Center for Subsurface Imaging and Fluid Modeling 2010 Shuyu Sun and GT Schuster 8 PhD students, 5 Research Fellows (Prof Sherif Hanafy, Dr. Chaiwoot B. et al.) Bill Bosworth: PhD Colgate, Marathon 21 years, Apache 5 years, senior research advisor Apache Mike Zinger: BS Iowa State, Amoco 20 years, 10 years Aramco,Team Leader Red Sea Expl. Shuyu Sun: PhD UT Austin, S. Carolina Univ., reservoir simulation Dinesh Kaushik: PhD, Gordon Bell Prize, algorithms C. Boonyasiriwat: PhD, U of Utah, FWI and simulation David Keyes: PhD Harvard, Columbia Univ.,Yale Univ., Gordon Bell Prize, VP SIAM Ibrahim Hoteit: PhD J. Fourier, Data assimilation Raed Al Huseini: PhD, Economic Development Great Appreciation Mara Rovelli, Sabrina Percher, Marielaure Boulot, Antonia Forshaw, Mirna Haydar, Mariam Fouad Center for Subsurface Imaging and Fluid Modeling 2010 Shuyu Sun and GT Schuster 8 PhD students, 5 Research Fellows (Prof Sherif Hanafy, Dr. Chaiwoot B. et al.) Center for Subsurface Imaging and Fluid Modeling (CSIM) Consortium • Goal: Develop innovative • computational methods for seismic imaging and subsurface fluid flow modeling. Examples include 3D waveform inversion, 3D RTM, TI modeling, reservoir fluid simulator. Advantages More than $1,500,000/yr in KAUST research funds, tightly coupled visualization+supercomputer resources + reservoir fluid modeling+ seismic imaging Computers: IBM Blue Gene 225 Tflop, Intel+GPU Clusters : • GPU+IBM experts • Benefits: Yearly Houston meeting, annual reports, access to student interns, expert in fluid flow modeling, seismic, and eventually EM imaging • Collaborations: UT Austin (Stoffa+TTI), UU (GPU) Research Goals G.T. Schuster (Columbia Univ., 1984) Seismic Interferometry: VSP, SSP, OBS Multisource+Preconditioned RTM+MVA+Inversion+Modeling: Seismic Lab: >630 Channel capacity, resisitivity TTI 3D RTM, GPU: Stoffa+CSIM, UUtah K. Johnson SCI, PSU, KAUST Cornea Shaheen Research Goals Shuyu Sun (UT Austin, 2005) Modeling of multiphase flow in porous media (new approaches for fractures, diffusion, capillarity …) Advanced finite element methods (dynamic mesh adaption, multiscale resolution, element-wise conservation, efficient linear solvers, …) Computational thermodynamics of reservoir fluid 2010 CSIM Consortium ($25 K/year) Inaugural Members: Aramco, Exxon, Chevron, BP, Petrobras, GXT, PEMEX Annual Meeting: Houston Jan. 2011 Midyear Report: Summer 2010 Software Policy: Same as UTAM for Schuster Shuyu Sun Policy http://utam.gg.utah.edu/csim Multisource Seismic Imaging vs CPU Speed vs Year 100000 10000 1000 copper Aluminum 100 VLIW Superscalar 10 RISC 1 1970 1980 1980 1990 2000 Year 2010 2020 Motivation for Better Seismic Imaging Strategy Jack Buckskin ¼ billion $$$ well Kaskida Tiber 35,055 Feet FWI Problem & Possible Soln. • Problem: FWI computationally costly • Solution: Multisource Encoded FWI Preconditioning speeds up by factor 2-3 Iterative encoding reduces crosstalk Multisource Phase Encoded Imaging { Forward Model: L { d d +d =[L +L ]m 1 2 1 2 mmig=LTd Multisource Migration: T T =[L +L ](d + d ) 1 (k+1) (k) 2 T 1 T m = m + = L d +L d + 1 1 2 2 Standard migration 2 T T L 1d 2+L2d1 Crosstalk noise Multisource S/N Ratio d 1 , d 2 , …. d1 +d 2 +…. LT [d1 + d2 +.. ] LT [d 1+ d 2 + … ] # CSGs # geophones/CSG Multisrc. Migration vs Standard Migration # geophones/CSG # CSGs MS ~ M vs ~ S-1 MS Iterative Multisrc. Migration vs Standard Migration # iterations MI vs MS Crosstalk Term T T L 1d 2+L2d1 Time Statics Time+Amplitude Statics QM Statics Summary T T L 1d 2+L2d1 Time Statics 1. Multisource crosstalk term analyzed analytically 2. Crosstalk decreases with increasing w, randomness, Time+Amplitude Statics dimension, iteration #, and decreasing depth 3. Crosstalk decrease can now be tuned QMdetailed Statics analysis and testing needed to refine 4. Some predictions. Multisource Technology • Fast Multisource Least Squares Kirchhoff Mig. • Multisource Waveform Inversion (Ge Zhan) 3 Z k(m) 0 The Marmousi2 Model 0 X (km) 16 The area in the white box is used for S/N calculation. Z k(m) 0 Conventional Source: KM vs LSM (50 iterations) 3 KM (1x) X (km) 16 Z (km) 0 0 3 LSM (100x) 0 X (km) 16 Z k(m) 0 200-source Supergather: KM vs LSM (300 its.) 3 KM (1/200x) X (km) 16 Z (km) 0 0 3 LSM (33x) 0 X (km) 16 S/N = MI 0 S/N 7 The S/N of MLSM image grows as the square root of the number of iterations. 1 I 300 Multisource Technology • Fast Multisource Least Squares Migration ( Dai) • Multisource Waveform Inversion (Boonyasiriwat) Multisource Encoded FWI Nd +Nd =[NL +NL ]m Forward Model: 1 Multisource Migration: Multisrc-Least FWI: 1 2 2 1 1 2 2 mmig=LTd m =[LTL]-1LTd multisource preconditioner Preconditioned m’ = m -f LT[Lm - d] f ~ [LTL]-1 Steepest Descent Multiscale Waveform Tomography 1. Collect data d(x,t) syn. 2. Generate synthetic data d(x,t) by FD method 3. Adjust v(x,z) until ||d(x,t)-d(x,t)syn.|| 2 minimized by CG. 4. To prevent getting stuck in local minima: a). Invert early arrivals initially mute b). Use multiscale: low freq. high freq. 7 Boonyasiriwat et al., 2009, TLE 0 km 6 km/s 6 km 3 km/s 0 km 20 km Waveform Tomograms 0 km 6 km/s Initial model 6 km 0 km 3 km/s 6 km/s 5 Hz 6 km 3 km/s 0 km 6 km/s 10 Hz 6 km 3 km/s 0 km 6 km/s 20 Hz 6 km 0 km 3 km/s 20 km Data Pre-Processing 3D-to-2D conversion Attenuation compensation Random noise removal 17 Source Wavelet Estimation Generate a stacked section Pick the water-bottom Stack along the water-bottom to obtain an estimate of source wavelet In some cases, source wavelet inversion can be used. 17 Gradient Computation and Inversion Multiscale inversion: low to high frequency Dynamic early-arrival muting window Normalize both observed and calculated data within the same shot Quadratic line search method (Nocedal and Wright, 2006) A cubic line search can also be used. 17 Low-pass Filtering (b)0-15 5-HzHz CSG (b) CSG (c)0-25 10-Hz (c) HzCSG CSG 0 0 0.5 0.5 0.5 1 1 1 1.5 1.5 1.5 2 2.5 Time (s) 0 Time (s) Time (s) (a) Original CSG 2 2.5 2 2.5 3 3 3 3.5 3.5 3.5 4 0 2 4 Offset (km) 4 0 2 4 Offset (km) 4 0 2 4 Offset (km) 18 Dynamic Early-Arrival Muting Window Window = 1 s CSG(a) Original CSG(b) 5-Hz CSG 0 0 0 5 0.5 0.5 1 1 1 1 1.5 1.5 1.5 1.5 2 2.5 2 2.5 2 2.5 Time (s) 5 2 0.5 Time (s) 1 (b) 5-Hz CSG (c) 10-Hz CSG (c) 10-Hz CSG 0 0 0-15 Hz CSG Time (s) 0.5 Time (s) 5 Window = 1 s 2 2.5 3 3 3 3 3 5 3.5 3.5 3.5 3.5 4 40 m) 4 0 2 4 Offset (km) 4 2 40 Offset (km) 4 04 2 Offset (km) 0-25 Hz CSG 4 2 40 Offset (km) 2 4 Offset (km) 19 Dynamic Early-Arrival Muting Window Window = 2 s CSG(a) Original CSG(b) 5-Hz CSG 0 0 0 5 0.5 0.5 1 1 1 1 1.5 1.5 1.5 1.5 2 2.5 2 2.5 2 2.5 Time (s) 5 2 0.5 Time (s) 1 (b) 5-Hz CSG (c) 10-Hz CSG (c) 10-Hz CSG 0 0 0-15 Hz CSG Time (s) 0.5 Time (s) 5 Window = 2 s 2 2.5 3 3 3 3 3 5 3.5 3.5 3.5 3.5 4 40 m) 4 0 2 4 Offset (km) 4 2 40 Offset (km) 4 04 2 Offset (km) 0-25 Hz CSG 4 2 40 Offset (km) 2 4 Offset (km) 19 Traveltime Tomogram Results Depth (km) 0 Velocity (m/s) 3000 2.5 Waveform Tomogram Depth (km) 0 2.5 1500 0 X (km) 20 20 3000 Waveform Tomogram Depth (km) Velocity (m/s) 0 1500 2.5 Vertical Derivative of Waveform Tomogram Depth (km) 0 2.5 0 X (km) 20 21 Kirchhoff Migration Images 22 Kirchhoff Migration Images 22 Comparing CIGs 23 Comparing CIGs CIG from Traveltime Tomogram CIG from Waveform Tomogram 24 Comparing CIGs 25 Comparing CIGs CIG from Traveltime Tomogram CIG from Waveform Tomogram 26 Comparing CIGs 27 Comparing CIGs CIG from Traveltime Tomogram CIG from Waveform Tomogram 28 Multi-Source Waveform Inversion Strategy (Ge Zhan) 144 shot gathers Generate multisource field data with known time shift Initial velocity model Generate synthetic multisource data with known time shift from estimated velocity model Multisource deblurring filter Using multiscale, multisource CG to update the velocity model with regularization 3D SEG Overthrust Model (1089 CSGs) 15 km 3.5 km 15 km Numerical Results Dynamic QMC Tomogram (99 CSGs/supergather) Static QMC Tomogram (99 CSGs/supergather) 3.5 km Dynamic Polarity Tomogram (1089 CSGs/supergather) 15 km Multisource FWI Summary (We need faster migration algorithms & better velocity models) Stnd. FWI Multsrc. FWI IO 1 vs Cost 1 vs Sig/MultsSig Resolution dx 1/20 1/20 or better ? 1 vs 1 Multisource FWI Summary (We need faster migration algorithms & better velocity models) Future: Multisource MVA, Interpolation, Field Data, Migration Filtering, LSM