Microseismic Monitoring and Geomechanical Modelling of CO2 - bris
Microseismic Monitoring and Geomechanical Modelling of CO2 - bris
Microseismic Monitoring and Geomechanical Modelling of CO2 - bris
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CHAPTER 6.<br />
GENERATING ANISOTROPIC SEISMIC MODELS BASED ON GEOMECHANICAL SIMULATION<br />
based 3rd order elasticity tensors (e.g., Prioul et al., 2004), <strong>and</strong> continuum effective medium modelling<br />
(e.g., Sayers <strong>and</strong> Kachanov, 1995).<br />
In seismology it is assumed that waves are elastic. As such, the relationship between stress <strong>and</strong><br />
strain for the infinitesimal deformation caused by the passage <strong>of</strong> a seismic wave can be described via<br />
the linear generalised Hooke’s law,<br />
σ ij = C ijkl ε kl , (6.1)<br />
where σ <strong>and</strong> ε are the symmetric 3×3 stress <strong>and</strong> strain tensors, <strong>and</strong> C is the 3×3×3×3 elastic stiffness<br />
tensor. As discussed in Chapter 3, the velocity <strong>of</strong> a seismic wave propagating in any direction through<br />
an elastic media can be calculated from the 21 independent components (although the 4th order<br />
tensor has 81 elements, symmetry arguments reduce the number <strong>of</strong> independent components to 21)<br />
that describe the stiffness tensor. Hence, whether we are using ray tracing or more complex techniques<br />
such as finite element or finite difference, if we are to predict the change in seismic properties caused<br />
by stress, we must be able to determine C as a function <strong>of</strong> σ (or ε). Two models that are capable <strong>of</strong><br />
doing this are discussed below.<br />
6.2.1 3rd-order nonlinear elasticity<br />
Prioul et al. (2004) develop a stress-dependent rock physics model that is capable <strong>of</strong> including the<br />
effects <strong>of</strong> anisotropy <strong>and</strong> non-hydrostatic stress fields. In a simplified form this model has become<br />
immensely popular with the oil industry in the form <strong>of</strong> the R-factor <strong>of</strong> Hatchell <strong>and</strong> Bourne (2005).<br />
The formulations for nonlinear elasticity include cubic (3rd-order) terms that account for the change<br />
in stiffness with stress. By assuming that the 3rd-order terms are isotropic, the following equations<br />
can be generated for the elastic stiffness as a function <strong>of</strong> strain,<br />
C 11 ≃ C11 0 + C 111 ε 11 + C 112 (ε 22 + ε 33 ), (6.2)<br />
C 22 ≃ C11 0 + C 111 ε 22 + C 112 (ε 22 + ε 33 ),<br />
C 33 ≃ C33 0 + C 111 ε 33 + C 112 (ε 22 + ε 33 ),<br />
C 12 ≃ C12 0 + C 112 (ε 11 + ε 22 ) + C 123 ε 22 ,<br />
C 13 ≃ C13 0 + C 112 (ε 11 + ε 33 ) + C 123 ε 22 ,<br />
C 23 ≃ C13 0 + C 112 (ε 22 + ε 33 ) + C 123 ε 22 ,<br />
C 66 ≃ C66 0 + C 144 ε 33 + C 155 (ε 11 + ε 22 ),<br />
C 55 ≃ C55 0 + C 144 ε 22 + C 155 (ε 11 + ε 33 ),<br />
C 44 ≃ C44 0 + C 144 ε 11 + C 155 (ε 22 + ε 33 ),<br />
where<br />
C 144 = (C 112 − C 123 )/2, (6.3)<br />
C 155 = (C 111 − C 112 )/4.<br />
The tensor C 0 describes the elastic stiffness (in Voigt notation) <strong>of</strong> the rock at reference stress<br />
state (commonly, but not necessarily, zero stress). The stress dependent behaviour <strong>of</strong> the rock is then<br />
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