EGU23-7357
https://doi.org/10.5194/egusphere-egu23-7357
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Numerical modelling of flanking structures in layered viscous media

Marcin Dabrowski
Marcin Dabrowski
  • Computational Geology Laboratory, Polish Geological Institute - National Research Institute, Wrocław, Poland (mdabr@pgi.gov.pl)

Flow perturbation can deflect the layering of the host rock around slip surfaces in shear zones resulting in the development of flanking structures. The details of flanking structure geometry can provide important clues about shear sense, flow kinematics, and finite strain, although not without ambiguities. The developing structures share similarities to fault-related folds that play an important role in sedimentary basins.

Mechanical anisotropy has been shown to have a major influence on both the slip rate and flow perturbation. Willis (1964) derived an analytical solution for an elliptical inclusion embedded in a homogeneous anisotropic elastic matrix subject to a uniform load in the far field. The solution can be reduced to the case of an incompressible viscous medium and an arbitrarily oriented inviscid slit (slip line). The reduced solution, which is exact for the initial state of homogeneous planar anisotropy, provides useful insights into the initial stages of deformation and it can be used to approximately study finite strain deformation of a power-law host. However, anisotropic fluids such as ductilely deforming foliated rocks keep a ‘memory’ of deformation due to their evolving microstructure, which affects the flow field. In this study, I will use different numerical modeling techniques to examine the impact of host layering on the perturbing flow and structure development around a slip surface in shear zone.

How to cite: Dabrowski, M.: Numerical modelling of flanking structures in layered viscous media, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-7357, https://doi.org/10.5194/egusphere-egu23-7357, 2023.