Brian Russell* and Tad Smith Hampson-Russell, A CGGVeritas Company * Adjunct Professor, University of Calgary

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The relationship between dry rock bulk modulus and porosity an empirical study Brian Russell* and Tad Smith Hampson-Russell, A CGGVeritas Company * Adjunct Professor, University of Calgary

Introduction There are various approaches to computing dry as a function of porosity, and thus inferring changes in fluid content as a function of porosity. One common approach is the pore space stiffness method, and a second approach uses critical porosity. Mavko and Mukerji (1995) propose a useful template for plotting the various porosity functions. Using a dataset collected by De Hua Han, and the Mavko-Mukerji template, we will evaluate the suitability of each method. Using the Han dataset, we will also derive an empirical relationship between pore space stiffness and pressure.

Pore space stiffness To model dry rock bulk modulus at different porosities, we can use pore space stiffness, the inverse of the dry rock space compressibility at a constant pore pressure, written: dry 1 1 = +, where : dry m = dry rock bulk modulus, = mineral = pore space stiffness, and = porosity. m bulk modulus, If we calculate dry directly, and divide through by m, this equation can be re-written as: dry m 1 =, 1+ k where : k = m.

Constant pore space stiffness k = 0.01 k = 0.05 k = 0.1 k = 0.5 k = 0.3 Note that a family of constant k curves can be drawn on a plot of dry / m versus porosity, allowing us to estimate trends from rock physics measurements.

Voigt and Reuss bounds Mavko and Mukerji,(1995), discuss other models such as the Voigt (high bound) and Reuss (low bound) averages, given by: Voigt dry Voigt = m air m 1 dry ( 1 ) + ( 1 ) = Ruess dry 1 = + m The critical porosity model (Nur, 1992) is given by: dry m air 1 Voigt dry 1 1 1, where = c m c = c 0 m critical porosity. c separates load-bearing sediments ( < c ) from suspensions ( > c ) and is like a scaled Voigt model.

The Mavko-Mukerji Template Mavko and Mukerji devised a template which plotted dry / m against porosity, and with which the various models could be compared. Here is their template with the different curves annotated. Critical Porosity Reuss c Voigt Constant k = / m max

Han s Dataset To test the various models, Mavko and Mukerji (1995) used a dataset collected by De Hua Han for his 1986 Ph.D. thesis. This dataset was graciously provided to us by Dr. Han of the University of Houston. Han s dataset consisted of a number of sandstones of various porosities and clay content, measured at different pressures and saturations. Han was able to derive empirical formulae for P and S- wave velocities versus porosity and clay content (Han et al., 1986). From Han s measurements, Mavko and Mukerji (1995) used the 10 clean sandstones at 40 MPa and a single clean sandstone at 5, 10, 20, 30, and 40 MPa.

Data points used by Mavko and Mukerji Decreasing Pressure (a) (b) Figure (a) shows the ten clean dry sandstones at a constant pressure of 40 MPa. Figure (b) shows a single clean dry sandstone at pressures of 5, 10, 20, 30, and 40 Mpa. The dotted line is the Voigt limit.

Best fits for constant pressure (a) Figure (a) shows the best pore space stiffness fit ( / m = 0.162 with RMS error = 0.039), and (b) shows the best critical porosity fit ( c = 34.3% with RMS error = 0.058). Based on RMS error, the fit is the best. (b)

Modeling dry versus porosity To model dry at different porosities using pore space stiffness, can be calculated for the in-situ porosity using the original equation: in situ = 1 dry 1 m = in situ 1 dry 1 m 1 Once we have estimated the in-situ value for the pore space stiffness, we can calculate a value for dry at a new porosity at the same pressure using: dry _ new = new + 1 1 m

Modeling μ versus porosity Murphy et al (1993) measured dry and μ for clean quartz sandstones, and found the ratio of dry /μ is constant for varying porosity. We can therefore compute the new value of μ from: μ new = μ in situ dry _ new dry _ in situ The figure on the next slide shows a cross-plot of V P /V S ratio versus P-impedance as a function of porosity and water saturation in a gas-charged sand using the following three assumptions: Biot-Gassmann is used to model fluid changes The pore space stiffness is used to model dry vs porosity change. The above equation is used to model μ vs porosity change.

V P /V S Ratio vs P-Impedance = 50% wet 33% 15% = 5% gas

Variable pressure k = / m decreases Decreasing Pressure c decreases (a) Next, consider the variable pressure case. Figure (a) shows that k = / m decreases as pressure decreases. Figure (b) shows that c also decreases with decreasing pressure. (b)

Variable pressure (a) (b) Han measured pressures of 5, 10, 20, 30, 40 and 50 MPa. Figure (a) shows the optimum pore stiffness fits for 50 MPa (blue) and 5 MPa (red). Figure (b) shows the equivalent c fits.

Variable pressure P(MPa) c RMSE / m RMSE 5 0.289 0.126 0.104 0.094 10 0.311 0.107 0.129 0.076 20 0.329 0.079 0.147 0.055 30 0.338 0.069 0.156 0.044 40 0.343 0.058 0.162 0.039 50 0.348 0.053 0.166 0.038 This table shows the best fits and RMS errors for both models at all pressures. Note that and c increase with increasing pressure and the error is smallest in all cases for.

Variable pressure (a) (b) Here are the plots of / m vs (a) pressure and (b) natural log of pressure. Note that the relationship in (b) shows a good linear fit.

Variable pressure From the previous plot, the best least-squares fit is: m = 0.065 + 0.027 ln( P) From this equation, we can derive the relationship between change in pore space stiffness and pressure: d dp Δ 0.027m = Δ = 0. 027 ΔP P m ΔP P This equation allows us derive constant curves at different pressures than the in-situ pressure, and hence predict a depth variable dry versus porosity relationship.

Carbonate example Finally, Baechle et al. (2006) modeled carbonates using pore space stiffness. They show that dolomites with microporosity (blue points on right) fit the curve k = 0.2 and dolomites with vuggy porosity (red) fit the curve k = 0.1. The dashed line is the critical porosity fit. k = 0.1 k = 0.2 microporosity vuggy porosity Baechle et al. (2006)

Conclusions We have reviewed the two different approaches (pore space stiffness and critical porosity) to model porosity changes in fluid-saturated rocks using the dry rock bulk modulus. When tested using Han s measurements, the pore space stiffness method gave the best fit to the data. We then showed a model incorporating the pore space stiffness method with Biot-Gassmann fluid changes. We next derived an equation that allowed us to calculate pore space stiffness as a function of pressure. Finally, we looked at a carbonate example from the literature using the critical porosity method. Limitations of this study were that only clean sandstones were modeled and that the pore space stiffness method is appropriate only at porosities much less than critical porosity.

References Baechle, G.T., Weger, R., Eberli, G.P., and Colpaert, A., 2006, Pore size and pore type effects on velocity Implications for carbonate rock physics models: Abstract of paper presented at Sound of Geology workshop in Bergen, Norway. Han, D., 1986, Effects of porosity and clay content on acoustic properties of sandstones and unconsolidated sediments: Ph.D. dissertation, Stanford University. Han, D.H., A. Nur, and D. Morgan, 1986, Effects of porosity and clay content on wave velocities in sandstones: Geophysics, 51, 2093-2107. Mavko, G., and T. Mukerji, 1995, Seismic pore space compressibility and Gassmann\'s relation: Geophysics, 60, 1743-1749. Murphy, W., Reischer, A., and Hsu,., 1993, Modulus Decomposition of Compressional and Shear Velocities in Sand Bodies: Geophysics, 58, 227-239. Nur, A., 1992, Critical porosity and the seismic velocities in rocks: EOS, Transactions American Geophysical Union, 73, 43-66.