Development of a 1,000 Level 3C Fiber Optic Borehole ... · •Goals: Design, build, and test a...
Transcript of Development of a 1,000 Level 3C Fiber Optic Borehole ... · •Goals: Design, build, and test a...
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© 2012 Paulsson, Inc. (PI)
Development of a 1,000 Level 3C
Fiber Optic Borehole Seismic Receiver
Array Applied to Carbon Sequestration
DE-FE0004522
Björn N.P. Paulsson
Paulsson, Inc.
U.S. Department of Energy
National Energy Technology Laboratory
Carbon Storage R&D Project Review Meeting
Developing the Technologies and Building the
Infrastructure for CO2 Storage
August 21-23, 2012
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
• Goals: Design, build, and test a high performance
borehole seismic receiver system to allow cost
effective geologic Carbon Capture and Storage (CCS)
• Objectives: A: Develop technology to allow
deployment of a 1,000 level drill pipe deployed 3C
Fiber Optic Geophone (FOG) receiver array for deep
boreholes. B: Build a 150 level 3C 15,000 ft long
prototype system. Test the prototype system, and
conduct a borehole seismic survey at a Carbon
Capture and Storage site with the fiber optic borehole
seismic prototype system
Project Overview: Goals and Objectives
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Long array => large
direct arrival angle range
Seismic Imaging
26,000 ft TD
3,000 ft
23,000 ft
Shot 3,000 ft
Surface (high noise level =
low S/N ratio)
Surface Seismic
Receiver array
Long Array Coverage Short Array Coverage
Weathering layer x 2
(high attenuation = low freq)
Long array => the large
reflection angle range
needed for inversion of
data
Surface Seismic Imaging Borehole Seismic Imaging with short arrays Borehole Seismic Imaging with ultra long arrays
Borehole (low
noise level =
high S/N ratio)
Interferometric Imaging
using receivers below
weathering layer
Weathering layer
X 1 (low
attenuation =
high freq)
Borehole (low
noise level =
high S/N ratio)
Weathering layer
X 1 (low
attenuation =
high freq)
More Receivers = Better Image
Micro
Seismic
event
Ultra
Lo
ng
Bo
reh
ole
Re
ce
ive
Arr
ay
Fault
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Micro Seismic – a closer look!
Examples of Fault Imaging using
Borehole Seismology
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© 2012 Paulsson, Inc. (PI)
SAFOD Survey Site – Parkfield, California
Zoback (2006) Alden (2009)
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
San Andreas Fault Survey Site – Parkfield, California
USGS 2005
The 3rd generation, 80 level
4,000 ft long array is too short –
should have use a longer array -
but not available in 2005!
The 80 level Receiver Array
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© 2012 Paulsson, Inc. (PI)
VSP 1D P-Wave Velocity Inversion
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A “Zero Offset” Micro Seismic Event Recorded on a Paulsson 3rd Generation Borehole Seismic Array
MD (m)
Tim
e (
ms)
FT FN V
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© 2012 Paulsson, Inc. (PI)
•P and S Wave Velocity Inversions using Micro-seismic Data:
•This is only possible with an Ultra Long Borehole Seismic Array
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Red: pushing first break
Green: pulling first break
M2.77
M1.03
Micro-Seismic Source Locations (Top View). Data from the 3rd Gen Paulsson Borehole Seismic Array
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© 2012 Paulsson, Inc. (PI)
Micro-Seismic Source Locations (3D View)
80 km3 monitored Red: pushing first break
Blue: Pulling first break
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A Micro-Seismic Event (5/1/2005 19:27) MD (m)
Tim
e (
ms)
FT FN V
USGS: M1.26
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Micro-Seismic Source Locations
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Micro-Seismic Source Locations
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© 2012 Paulsson, Inc. (PI)
A Micro-Seismic Event (5/4/2005 9:23) MD (m)
Tim
e (
ms)
FT FN V
USGS: M1.86
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© 2012 Paulsson, Inc. (PI)
Micro-Seismic Source Locations
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Micro-Seismic Source Locations
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© 2012 Paulsson, Inc. (PI)
Frio CO2 Site, VSP Deconvolved + Upgoing P Waves
Using Paulsson 3rd Generation Borehole Seismic Array
Shot #1 - upgoing Shot #1 - deconvolved He & Paulsson, 2011
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© 2012 Paulsson, Inc. (PI)
Frio VSP: P & S Velocity Models
Using Paulsson’s 3rd Generation Array
He & Paulsson, 2011
High Quality Velocity Model needed to map Micro Seismic Events
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© 2012 Paulsson, Inc. (PI)
Generalized Interferometric Migration (GIM)
of Side Reflections in VSP Data
He & Paulsson, 2011
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© 2012 Paulsson, Inc. (PI)
Paulsson 3rd Generation Borehole Seismic Data
Hodograms to Determine Vector of Reflection
S1 S2
S4
S3
S5 S6
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VSP Generalized Interferometric Migration (MIG)
of a Salt Flank (red) & Faults (yellow)
He & Paulsson, 2011
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© 2012 Paulsson, Inc. (PI)
Frio CO2 Site: Surface Seismic Image
with VSP mapped Salt Flank location
~ 3000 ft
Salt flank Image
from VSP
He & Paulsson, 2011
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Frio Well Ties: Compare Fault image from well log
geology and from VSP imaging
Well # 4 Well # 3
Image of fault
from VSP data
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Baseline – 2002 Monitor – 2003 after 18 months
Depth Amplitude Maps showing the CO2 Injection
O’Brien et al., 2004
Change of reflectivity due
to the injected CO2
Paulsson 3rd Generation Borehole Seismic arrays
used for CO2 Time Lapse Monitoring Surveys
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
Accomplishments to Date
– Developed an Ultra Sensitive Fiber Optic Geophone
– Tested the Fiber Optic Geophone at High Temperature at
large Range of Frequencies and Loads
– Developed a Facility to Manufacture High Performance
Fiber Optic Geophone (FOG’s) Arrays
– Designed and built a 30,000 psi capable 3C geophone
pod for the Fiber Optic Geophones
– Developed a Deployment System strong enough to
deploy a 1,000 level 3C borehole seismic arrays in
vertical and horizontal boreholes.
– Manufactured components for a five level FOG array
49
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© 2012 Paulsson, Inc. (PI)
1. Fiber Optic Sensor Development
2. Deployment System Development
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Public Service of Colorado Ponnequin Wind Farm
The Clean Room for the Manufacturing of the
300ºC Fiber Optic Borehole Geophones
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
The 300ºC Dynamic Test Station for the 300ºC
Fiber Optic Borehole Geophones
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
Dynamic Test Facility
- Sensors are mounted onto a plate on the shaker
table: Swept frequency (0 up to 4kHz)
- Accelerometer (x2) and Electric Geophone signal
are both directly captured by the DAQ system
(oscilloscope/Spectrum Analyzer).
- The Paulsson Fiber Optic Geophone signal:
- The optical measurement is the differential phase
(radians)
- The measured modulated phase is first analyzed by
the interrogator, then
- The optical modulation is then converted to electric
signal (digital).
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© 2012 Paulsson, Inc. (PI)
Dynamic Test Station Noise Improvements: April – August 2012
Noise @ 60 Hz, 120 Hz, 180Hz
Shaker Blower Noises
April 2012: Shaker On (but no vibration)
August 2012: Shaker On (but no vibration)
Noise Floor has been improved by a factor > 100
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Paulsson Fiber Optic Geophone (PFOG)
Improved Sensor’s Sensitivity > 4x in V2 vs. V1
Both sensors being driven @ 10mG and 200 Hz
- Great Improvements in sensitivity in V2 ( > 4x Improvement!) compared with V1.
- Sensor will be better isolated in a down-hole environment where the temperature will
also be stable
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Environmental noise
- Great Improvements in noise floor in V2 compared to V1
- As expected, we still experience higher environmental noises in our lab at low frequencies.
- Sensor will be better isolated in a down-hole environment where the temperature will also be stable
- We are confident, we can reduce the noise floor to < 10 nG for the whole band in the near future
50 nG
10 nG
Fiber Optic Geophones and Interrogator Noise Floor
Sensor’s Sensitivity and noise floor improvement
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© 2012 Paulsson, Inc. (PI)
THE PAULSSON FIBER OPTIC
GEOPHONE
VS.
OTHER SENSORS
@ 25°C
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
All Sensors - Frequency Response (10 Hz 400 Hz)
using a 600 µG Acceleration @ 25°C
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© 2012 Paulsson, Inc. (PI)
0
0.0002
0.0004
0.0006
0.0008
0.001
0 20 40 60 80 100 120 140 160 180 200
Reco
rded
Am
plitu
des
Frequency (Hz)
10 to 200 Hz 600 µG Sweep @ 25°C PCB (Ref)
15 Hz High Temp Geophone
PFOG
PCB Acc
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© 2012 Paulsson, Inc. (PI)
0
0.0002
0.0004
0.0006
0.0008
0.001
0 50 100 150 200 250 300 350 400
Reco
rded
Acc
ele
rati
on
(G
's)
Frequency (Hz)
10 to 400 Hz 600 µG Sweep @ 25°C PCB (Ref)
15 Hz High Temp Geophone
PFOG
PCB Acc
Mounting plate imbalance
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© 2012 Paulsson, Inc. (PI)
0
0.0002
0.0004
0.0006
0.0008
0.001
0 100 200 300 400 500 600 700 800
Reco
rded
Am
plitu
des
Frequency (Hz)
10 to 800 Hz 600 µG Sweep @ 25°C PCB (Ref)
15 Hz High Temp Geophone
PFOG
PCB Acc
Mounting plate imbalance
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© 2012 Paulsson, Inc. (PI)
0
0.0002
0.0004
0.0006
0.0008
0.001
0 200 400 600 800 1000 1200
reco
rded
Am
plitu
de
Frequency (Hz)
10 to 1200 Hz 600 µG Sweep @25°C PCB (Ref)
15 Hz High Temp Geophone
PFOG
PCB Acc
Mounting system resonance Mounting plate imbalance
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© 2012 Paulsson, Inc. (PI)
THE PAULSSON FIBER OPTIC
GEOPHONE
VS.
OTHER SENSORS
@ 200°C
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
All Sensors - Frequency Response (10 Hz 400 Hz)
using a 600 µG Acceleration @ 200°C
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
0.0000
0.0002
0.0004
0.0006
0.0008
0.0010
0 100 200 300 400 500 600 700 800
Re
co
rde
d A
mp
litu
de
s
Frequency (Hz)
10 to 800 Hz 600 µG Sweep @ 200°C PCB (Ref)
15 Hz High Temp Geophone
PFOG
PCB Acc
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© 2012 Paulsson, Inc. (PI)
0
0.0002
0.0004
0.0006
0.0008
0.001
0 100 200 300 400 500 600 700 800
Reco
rded
Am
plitu
des
Frequency (Hz)
10 to 800 Hz 600 µG Sweep @ 25°C PCB (Ref)
15 Hz High Temp Geophone
PFOG
PCB Acc
Mounting plate imbalance
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© 2012 Paulsson, Inc. (PI)
High Precision Low Frequency
Vibration System @ Low Amplitude
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PFOG Performance Test at Frequencies < 1Hz
Test @
0.03 Hz
- 3 PFOGs are mounted axially to motion and modulated at 0.03 Hz
- The motion is controlled by a PC at all frequencies (from <1 Hz to higher frequencies)
Test @
0.03 Hz
- Single PFOG sensor modulated at 0.03 Hz (33 seconds period)
- The Actuator is controlled by a PC at all frequencies (from <1 Hz to higher frequencies)
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
PFOG Test @ 0.03 – 1 Hz (33 – 1 sec period)
0
50
100
150
200
250
300
0.00 0.20 0.40 0.60 0.80 1.00
Am
pli
tud
e
Frequency (Hz)
Low Frequency Response Amplitude
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
Seismic Traces from Tap Test Simultaneous Acquisition of all sensors; Band Pass Filter: 5 – 2,500 Hz
Reference Accelerometer
Reference 15 Hz Geophone
Fiber Optic Geophone (FOG)
Note the high S/N ratio
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© 2012 Paulsson, Inc. (PI)
1. Fiber-Optic Geophone’s design is successful
a. Flat frequency response over a large frequency
range
b. Low Frequency performance
c. Very high sensitivity
d. High Signal to Noise ratio
2. Outstanding Issues
a. Resonances in the test setup
b. Facility’s environmental noise
c. Interrogation system tuning
Conclusions
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
The OpticSeis™ 3C Pod
For The Fiber Optic Geophone
2” OD
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© 2012 Paulsson, Inc. (PI)
1. Fiber Optic Sensor Development
2. Deployment System Development
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© 2012 Paulsson, Inc. (PI)
Drill Pipe Based Borehole Seismic
Deployment System
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© 2012 Paulsson, Inc. (PI)
The Borehole Seismic Deployment System
Drill Pipe Based Deployment System
Pipe Strength: 140,000 lbs (verified July 25, 2011)
Depth Capability: 30,000 ft
Pressure Rating: 30,000 psi
Clamping Actuators: 572ºF (300ºC)
Temperature for Optical System: 572ºF (300ºC)
Optical 3C Levels: 1,000
Deployable in both Vertical and Horizontal wells
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
Geophone Pod
Housing
and the Fiber Optic
Pod Geophone pod
Casing Casing
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
Destructive Testing of Tool Joints
Test of Tool Joints for
Seismic Array on Nov. 22, 2010
Measured Strength: 210,000 lbs.
Failed at 238,000 lbs.
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
Destructive Testing of Deployment drill pipe
Test of Deployment Drill Pipe for
Seismic Array on July 25, 2011
Measured Strength: 145,000 lbs.
Failed at 160,000 lbs.
Failed at 160,000 lbs.
Strength: 145,000 lbs.
Before Failure After Failure
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
Deployment Drill Pipe During Manufacturing
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
15,000 ft of Deployment Drill Pipe
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© 2012 Paulsson, Inc. (PI)
4 min. 10 sec.
4 min. 27 sec.
Destructive Test of Geophone Pod Housing
20,000 lbs.
300,000 lbs.
¾” elongation
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© 2012 Paulsson, Inc. (PI)
4 min. 27 sec.
4 min. 28 sec.
Destructive Test of Geophone Pod Housing
July 30, 2012
300,000 lbs.
303,100 lbs.
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
Paulsson Project Summary
– Fiber Optic Geophones (FOG’s) are more sensitive than
regular geophones
– FOG’s can operate at high temperature
– FOG’s have a very large band width: 0.03 Hz – 4kHz
– Lessons Learned:
• Require a high quality measurement and calibration system
• Manufacturing is expensive
• Manufacturing takes a long time and must be carefully tracked
– Currently Building a Five Level 3C Array
– Plan to test Five level array in September 2012
– Complete a 150 level 3C FOG array in 2013
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
Thank you!
www.paulsson.com
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
Appendix
– These slides will not be discussed during the
presentation, but are mandatory
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
Project Team and Project Organization
• Project Team
• Paulsson, Inc. − Principal Investigator, System design, Fiber Optic Sensor
Design and Manufacturer, Design geophone pods
• Fiber Optic Interrogator Manufacturer − System noise abatement, Interrogator design & manufac.
• Drill Pipe Manufacturer − Design tool joints, manufacture drill pipe and related
components
• Machine Shops − Manufacture geophone pods, geophone pod housings
and other components
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
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Paulsson Organization Chart
Paulsson, Inc.
Fiber Optic Interrogator
Manufacturer
Drill Pipe Manufacturer
Machine Shops
Engineering Consultants
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Paulsson Fiber Optic Geophone
Project Gantt Chart
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© 2012 Paulsson, Inc. (PI) © 2012 Paulsson, Inc. (PI)
Bibliography
List peer reviewed publications generated from
project per the format of the examples below
• First Publication Expected in 2013
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