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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6.3. A MICRO-STRUCTURAL MODEL FOR NONLINEAR ELASTICITY<br />
<strong>and</strong> the partial derivatives for C ii (i ≥ 4) terms are<br />
∂C 44<br />
∂α 11<br />
= − 4f 9 (Sr 44 + α 22 + α 33 + 4f 9 αm ) −2<br />
∂C 44<br />
∂α 22<br />
= −(1 + 4f 9 )(Sr 44 + α 22 + α 33 + 4f 9 αm ) −2<br />
∂C 44<br />
∂α 33<br />
= −(1 + 4f 9 )(Sr 44 + α 22 + α 33 + 4f 9 αm ) −2<br />
∂C 55<br />
∂α 11<br />
= −(1 + 4f 9 )(Sr 55 + α 11 + α 33 + 4f 9 αm ) −2<br />
∂C 55<br />
∂α 22<br />
= − 4f 9 (Sr 55 + α 11 + α 33 + 4f 9 αm ) −2<br />
∂C 55<br />
∂α 33<br />
= −(1 + 4f 9 )(Sr 55 + α 11 + α 33 + 4f 9 αm ) −2<br />
∂C 66<br />
∂α 11<br />
= −(1 + 4f 9 )(Sr 66 + α 11 + α 22 + 4f 9 αm ) −2<br />
∂C 66<br />
∂α 22<br />
= −(1 + 4f 9 )(Sr 66 + α 11 + α 22 + 4f 9 αm ) −2<br />
∂C 66<br />
∂α 33<br />
= − 4f 9 (Sr 66 + α 11 + α 22 + 4f 9 αm ) −2 . (6.32)<br />
This method finds the best fitting values <strong>of</strong> α at a given B N /B T value. I found that when<br />
B N /B T was included in the Newton-Raphson scheme, it was seldom possible to find stable, convergent<br />
solutions: stationary points in the objective function were too close to the desired solution. Therefore<br />
a grid search was performed over B N /B T , <strong>and</strong> for each B N /B T value the Newton-Raphson approach<br />
was used to find α. These α values were used to back-calculate velocities, <strong>and</strong> the value <strong>of</strong> B N /B T<br />
that, in conjunction with the α values computed from it, minimised the misfit between back-calculated<br />
<strong>and</strong> observed velocities was selected as the most appropriate. This approach is illustrated in Figure<br />
6.3.<br />
The results <strong>of</strong> this inversion for the samples from the Clair reservoir are shown in Figure 6.4.<br />
Figure 6.5 shows the optimum values <strong>of</strong> B N /B T<br />
determined via this method. We also perform the<br />
inversion for Berea (Lo et al., 1986) <strong>and</strong> Penrith (Sayers, 2002) s<strong>and</strong>stone samples. Because EBSD<br />
<strong>and</strong> XRTG information is not available for these samples, S r is determined from the behaviour <strong>of</strong> the<br />
samples at high pressure following MacBeth (2004). The results are shown in Figure 6.6, with B N /B T<br />
plotted in Figure 6.7. At high pressures the observed stiffness tensors become close to S r , hence α<br />
becomes small <strong>and</strong> our inversion for B N /B T becomes less reliable. This problem is not encountered<br />
by the Clair samples, where the observed stiffness is always well below S r .<br />
Figures 6.5 <strong>and</strong> 6.7 give an indication as to how appropriate the scalar crack assumption is.<br />
For a flat crack with no infill, equation 6.15 suggests that B N /B T should be between 0.8 <strong>and</strong> 1,<br />
depending on the Poisson’s ratio <strong>of</strong> the background matrix. Although there is some spread outside<br />
these bounds, the majority <strong>of</strong> inverted B N /B T values are found close to this range, indicating that the<br />
scalar crack assumption is appropriate. It is also worth noting that there appears to be no systematic<br />
variation <strong>of</strong> B N /B T with pressure, which is implicitly predicted by the scalar crack assumption, further<br />
strengthening our confidence in making it.<br />
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