Analogue modeling of the collapse of non-homogeneous granular slopes along weak horizons
2014 (English)In: Tectonophysics, ISSN 0040-1951, E-ISSN 1879-3266, Vol. 632, 76-95 p.Article in journal (Refereed) Published
In this study, we use results of analogue models to investigate the effect of the orientation, location and thickness of a weak horizon on the stability/failure, kinematics and internal deformation of a granular slope. The models are systematically designed to simulate the collapse of non-homogeneous granular slopes by focusing on the spatial and temporal distribution of their internal deformation. Model results show that the presence of a weak horizon embedded within the granular slope has a significant influence on the granular failure which is accommodated through different generation pulses that successively decrease in volume. However, the dip and stratigraphic location of the weak horizon dictate whether the weak horizon plays a role during the failure or not. When the main failure surface is contained within a weak horizon, the dip and thickness of the weak horizon have a positive effect on the displacement of the failure mass, whereas a shallow-located weak horizon causes larger displacement of the failure mass during the collapse of granular slopes. In addition, the collapse of granular slopes results in formation of different-generation normal faults and shortening structures (folds and thrusts) within the failure mass. The first-generation normal faults with a steep dip (about 60º) cut across the entire stratigraphy of the slope, whereas the later-generation normal faults with a gentle dip (about 40º) cut across the shallow units. The distribution of these internal structures within the failure mass is affected significantly by the orientation, location and thickness of the weak horizon.
Place, publisher, year, edition, pages
2014. Vol. 632, 76-95 p.
Non-homogeneous granular slopes; Analogue models; Landslides; Internal deformation; Weak horizon
Research subject Earth Science with specialization in Mineral Chemistry, Petrology and Tectonics
IdentifiersURN: urn:nbn:se:uu:diva-223785DOI: 10.1016/j.tecto.2014.06.007ISI: 000343378500007OAI: oai:DiVA.org:uu-223785DiVA: diva2:714102