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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8.2. MODEL DESCRIPTION<br />
Unit E (GPa) ν ρ (kg/m 3 ) Φ Layer top (m) Layer base (m)<br />
Overburden 5.0 0.25 2000 0.2 0 1210<br />
Watrous 14.0 0.23 2000 0.1 1210 1410<br />
Marly Evaporite 24.0 0.34 2700 0.05 1410 1430<br />
Reservoir 14.5 0.31 2200 NA 1430 1470<br />
Frobisher Evaporite 24.0 0.34 2700 0.05 1470 1490<br />
Underburden 20.0 0.25 2500 0.1 1490 2490<br />
Table 8.2: Material parameters for the units <strong>of</strong> the Weyburn geomechanical model. All layers are<br />
saturated with water with K=2.2GPa <strong>and</strong> ρ=1100kg/m 3 , except the reservoir, whose porosity<br />
<strong>and</strong> saturation are determined by the fluid-flow simulation.<br />
coarsening away from the wells. The different reservoir units are too thin to model separately, because<br />
as the aspect ratios <strong>of</strong> the elements become too high, so the solutions become unstable. One solution<br />
would be to reduce the mesh spacing in the x <strong>and</strong> y directions, allowing for a reduction in mesh<br />
spacing in the z direction. However, this would significantly add to the computation time <strong>of</strong> the<br />
models. Average material values across the reservoir are used instead. The top <strong>of</strong> the reservoir is at<br />
1430m. The overburden is modelled to the surface, the underburden is modelled to a depth <strong>of</strong> 2480m.<br />
The non pay rocks are divided into 4 units: the evaporite units bounding the reservoir, the overlying<br />
Watrous shale, while the remainder <strong>of</strong> the overburden above the Watrous, <strong>and</strong> the underburden below<br />
the Frobisher evaporite are modelled with uniform representative properties.<br />
8.2.3 Material properties<br />
The material properties for each unit are given in Table 8.2, based on core sample work by Jimenez<br />
Gomez (2006) <strong>and</strong> Chalaturnyk (pers. comm. 2007 ). The boundary conditions are set as for all the<br />
models in Chapter 5, where the top <strong>of</strong> the model is a free surface. The planes at the sides <strong>and</strong> base <strong>of</strong><br />
the model are prevented from moving in a direction normal to the boundary, although they are free<br />
to move within the plane <strong>of</strong> the boundary (i.e. at the x − z boundary, nodes can move vertically <strong>and</strong><br />
horizontally in the x direction, but not in the y direction).<br />
8.2.4 Rock physics properties<br />
To predict the changes in seismic properties as outlined in Chapters 6 <strong>and</strong> 7 the crack density <strong>and</strong><br />
aspect ratio parameters must be calculated using ultrasonic velocity measurements. The data that<br />
I use are taken from Brown (2002), who performed ultrasonic velocity measurements on Vuggy <strong>and</strong><br />
Marly core samples with variations in the applied hydrostatic stress (Figure 8.3). Brown (2002) only<br />
makes measurements along one axis, so it is only possible to invert for an isotropic rock. I use the<br />
method outlined in Chapter 6 to invert these measurements for the rock physics parameters, given<br />
in Table 8.3. The values fit comfortably within the global trends identified during calibration with<br />
literature samples given in Chapter 6. A comparison between modelled <strong>and</strong> observed velocities is<br />
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