Evolution of the internal structure of fault zones in three-dimensional numerical models of normal faults

被引:17
|
作者
Schopfer, Martin P. J. [1 ]
Childs, Conrad [1 ]
Walsh, John J. [1 ]
Manzocchi, Tom [1 ]
机构
[1] UCD Sch Earth Sci, Fault Anal Grp, Dublin 4, Ireland
基金
爱尔兰科学基金会;
关键词
Fault zone structure; Fault lenses; Asperity bifurcation; Tip-line bifurcation; Distinct element method;
D O I
10.1016/j.tecto.2015.11.003
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
Fault zone internal structure is characterised by heterogeneous distributions of both continuous (drag, lens rotation) and discontinuous (joints, faults) deformation which cannot be easily modelled using continuum numerical methods. Distinct element method (DEM) models, that exhibit bulk rheologies comparable to rock, demonstrate emergent behaviours that make them ideal for modelling both the nucleation and growth of fault zones. The ability to model fault zones numerically allows extant conceptual models for fault zone evolution based on outcrop studies to be tested, and controls on fault zone structure to be analysed. Three-dimensional DEM models of faults zones in mechanically layered sequences demonstrate that internal fault zone structure is predominantly controlled by the geometry of the initial fault. Whether the initial fault is a segmented array or an irregular surface determines the complexity of structure it will develop as displacement increases. Confining pressure at the time of faulting determines the irregularity of the initial fault array and also the efficiency with which irregularities are incorporated into a fault and subsequently comminuted, leading to a relationship whereby brittle faulting at high confining pressure results in less complex internal fault zone structure than at low confining pressure. (C) 2015 Elsevier B.V. All rights reserved.
引用
收藏
页码:158 / 163
页数:6
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