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Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

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Page 1: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Physical Modeling: Time Lapse, 3D, and VSP

Robert W. WileyAllied Geophysical Laboratories

University of Houston

Page 2: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Outline

• Properties of Physical Modeling

• Fracture Model

• Time-Lapse Model

• 3D VSP Model

• Hardware

• Future Directions

• Conclusions

Page 3: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Properties that scale well

• Distance (typically we use 1km = 10 cm)• Time (typically we use 4 ms = 0.4 s)• Frequency (typically we use 30 Hz = 300 kHz)• P and S velocity

– For acoustic propagation we scale vp by 0.5– For elastic propagation we do not rescale

• Viscosity– Gas by air– Water by water– Oil by glycerol

Page 4: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Properties that do not scale well• Source and receiver size• Pore size (other physics takes place for extremely small pores)• Frequency dependent attenuation mechanisms (which we don’t

yet understand anyway!)• Soft sediments and weathering zones

Other limitations• A model 1 m by 1 m by 0.5 m (corresponding to 10 km x 10

km by 5 km) weighs more than one metric ton!• Models take months to build • We needed bigger, stronger, and more patient graduate

students!

Page 5: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Fracture Model

Page 6: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Fracture ConstructionFracture Construction

1.1 cm

Glass slides

35.5 cm

Glass blocks

Resin

x

Fracture model under construction showing glass slides in situ

y

Page 7: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

HTI model

y

x

63.5 cm63.5 cm

50.8 cm50.8 cm

Fracture zoneFracture zone

Page 8: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

2.5

3

2

1071 CDP 1360

Line 2151

Page 9: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

+ + -

2.2

2.4

2.6

1071 1360

Tim

e (s

)

CDPLine 2140 500 m Offset

Page 10: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Trace Number

200

1

1 200100 300

Line

Damp for 750 m offset – time slice 2430 ms – Perp.

Page 11: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Positive Amplitude

Most Positive Curvature Most Negative Curvature

Principle Comp Filter

Page 12: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Time-Lapse Model

Page 13: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

The model as constructed

(Wardana, 2001)

Page 14: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Time lapse modeling

(Wardana, 2001)

wet

half wet

dry

near mid far

Amplitude

Page 15: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Time lapse modeling

(Wardana, 2001)

wet

half wet

dry

near mid far

Coherence

Page 16: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

3D VSP Model

Page 17: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Physical model

6 layer alternate blue and black & a salt body ρblue= 2.4 g/cc ρblack = 1.34 g/cc Vblack= 2586.9 m/sVblue =3264.3 m/s

Page 18: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Preprocessing (First break pick)

Page 19: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Hardware

Page 20: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

3 C Transducers Shear Transducers

Pin TransducersSpherical Transducers

TRANSDUCERS

Page 21: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Old System (Backup System)

Page 22: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

NI 2 Source 4 Receiver System

Dry Tank

Page 23: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

NI 8 Source 16 Receiver System

Wet Tank

Page 24: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Initial Configuration

Data Configuration

Page 25: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

NI System Control- LabView Based

Main Window

Position Control Window

Page 26: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Future Directions

• Bring the two new systems on line

• Develop a 16 receiver system

• Develop a multiple source system

• Collect porous model data

• Test additional transducers

• Investigate other materials

Page 27: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Conclusions

• We are able to build reasonably complex physical models

• Results are similar to seismic data

• This is an excellent approach to acquiring controlled data for testing algorithms

• Physical modeling is cost effective compared to field experiments

Page 28: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Thank You

Page 29: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

CurvatureCurvature2.4

2.6

CDP

Line 2140 500 m Offset

1150 1202

Page 30: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Pinducer

Page 31: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Physical Limitations

• Inaccurate construction of actual model

• Limited selection of velocity and density parameters

Page 32: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Some Limitations

• Limited bandwidth with strong resonance at one frequency

• Limited to materials with specific elastic parameters

• Difficult to build lateral velocity variations

• Labor intensive

• Cannot model all real earth materials/layers

Page 33: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Source and Receiver Issues

• Inaccurate location of source and receiver with respect to the model

• Source and receiver resonate at one frequency

• Source and receiver dimensions are large

• Source and receiver have pronounced radiation patterns

Page 34: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

+ + -

2.2

2.4

2.6

1071 1360

Tim

e (s

)

CDPLine 2140 500 m Offset

Page 35: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Properties that do not scale well• Source and receiver size• Pore size (other physics takes place for extremely small pores)• Frequency dependent attenuation mechanisms (which we don’t

yet understand anyway!)• Soft sediments and weathering zones

Other limitations• A model 1 m by 1 m by 0.5 m (corresponding to 10 km x 10

km by 5 km) weighs more than one metric ton!• Models take months to build • We needed bigger, stronger, and more patient graduate

students!

Page 36: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Why Run Models

• To test interpretation – Salt dome, coal seam

• To test algorithm – Migration, Multiple removal

• To test interpretation tools – fracture identification, fluid content

• To test theory – Lamb’s problem, Kirchhoff diffraction, anisotropy

Page 37: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Why Physical Modeling

• No simplifying mathematical assumptions

• No approximations to mathematical functions

• No round-off errors

• No a priori mathematical understanding required

Page 38: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Limitations

• Limited selection of velocity and density parameters

• Difficult to build lateral velocity variations

• Labor intensive

• Inaccurate construction of actual model

• Limited to frequency response of transducers

• Source and receiver dimensions

Page 39: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Benefits of Physical Modeling

• Experimental repeatability and controlled conditions

• Very cost-effective compared to field work

• Physics of elastic energy propagation through physical models is same as real world

• Arbitrary earthlike conditions closer to real earth data than numerical modeling

Page 40: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

Spherical Transducer

Page 41: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

3C Transducer

Page 42: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston

www.valpeyfisher-ud.com

Shear Transducer Design

Page 43: Physical Modeling: Time Lapse, 3D, and VSP Robert W. Wiley Allied Geophysical Laboratories University of Houston