KYLE T. SPIKES Research Group

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Transcription:

KYLE T. SPIKES Research Group 1

WELCOME TO THE MEETING Welcome everyone! Currently we have 8 PhD and 3 MS students in total Presentations today cover a variety of topics in various stages of development Collaborator, Nicola Tisato, is currently building his laboratory, to be and running sometime this year Integrating his work with EDGER work is in the plans 2

Group Members Kyle T. Spikes, Associate Professor Dr. Kelvin Amalokwu, Post-Doctoral Fellow Mr. Tom Hess, Research Engineering Scientist Associate 3

Student Members 1. Elliot Dahl, PhD Student (EDGER) 2. David Tang, PhD Student (EDGER) 3. Wei Xi, PhD Student (EDGER) 4. Michael McCann, MS Student (EDGER) 4

Funding Effective medium model of shale properties: BP (PI: Spikes) Big data challenges subsurface fracture characterization: NSF (Wheeler and Sen) EDGER 5

CURRENT WORK ELLIOT DAHL P-wave velocity 3000 2950 a) ε = 0.04 Velocity [m/s] 2900 2850 2800 2750 ε = 0.02 ε = 0 2700 0 5 10 15 20 Frequency [khz] 6

CURRENT WORK ELLIOT DAHL P-wave dispersion ε= 0 ε= 0.02 ε= 0.04 7

CURRENT WORK DAVID TANG Energy Dispersive X-ray Spectroscopy (EDS) 8

CURRENT WORK DAVID TANG Segmentation Results NN Output 100 Clay/Pore 200 300 TOC 400 500 Quartz 600 Feldspar 700 800 Calcite 900 100 200 300 400 500 600 700 800 900 9

CURRENT AND ONGOING WORK Unconventionals Segmentation-less digital rock physics Probabilistic rock physics templates 10

UNCONVENTIONALS Well B4 Well B4 (Xline) 1655 1673 1691 1709 1655 1673 1691 1709 1230 1250 Lower EF 1270 1290 (TWT) Large Contrast P-Impedance S-Impedance 11

UNCONVENTIONALS Top of Eagle Ford Xline 2012 Eagle Ford Well B7 Porosity plus kerogen Porosity plus kerogen 12

SEGMENTATION-LESS DRP 13

SEGMENTATION-LESS DRP Typically, segmentation-based DRP overestimates velocities. Sell et al., 2016, Solid Earth 14

SEGMENTATION-LESS DRP Can we eliminate segmentation? (At least for ~mono-mineralic rocks) The premise: 1) Using ghosts or targets with known densities, we can calibrate our CT imagery to obtain a density model; 2) For mono-mineralic rocks, density can be easily translated to porosity; 3) Total density and porosity should match density and porosity from laboratory measurements. The concept: 1) Each voxel can be considered as an elementary volume whose effective elastic properties can be described by effective medium theory, e.g. Hashin-Shtrikman; 2) Thus the model does not depend upon the geometry of pores and grains but rather upon the distribution of porosity. 15

Gray Level to Density argets: Air AISI304 Al alloy SEGMENTATION-LESS DRP Log In addition, the rock is a target as we know its average density: Sample Applied the calibration formula to a sub-sample ~22x12 mm Calculated density: 2038 kg/m 3 (-1.1% measured, ~error) 16

SEGMENTATION-LESS DRP Segme ρ qtz = 2650 kg/m 3 ρ L = voxel density Φ L =0 for ρ L ρ qtz Φ L =1 for and ρ L =ρ air 1 Calculated total porosity 0.23 (~ +8%) 17

SEGMENTATION-LESS DRP Modified upper Hashin-Strikman bound (Nur et al., 1991,1995) with critical porosity Φ C =0.38 V p Segme Quartz density (ρ qtz ) 2650 kg/m 3 Quartz Bulk modulus (K qtz ) 36 GPa Quartz Shear modulus (G qtz ) 44 GPa Critical porosity (Φ c ) 0.38 V s V p V s (km/s) (km/s) 5.9 4.1 Note: ~3% of the voxels had Φ L >Φ C. Φ L forced to be = Φ C 0 0 18

Segme SEGMENTATION-LESS DRP Sofi3D to propagate elastic waves (Bohlen, 2002, Computers and Geosciences); Compressive wave generated at Z=0 mm (f=1mhz, sin 3 ); Measured the arrival time. Average of the displacement at Z=19.96 mm. V p =2875 m/s (~ +17% vs +74% of segm.) Note: The modified upper Hashin-Shtrikman bound calculated on the entire sample (i.e,. only considering Φ and not Φ L ) provided a P-wave velocity of 3680 m/s. 19

CONVENTIONAL ROCK PHYSICS TEMPLATE 2.8 2.6 2.4 *Gas sands *Brine sands? = 40% S W = 1.0 S W = 1 Establish a range of models that qualitatively explains the elastic properties as a function of the rock properties. V P /V S 2.2? = 24% In this case, lithology, porosity and saturation are the most dominant rock properties. 2 1.8 S W = 0.2 We then argue that the model does a decent job of explaining the data.? = 40%? = 24% S W = 0.2 2.5 3 3.5 4 4.5 5 5.5 6 6.5 I P km/s x g/cm 3 What about the uncertainty or error in the model?

PROBABILISTIC ROCK PHYSICS TEMPLATE P(φ,Sw Ip,./ )~P(φ,Sw) P(Ip,./ φ, Sw).0.0 Color = Relative Probability

PROBABILISTIC ROCK PHYSICS TEMPLATE How do you fill the model space? P(φ,Sw Ip,./.0 )~P(φ,Sw) P(Ip,./ φ, Sw) How do you determine how many distributions to have?.0 How much overlap or lack thereof should occur from one distribution to the next?

CLASSIFICATION OF LOG DATA 17 = Shale 9-16 = Sand, oil to brine 1-8 = Sand, gas to brine P(m) = P φ, Sw Ip,./.0 L d m = exp 1 2 x μ B Σ DE x μ 2πΣ P(m d) ~L(d m)p(m)

IMPLICATIONS Integrate inverted seismic data with rock physics models for quantitative seismic interpretation. Combine rock physics information with seismic information through Bayesian classification techniques. Account for non-unique relationships between rock and elastic properties. Shale Brine sand Brine sand Oil sand Gas sand

SIMULATION OF THE 5 FACIES

INVERTED SECTIONS P-impedance Vp/Vs [ ] km/s x g/cm 3

BAYESIAN CLASSIFICATION FOR MOST LIKELY FACIES Shale Brine sand Brine sand Oil sand Gas sand P(m d) = P(m)P(d m) P(d) P(m d) P(m)P(d m) P(c j d) = P(c j )P(d c j ) P(c j d) > P(c u d) for all j u. Shale Brine sand Brine sand Oil sand Gas sand

BAYESIAN CLASSIFICATION AND PROBABILISTIC MODELS 17 = Shale 17 = Shale 9-16 = Sand, 9-16 oil to = brine Sand, oil brine Probability 1-8 Sand, gas 1-8 = Sand, brine gas to brine 17 = Shale 17 = Shale 9-16 = Sand, o brine 9-16 = Sand, 1-8 oil to = brine Sand, ga brine 1-8 = Sand, gas to brine

BAYESIAN CLASSIFICATION AND PROBABILISTIC MODELS Shale 17 = Shale Brine sand Brine sand 9-16 = Sand, oil to brine Oil sand Gas sand 1-8 = Sand, gas to brine

BAYESIAN CLASSIFICATION AND PROBABILISTIC MODELS log(probability) log(probability) log(probability)

SUMMARY Current research activities in Reservoir characterization Digital rock physics Dispersion and attenuation modeling Probabilistic RPTs Incoming students will take part in these continuing and in new areas Collaborator, Nicola Tisato, is currently building his laboratory, to be and running sometime this year Integrating his work with EDGER work is in the plans 31