Details
Original language | English |
---|---|
Pages (from-to) | 570-582 |
Number of pages | 13 |
Journal | Earth and Planetary Science Letters |
Volume | 284 |
Issue number | 3-4 |
Publication status | Published - 15 Jul 2009 |
Abstract
Although it is well accepted that mass redistribution on Earth's surface due to erosion and sedimentation affects the rate of crustal deformation, the influence of surface processes on the slip behaviour of individual faults remains poorly understood. Here we use the new tool CASQUS, which combines landscape evolution modelling with three-dimensional tectonic models, to investigate how erosion and sediment deposition affect fault behaviour in extensional tectonic regimes. A systematic set of experiments with models consisting of an isostatically responding elastic upper crust containing a single normal fault shows that the slip accumulation on the fault is accelerated by erosion and sedimentation. Depending on fault geometry, extension rate and parameters controlling erosion and sediment deposition, the slip rate of the normal fault is up to ~ 15% higher when surface processes are taken into account. The slip acceleration can be explained by an increase in the differential stress caused by erosion of the fault footwall and sedimentation in the hanging wall, which alter the faulting-induced flexure of the crust. We observe a similar slip rate increase in a more complex model of a growing horst bounded by three faults of different length. Our results show that a positive feedback exists between surface processes and tectonics and imply that geologically derived fault slip rates that integrate over several earthquake cycles may contain a contribution from surface processes.
Keywords
- fault, neotectonics, numerical modelling, slip rate, surface processes
ASJC Scopus subject areas
- Earth and Planetary Sciences(all)
- Geophysics
- Earth and Planetary Sciences(all)
- Geochemistry and Petrology
- Earth and Planetary Sciences(all)
- Earth and Planetary Sciences (miscellaneous)
- Earth and Planetary Sciences(all)
- Space and Planetary Science
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In: Earth and Planetary Science Letters, Vol. 284, No. 3-4, 15.07.2009, p. 570-582.
Research output: Contribution to journal › Article › Research › peer review
}
TY - JOUR
T1 - Slip acceleration on normal faults due to erosion and sedimentation - Results from a new three-dimensional numerical model coupling tectonics and landscape evolution
AU - Maniatis, Georgios
AU - Kurfeß, Daniel
AU - Hampel, Andrea
AU - Heidbach, Oliver
N1 - Funding information: We thank two anonymous reviewers for their constructive reviews, J. Braun for making the CASCADE code available to us and R. Hetzel for critical comments on the manuscript. Funding to A. H. and G. M. was provided by the German Research Foundation (DFG) within the framework of an Emmy-Noether fellowship (grant HA 3473/2-1).
PY - 2009/7/15
Y1 - 2009/7/15
N2 - Although it is well accepted that mass redistribution on Earth's surface due to erosion and sedimentation affects the rate of crustal deformation, the influence of surface processes on the slip behaviour of individual faults remains poorly understood. Here we use the new tool CASQUS, which combines landscape evolution modelling with three-dimensional tectonic models, to investigate how erosion and sediment deposition affect fault behaviour in extensional tectonic regimes. A systematic set of experiments with models consisting of an isostatically responding elastic upper crust containing a single normal fault shows that the slip accumulation on the fault is accelerated by erosion and sedimentation. Depending on fault geometry, extension rate and parameters controlling erosion and sediment deposition, the slip rate of the normal fault is up to ~ 15% higher when surface processes are taken into account. The slip acceleration can be explained by an increase in the differential stress caused by erosion of the fault footwall and sedimentation in the hanging wall, which alter the faulting-induced flexure of the crust. We observe a similar slip rate increase in a more complex model of a growing horst bounded by three faults of different length. Our results show that a positive feedback exists between surface processes and tectonics and imply that geologically derived fault slip rates that integrate over several earthquake cycles may contain a contribution from surface processes.
AB - Although it is well accepted that mass redistribution on Earth's surface due to erosion and sedimentation affects the rate of crustal deformation, the influence of surface processes on the slip behaviour of individual faults remains poorly understood. Here we use the new tool CASQUS, which combines landscape evolution modelling with three-dimensional tectonic models, to investigate how erosion and sediment deposition affect fault behaviour in extensional tectonic regimes. A systematic set of experiments with models consisting of an isostatically responding elastic upper crust containing a single normal fault shows that the slip accumulation on the fault is accelerated by erosion and sedimentation. Depending on fault geometry, extension rate and parameters controlling erosion and sediment deposition, the slip rate of the normal fault is up to ~ 15% higher when surface processes are taken into account. The slip acceleration can be explained by an increase in the differential stress caused by erosion of the fault footwall and sedimentation in the hanging wall, which alter the faulting-induced flexure of the crust. We observe a similar slip rate increase in a more complex model of a growing horst bounded by three faults of different length. Our results show that a positive feedback exists between surface processes and tectonics and imply that geologically derived fault slip rates that integrate over several earthquake cycles may contain a contribution from surface processes.
KW - fault
KW - neotectonics
KW - numerical modelling
KW - slip rate
KW - surface processes
UR - http://www.scopus.com/inward/record.url?scp=67650676741&partnerID=8YFLogxK
U2 - 10.1016/j.epsl.2009.05.024
DO - 10.1016/j.epsl.2009.05.024
M3 - Article
AN - SCOPUS:67650676741
VL - 284
SP - 570
EP - 582
JO - Earth and Planetary Science Letters
JF - Earth and Planetary Science Letters
SN - 0012-821X
IS - 3-4
ER -