.
264
Blo
ck
23/2
6b
Machar Field boundary (above 12000’)
GW
C
N2 km
2STRE
19Y
W1
W2
W4
W5
8 4
3RE
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14
W1
W2
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W5
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3RE
19Y
2STRE
Erskine Field: Wells
W3
Salt Dome
DOC ID© Chevron 2005 6
Seismic & Geoseismic section
Top Erskine
Top Pentland
B.C.U.
Base Chalk
A A’
B.C.U.
Chalk Group
Cromer Knoll Group
Heather Formation
Erskine Sands
Erskine Shale
Pentland Formation
Pre Jurassic
A A’
GWC
GWC
1.5km
Main Field Beta Terrace
Alpha Terrace
DOC ID© Chevron 2005
Erskine – Some Numbers
First HPHT field developed in CNS
Discovered 1987; Field Producing since 1998
HPHT Gas Condensate; Reservoir Temp ~175 DegC;
Initial Pressure: ~14070 PSI; Today: 2760-6380 PSI Max. Drop: ~11000 PSI
Field off plateau since approx. 2004
7
0
5,000
10,000
15,000
20,000
25,000
30,000
35,000
40,000
0
10
20
30
40
50
60
70
80
90
100
110
120
130
140
150
160
Oil
or W
ate
r R
ate
(b
bls
/d)
Gas R
ate
(m
mscf/
d)
Erskine Historical Field Performance
Field Gas Rate Field Oil Rate Field Water Rate
Pipeline failure W2 pluback to Erskine
Export pipeline to Lomond blockage due to stuck pig (outage from 30/06/07,
Field startup on 18/08/08)
W5 shut due to downhole scale buildup
W1 back online 01/05/09 after tophole
scale removal
W5 online 26/06/09 after perforating
E50/E60 dry zones
DOC ID© Chevron 2005
Erskine Field – Subsurface Challenges
Significant stress redistribution
Reservoir
Overburden
Well integrity problems
Liner deformation
Sanding Problems
Scaling Issues
Drilling into depleted reservoirs
Very difficult & very expensive (>$100MM)
8
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010 9
Liner Deformations Can we predict failures ?
2004 2005 2006
20x magnification of lateral displacementsHere at ~15600’.
Oct 04
Nov04
2010 ?
Liner Deformation vs Depletion
0
10
20
30
40
50
60
70
80
90
100
110
0 100 200 300 400 500 600 700 800
Reservoir Depletion (bar)La
tera
l Def
orm
atio
n (m
m)
Liner Failure Strain LimitUncertainty
Data Points
Goal: Predict life of existing wells & plan for replacement wells
Feed data into DA model
DOC ID© Chevron 2005 10
Where would we drill the next well ? How can Geophysics help ?
3D Seismic: Provide correct structure
4D Seismic: Identify unswept reserves
Geomechanics: Avoid areas with high drilling risk, predict well failures
Microseismic: Avoid drilling close to faults with subseismic resolution
Proposed Location
Existing Wellbore
W1
14
W4
W3
W2
84
W5
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010 11
2km Thickness
Coal Surface
Machar Salt Body
Base Chalk
Cromer Knoll Wedge
BCU
Anisotropic PSDM Reprocessing
Better velocity control away from wells
Improved imaging, better event continuity and fault definition at relatively low costs.
Vint [m/s]
Seismic Reprocessing PSDM Migration Velocities
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010 12
NS NErskine Main field
Two w
ay time (m
s)
Clearly improved imaging
Better interpretation product
Better event continuity, fault definition & signal/noise ratio.
Cromer Knoll wedges shown in green.
Excellent synthetic ties
Erskine Main Field
SErskine Main field
Two w
ay time (m
s)
AFTE R
2007 Anisotropic PSDM volume
Seismic Reprocessing Results 1989 vs 2007 comparisons
BEFOR E
N
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010 13
EDGE Extraction Pentland horizon)
Alpha Terrace
Main Field
Good imaging of main field faults.
Poorer fault definition near the salt dome due to high degree of distortion of reflectors
Suitable as input into Reservoir modelling
Interpretation
Fault Interpretation
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010
1D Geomechanical model: Drilling
14
Erskine Mud weight window. 30 deg incl
Studied sensitivity of mud weight window as a function of well inclination
Already at 30Deg inclination mud weight window closes
Collapse Gradient in undepleted shale is higher than Fracture Gradient in reservoir
Highly challenging drilling
Undepleted Shales
Depleted Sands
Pore
Pre
ssure
Fract
ure
Colla
pse
Min
. H
oriz.
Str
ess
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010 15
Pentland Mud weight window. 30 deg incl
Even worse in Pentland Reservoir.
Mud weight window closes in correspondence of several intra – reservoir shales.
Erskine Mud weight window. 30 deg incl
Pore
Pre
ssure
Fract
ure
Colla
pse
Min
. H
oriz.
Str
ess
1D Geomechanical model: Drilling
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010
1D Geomechanical Model: Sand Failure Analysis
16
Sanding
Safe
Sanding
Safe
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010
1. Build full field model to investigate production induced stresses in overburden
2. Overburden grid starts top reservoir & extends up top Chalk.
3. Assume homogeneous, uniform elastic material.
4. Use different simulation scenarios to calculate reservoir compaction (see below)
5. Reservoir compaction used to calculate overburden stresses - Nucleus-of-strain equations (Geertsma)
Full Field Geomechanical – Model
20052018 & No New Well 2018 & New Well
Input Data: Total vertical compaction based on reservoir simulation scenarios.
Overburden Model
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010 18
Full Field Geomechanics Overburden Coulomb Failure Function
Even in 2005 there are large regions predicted to slip (CFF > 0)
Slip-prone region expands due to continued reservoir depletion (e.g. 2018)
Additional well production worsens slip
Highest risk: close to major faults;
Consistent with liner deformations
2005
2018 / No New Well
2018 / With New WellExtract CFF
(Above Reservoir) New well Target
Beta Terrace
Main fieldAlpha terrace
CFF0 +100-100
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010
Reservoir Monitoring
4D Seismic
Timelapse 3D Surveys
Observe amplitude and travel time changes
Draw conclusions from changes
Microseismic
Deploy Geophones in Boreholes or Ocean-Bottom
Record “passive” Seismicity
High Potential at HPHT due to Production related stress re-distribution
19
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010
4D Seismic Monitoring (It works) Erskine 1989 vs Machar4D 2001
20
4D seismic response detected (after 3yrs production)
4D Time Effect observed
Shows connection of Beta Terrace
Would need new 4D survey to detect later production effects
Value considered small due to late stage in field life
Beta Terrace clearly Connected to Main Field
Main Field
Triassic Surface
Tim
e Shifts
[m
s]
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010
Microseismic Monitoring
Conducted Feasibility Study
Motivation
Identify 3D distribution of stress changes
Detect re-activation of major faults (seismic resolution)
Detect compaction and movements (sub-seismic faults)
Impact
Constrain Geomechanical model
Help predict well failures
Reduce drilling risks
Optimize well placement
21
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010
Microseismic Monitoring Feasibility Study
Workflow
Modelled microseismic source events
Used different layouts of Geophones
Ocean-Bottom Nodes & Borehole deployed sensors
Investigated detectability of events
Results:
Seismic signal very likely detectable.
Significantly better sensitivity for borehole deployed sensors
Deployment in production wells would be very challenging.
Comments
Value too low at stage of field life
May have been very useful early in field life, i.e. deployment in appraisal or exploration wells
Focal Mechanism based on Geomechanical Modelling
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010
ConclusionsGeophysical & Geomechanical work lead to improved understanding of subsurface
3D Reprocessing improved seismic data quality significantly.
Geomechanical modelling improved understanding of stress regime and highlights zones of increased risk for well failure. Can be used to mitigate risk and optimize well placement.
Reservoir monitoring techniques such as Seismic 4D and Microseismic monitoring applicable to Erskine and probably other HP/HT fields
Maturity of field makes it very difficult to justify any new seismic or other surveillance methods
Recommend to consider Seismic 4D & Microseismic Monitoring techniques early on in field life for other HPHT fields.
23
HPHT Wells Summit 2010, Nov 24, 2010, Aberdeen© Chevron 2010
Acknowledgements
We wish to thank our management and co- venturers BG and BP for permission to present this work.
24