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AVO analysis and Impedance Inversion Okey Ileka 1
AVO analysis and Impedance Inversion Okey Ileka 1 AVO Analysis • • • • • • • • Introduction AVO Pre-processing AVO modeling AVO parameters AVO crossplot analysis AVO attributes Some application of AVO Probabilistic AVO analysis 2 Impedance Inversion • • • • • • Post stack 1D Impedance Inversion Far-offset elastic Impedance Lambda-mu-rho estimation P to S elastic Inversion Anisotropic elastic Impedance Interpretation of Rock physics template 3 Introduction • AVO is the amplitude variation with offset 4 Introduction Castagna lecture notes 5 Introduction Castagna lecture notes 6 Simplified Shuey (1985) Form of the Richards and Frazier (1976) Approximation R(θ ) ≈ A + B sin θ 2 A = Rp B ≈ R p − 2 Rs 1 ⎛⎜ ΔV p Δρ ⎞⎟ A≈ + ⎜ 2 ⎝ Vp ρ ⎟⎠ Vs Δρ 1 ΔV p Vs ΔVs B ≈ −2 2 + −4 2 Vp ρ 2 Vp V p 7 Vs 2 2 Third Order Approximation R(θ ) ≈ A + B sin θ + C sin θ tan θ 2 1 ⎛⎜ ΔV p Δρ ⎞⎟ A= + 2 ⎜⎝ V p ρ ⎟⎠ 2 2 1 ΔV p C≈ 2 Vp 1 Δρ A−C ≈ 2 ρ Castagna lecture note 8 Hiltermann Approximation 6 474 8 2 2 R(θ ) ≈ A cos θ + 2.25Δσ sin θ G G = A+ B Castagna lecture note 9 AVO preprocessing Castagna lecture notes 10 11 Castagna lecture note Factors that amplitudes • Earth effects • Acquisition related effects • Noise 12 Earth effects • • • • • • • • Spherical divergence Absorption Transmission losses Interbed multiples Converted phases Tunning effect Anisotropy structure 13 Acquisition-related effects and noise • Acquisition-related effects • Source reciever arrays • Reciever sensitivity • Noise • Source generated noise • Coherent or random noise 14 AVO Pre-processing • Spiking deconvolution and wavelet processing • Spherical divergence correction • Surface consistent amplitude balancing • Multiple removal • NMO correction • DMO correction • Pre-stack migration 15 AVO preprocesing Castagna lecture notes 16 Castagna lecture notes 17 AVO modeling 18 Physical Interpretation R (θ ) ≈ A + B sin θ 2 Castagna lecture notes 19 (Russel, 1999) AVO parameters 20 21 Castagna lecture notes AVO crossplot 22 From Simm et al., 2000 Castagna lecture notes 23 AVO attributes 24 AVO Indicators/Attributes • • • • • • • Intercept Gradient Near and far stacks Curvature CDP stack Change in Poisson’s ratio Fluid Factor Castagna lecture notes • • • • • Intercept minus Gradient Intercept plus Gradient Intercept times Gradient Rp-Rs P and S wave velocity contrast • Density Contrast • Amoco Indicator F(F-N) • Lamba-mu-rho 25 Calculated AVO Attributes A = intercept B = gradient r² = correlation A×B (A + B)/2 ~ Rp - Rs (A – B)/2 ~ Rs A = intercept B = gradient C = curvature r² = correlation A×B (A + B)/2 ~ Rp - Rs (A – B)/2 ~ Rs A–C NI = normal intercept PR = Poisson reflectivity r² = correlation NI × PR Castagna lecture notes Shuey 2 Term RC (θ) = A + B (sin²θ) Shuey 3 Term RC (θ) = A + B (sin²θ) + C (sin²θ)(tan²θ) Verm-Hilterman RC (θ) = NI(cos²θ) + PR(sin²θ) 26 Roden, 2005 Some application of AVO • Residual gas saturation (converted waves) • Flat spot analysis • Overpressure detection • Density estimation 27 Probabilistic AVO analysis • In probabilistic AVO analysis the AVO parameters and attributes are assigned probability density function (PDF) or cumulative density function (CDF) 28 Impedance Inversion • The goal of geophysical inversion is to estimate model parameter from observed data 29 Impedance Inversion • • • • • • Post stack 1D Impedance Inversion Far-offset elastic Impedance Lambda-mu-rho estimation P to S elastic Inversion Anisotropic elastic Impedance Interpretation of Rock physics template 30 Poststack 1D impedance Inversion • Inversion of near stack traces 31 Acoustic Impedance Inversion Near Angle Stack Sonic,Density Logs tie Wavelet tie Bandlimited Inversion Horizons AI Earth Model Trend Model Merged AI Castagna lecture note 32 Sena, 1997 Far offset elastic Impedance • Inversion of far offset traces 33 The Elastic Impedance E = Vpα Vsβ ργ α = 1/cos2θ β = -8(Vs/Vp)2sin2θ γ = 1 + β/2 Castagna lecture notes Sena, 1997 34 Elastic Impedance Inversion Far Angle Stack Sonic,Shear Sonic and Density Logs tie Wavelet tie Bandlimited Inversion Horizons EI Earth Model Trend Model Merged EI Castagna lecture note 35 Sena, 1997 Lambda Rho estimation Hilterman’s lecture note 36 P –to- S elastic Inversion 37 Reflection Coefficients: Angle vs. Offset σ σ σ σ 38 Stewart and Gasier lecture note P-S Reflection Coefficient (Aki & Richards, 1980) Rps First Order Relative S-velocity change Stewart and Gasier lecture note 39 Relative density change Anisotropic elastic Inversion 40 Anisotropy Hilterman course notes 41 Anisotropic Inversion Hilterman course notes 42 Interpretation of Rock Physics Template • The rock physics template is based on a compiled catalog or atlas of RPT’s calculated by a rock physics expert. • The seismic interpreter can interpret elastic inversion results without in-depth knowledge about rock physics theory 43 • Thank you 44