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Gassmann's equation : ウィキペディア英語版
Gassmann's equation
The Gassmann equation is used in geophysics and its relations are receiving more attention as seismic data are increasingly used for
reservoir monitoring. The Gassmann equation is the most common way of performing a fluid substitution model from one known parameter.
==Procedure==
These formulations are from Avseth ''et al.'' (2006).〔Avseth, P, T Mukerji & G Mavko (2006), Quantitative seismic interpretation, Cambridge University Press, 2006.〕
Given an initial set of velocities and densities, V_^, V_^, and \rho ^ corresponding to a rock with an initial set of fluids, you can compute the velocities and densities of the rock with another set of fluid. Often these velocities are measured from well logs, but might also come from a theoretical model.
Step 1: Extract the dynamic bulk and shear moduli from V_\mathrm^, V_\mathrm^, and \rho ^:
:K_\mathrm^ = \rho \left ((V_\mathrm^)^-\frac(V_\mathrm^)^ \right)
:\mu_\mathrm^ = \rho (V_\mathrm^)^
Step 2: Apply Gassmann's relation, of the following form, to transform the saturated bulk modulus:
:\frac}^}-\frac}^)}=\frac}^}-\frac}^)}
where K_\mathrm^ and K_\mathrm^ are the rock bulk moduli saturated with fluid 1 and fluid 2, and K_\mathrm^ and K_\mathrm^ are the bulk moduli of the fluids themselves.
Step 3: Leave the shear modulus unchanged (rigidity is independent of fluid type):
:\mu_\mathrm^=\mu_\mathrm^
Step 4: Correct the bulk density for the change in fluid:
: \rho^= \rho^+\phi (\rho_\mathrm^ -\rho_\mathrm^)
Step 5: recompute the fluid substituted velocities
:V_\mathrm^=\sqrt \frac+\frac \mu_\mathrm^}^ = \sqrt \frac}{\rho^{(2)}}

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