Quantitative implementation of Preisach-Mayergoyz space to find static and dynamic elastic moduli in rock

被引:76
作者
Guyer, RA
McCall, KR
Boitnott, GN
Hilbert, LB
Plona, TJ
机构
[1] UNIV NEVADA, DEPT PHYS, RENO, NV 89557 USA
[2] UNIV CALIF BERKELEY, DEPT MAT SCI & MINERAL ENGN, BERKELEY, CA 94720 USA
[3] SCHLUMBERGER DOLL RES CTR, RIDGEFIELD, CT 06877 USA
[4] NEW ENGLAND RES INC, WHITE RIVER JCT, VT 05001 USA
关键词
D O I
10.1029/96JB03740
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
In this paper we describe the analysis of quasi-static stress-strain data using a Preisach-Mayergoyz (PM) [after Preisach, 1935; Mayergoyz, 1985] space picture for the elastic behavior of rock. In contrast to the traditional analytic approach to stress strain (an energy density as a function of the strain invariants), the PM space picture reproduces hysteresis and discrete memory seen in the data. In addition, the PM space picture establishes a relationship between experimental data and a number density rho of microscopic mechanical units within the rock. The density rho allows us to make quantitative predictions of dynamic elastic properties. Determining rho from quasi-static stress-strain data requires us to solve a highly underdetermined inverse problem. We explore the following three methods of solving the inverse problem: simulated annealing, normal modes, and exponential decay. All three methods are tested on a Berea sandstone data set and found to give an excellent description of stress versus strain. Choosing one method, the normal mode method, we analyze quasi-static stress-strain curves on two additional sandstones, namely, another sample of Berea and a sample of Castlegate sandstone. From the density rho for each sample we predict the dynamic modulus as a function of pressure and the nonlinear elastic constants. For each of these cases the agreement between the predictions based on rho and experiment is quite good. We establish that PM space provides a quantitative description of the elastic response of a rock and that PM space may be found by a variety of inversion methods.
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收藏
页码:5281 / 5293
页数:13
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