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Velocity Estimation by Waveform Tomography in the Canadian Foothills: A Synthetic Benchmark Study Andrew J. Brenders 1 Sylvestre Charles 2 R. Gerhard Pratt 1 1 Queen’s University, Kingston, Ontario 2 Talisman Energy Inc., Calgary, Alberta
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2 Outline Introduction to the Canadian Foothills and Motivation for Waveform Tomography Synthetic Geological Model and Data Waveform Tomography: Methodology Waveform Tomography: Results Discussion & Conclusions
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3 Canadian Foothills Exotic terranes accreted to Pacific margin of N.America West: Series of large sheets of thrusted Paleozoic rocks East: WCSB (relatively undeformed) Waveform Tomography in the Foothills: Introduction to the Canadian Foothills Rocky Mountain Fold & Thrust Belt Western Canadian Sedimentary Basin Foothills
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4 Waveform Tomography in the Foothills: Motivation Great difficulties in velocity model estimation and subsequent imaging of Foothills seismic data Conventional seismic data processing usually inadequate Steep dips Rugged topography Near-surface weathering Poor signal quality
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5 Waveform Tomography in the Foothills: Motivation Gray and Marfurt, 1995 Yan and Lines, 2001 Dell’Aversana et al., 2003 Operto et al., 2004 Assumptions: Velocity generally increasing with depth Relatively simple near-surface model “Migration from topography…” “Imaging of an Alberta foothills seismic survey” “Velocity/interface model building in a thrust belt by tomographic inversion of global offset data” “Quantitative imaging of complex structures from dense wide- aperture seismic data by multiscale traveltime and waveform inversions: a case study”
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6 Waveform Tomography in the Foothills: A Synthetic, Structurally Complex Model Model defined on 1 x 1 m grid 26 km horizontally & 6.5 km vertically Based on PSTM structural interpretation Estimates of P-wave velocity and density from well logs For future studies: S-wave velocity and anisotropy parameters ( and ) Targets
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7 767 m Waveform Tomography in the Foothills: A Synthetic, Structurally Complex Model Topography Low-velocity weathering (25 m) and sub-weathering (100 m) layers
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8 Waveform Tomography in the Foothills: A Synthetic, Structurally Complex Model Low velocity river fill Steep dips High velocity carbonate outcrops Varying topography & near-surface velocity
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9 Waveform Tomography in the Foothills: A Synthetic, Structurally Complex Model Poor geophone coupling Trapped modes Base sub-weathering layer Karsting, Fractures
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10 Waveform Tomography in the Foothills: Methodology Waveform Tomography Traveltime (diving wave) tomography followed by full-waveform inversion Visco-acoustic wave equation Nonlinear inversion by linearised gradient method Implemented in the frequency-domain Successes: Synthetic, blind tests with visco-elastic data (e.g., Brenders and Pratt, 2003 & 2007) Real, long-offset data in exploration settings (e.g., Operto et al., 2004; Jaiswal et al., 2008)
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11 Waveform Tomography in the Foothills: Methodology Why Waveform Tomography ? Emphasis on refracted energy carbonate outcrop Shadow zone; MVA failure
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12 Waveform Tomography in the Foothills: Methodology Advantages: Frequency-space domain Low frequencies inverted first Mitigates non-linearity Multi-scale strategies Efficient modelling for multiple sources Incorporation of Q( ) Challenges Requires low-frequencies or long-offsets Accurate starting models are required Limitations Acoustic wave-equation only Missing explicit case of a free-surface above rugged topography (e.g., Saenger et al., 2000) TTI/VTI anisotropy
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13 Waveform Tomography in the Foothills: A Synthetic Benchmark Dataset Finite-Difference Modelling of Synthetic Data Acquisition Parameters: Typical “Real” Foothills data Shot interval: 100 m, 18 to 30 m depth Receiver interval: 25 m (grouped) Maximum offsets: 10+ km, split-spread Our Synthetic Foothills data Shot interval: 25 m, 20 m depth below surface Receiver interval: 12.5 m, on surface topography Maximum offsets: 26 km recorded (not all used)
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14 Waveform Tomography in the Foothills: A Synthetic Benchmark Dataset Finite-Difference Modelling of Synthetic Data Computationally intensive: Modelled with Q = 20 in air, Q = 1000 in model to damp air wave, add numerical stability f max [m/s] v min [m/s] x, z X [m]Z [m]NxNzRAM 480050260256500542151152 Mb 1680012““21905631.6 Gb 258008““32748343.6 Gb 408004““52261321? f max [m/s] v min [m/s] x, z X [m]Z [m]NxNzRAM 480050260256500542151152 Mb 1680012““21905631.6 Gb 258008““32748343.6 Gb 408004““52261321?
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15 Waveform Tomography in the Foothills: A Synthetic Benchmark Dataset Minimum phase source signature Low dominant frequency, f max = 16 Hz
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16 Waveform Tomography in the Foothills: A Synthetic Benchmark Dataset Minimum phase source signature Low dominant frequency, f max = 16 Hz
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17 Waveform Tomography in the Foothills: A Synthetic Benchmark Dataset Minimum phase source signature Low dominant frequency, f max = 16 Hz
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18 Waveform Tomography in the Foothills: A Synthetic Benchmark Dataset Synthetic shot gatherReal Foothills shot gather Realistic offsets: 10 km, split-spread
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19 Waveform Tomography in the Foothills: A Synthetic, Benchmark Dataset Synthetic data preprocessing / preparation Starting Model Diving wave methods (e.g., Sirgue and Pratt (2004), Ravaut et al. (2004))
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20 Waveform Tomography in the Foothills: Starting Models from Diving Wave Methods Starting model, 1-D RMS misfit: 141 ms
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21 “Shadow” zones Waveform Tomography in the Foothills: Starting Models from Diving Wave Methods 20 iterations, 131 x 1041 traveltimes, 26 km offset RMS misfit: 34 ms RMS misfit: 141 ms
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22 Waveform Tomography in the Foothills: Forward Modelling for Waveform Comparison Sx = 15.525 km
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23 Waveform Tomography in the Foothills: Results from a Synthetic Model f min = 0.4 Hz f max = 7.083 Hz 2 - 8 km offset
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24 Waveform Tomography in the Foothills: Results from a Synthetic Model BlackTrueRed0.4 - 3.0 Hz GrayStartBlue3.0 - 7.0 Hz
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25 Waveform Tomography in the Foothills: Results from a Synthetic Model BlackTrueRed0.4 - 3.0 Hz GrayStartBlue3.0 - 7.0 Hz
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26 Fullwv Model 0.4 - 3 Hz Sx = 15.525 km Fullwv Model 2.1 - 7 Hz Sx = 15.525 km Waveform Tomography in the Foothills: Results from a Synthetic Model
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27 Waveform Tomography in the Foothills: Effects of Higher Starting Frequencies f min = 0.4 Hz, f max = 7.0 Hz 2 - 8 km offset, = 2.6 Black True Gray StartBlue0.4 - 7.0 Hz Higher starting frequencies?
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28 Waveform Tomography in the Foothills: Effects of Higher Starting Frequencies f min = 2.1 Hz, f max = 7.0 Hz 2 - 8 km offset, = 2.6 Black True Gray StartBlue2.1 - 7.0 Hz
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29 Waveform Tomography in the Foothills: Effects of Higher Starting Frequencies f min = 2.1 Hz, f max = 7.0 Hz 2 - 12 km offset, = 2.6 Black True Gray StartBlue2.1 - 7.0 Hz
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30 Waveform Tomography in the Foothills: Effects of Higher Starting Frequencies f min = 3.1 Hz, f max = 7.0 Hz 2 - 12 km offset, = 2.6 Black True Gray StartBlue3.1 - 7.0 Hz
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31 Waveform Tomography in the Foothills: Discussion & Conclusions Results: Resolution within “shadow zones” Steeply dipping fault imaged between Triassic carbonates and Cretaceous clastics Syncline structures of Jurassic / Cretaceous clastics between tightly folded Triassic structures well imaged Structural indication of fault propagation fold Mississipian targets Anticlines above duplex structures visible
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32 Waveform Tomography in the Foothills: Discussion & Conclusions Waveform tomography with low-frequency data insensitive to near-surface, short-wavelength “statics” Improvement on conventional refraction “statics”? Are elastic / anisotropic effects an issue? Time-domain, elastic, anisotropic data under construction Migration with waveform tomography velocity models? Is this necessary, given the “migration-like” images obtained?
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33 Waveform Tomography in the Foothills: Discussion & Conclusions Conventional reflection processing “Model” and “image” have different spectral characteristics Each derived from distinct aspects of the data Reflectivity “image” (Yilmaz, 2003) Velocity model for PSDM vs.
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34 Waveform Tomography in the Foothills: Discussion & Conclusions High-wavenumber, geologically interpretable “images” resolved in “model”
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35 Waveform Tomography in the Foothills: Discussion & Conclusions High-wavenumber, geologically interpretable “images” resolved in “model”
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36 Waveform Tomography in the Foothills: Discussion & Conclusions High-wavenumber, geologically interpretable “images” resolved in “model”
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37 Waveform Tomography in the Foothills: Discussion & Conclusions “Conventional” reflection processing (with real data)
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38 Acknowledgements Sylvestre Charles, Gerhard Pratt Steve Cloutier Bob Quartero, Ross Deutscher, Francois Legault, Mark Hearn, Hugh Geiger, Carmela Garcia
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