HOW DOES A VISCOUS LAYER AFFECT THE MECHANICS AND KINEMATICS OF ACCRETIONARY WEDGES?
In some cases décollements are generated in the vicinity of viscous salt layers, e.g. at the Hellenic subduction zone in the eastern Mediterranean. Here the accretionary wedge – the Mediterranean Ridge, is partly underlying by large evaporite horizons which correlate with a shallow décollement responsible for evolution of the outer prism.
Hence, major aim of this study is to verify the influence of an embedded viscous layer on the mechanics of evolving wedges. An extensive parameter sensitivity study varying the viscosity will enable us to investigate does and how does this parameter control wedge geometry, accretion mode, fault geometry, mass transport pattern and the location of the detachment.
We develop 2D numerical ‘sandbox’ model utilizing the Discrete Element Method to simulate the deformation behaviour of accretionary wedges. A mechanically weaker viscous layer based on the Burger’s Model is embedded in the brittle undeformed ‘sediments’. This viscous rheology describes the creep behaviour of natural rocks. We tested different viscosity values from 5*1016 to 1*1018 Pas to quantify their influence on the wedge kinematics and the development of the detachment.
Within all experiments at least two active detachments develop at different depth generating a down-steeping décollement. So, a temporary decoupling of the viscous layer from the underlying or overlying brittle strata takes place.
References
Burbidge, D. R., Braun, J., 2002. Numerical models of the evolution of accretionary wedges using the distinct element method. Geophys. J. Int., 148, 542-561.
Mulugeta, G., 1988. Modelling the geometry of Coulomb thrust wedges. J. Struct. Geol. 10, 847-859.