Journal article
Scaling of viscous shear zones with depth-dependent viscosity and power-law stress-strain-rate dependence
- Abstract:
- One of the unresolved questions concerning fault deformation is the degree and cause of localization of shear at depth beneath a fault. Geologic observations of exhumed shear zones indicate that while the motion is no longer planar, it can still be localized near the down-dip extension of the fault; however, the degree of localization is uncertain. We employ simple analytic and numerical models to investigate the structural form of distributed shear beneath a strike-slip fault, and the relative importance of the physical mechanisms that have the potential to localize a shear zone. For a purely depth dependent viscosity, η = η0 exp (-z/z0), we find that a shear zone develops with a half-width δw ~ √z0 for small z0 at the base of the layer, where lengths are non-dimensionalized by the layer thickness (d km). Including a non-linear stress-strain-rate relation (ε ∝ σn) scales δw by 1/√n, comparable to deformation length scales in thin viscous sheet calculations. We find that the primary control on the shear-zone width is the depth dependence of viscosity that arises from the temperature dependence of viscosity and the increase in temperaturewith depth. As this relationship is exponential, scaling relations give a dimensional half-width that scales approximately as where T1/2 (K) is the temperature at the midpoint of the layer, R (J mol-1 K-1) the gas constant, Q (J mol-1) the activation energy and β (K km-1) the geothermal gradient. This relation predicts the numerical results for the parameter range consistent with continental rheologies to within 2-5 per cent and shear-zone half-widths from 2 to 6 km. The inclusion of shear-stress heating reduces δw by only an additional 5-25 per cent, depending on the initialwidth of the shear zone. While the width of the shear zone may not decrease significantly, local temperature increases from shear-stress heating range from 50 to 300 °C resulting in a reduction in viscosities beneath the fault of several orders of magnitude and a concomitant reduction in the stresses needed to drive the motion.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, pdf, 8.2MB, Terms of use)
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- Publisher copy:
- 10.1093/gji/ggv143
Authors
- Publisher:
- Oxford University Press
- Journal:
- Geophysical Journal International More from this journal
- Volume:
- 202
- Issue:
- 1
- Pages:
- 242-260
- Publication date:
- 2015-04-24
- Acceptance date:
- 2015-03-27
- DOI:
- EISSN:
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1365-246X
- ISSN:
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0956-540X
- Keywords:
- Pubs id:
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pubs:550973
- UUID:
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uuid:eaf71ae3-14ca-40f3-8a00-f4e7a7869185
- Local pid:
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pubs:550973
- Source identifiers:
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550973
- Deposit date:
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2016-06-16
- ARK identifier:
Terms of use
- Copyright holder:
- James Moore and Barry Parsons
- Copyright date:
- 2015
- Notes:
-
This is an Open Access article
distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited
- Licence:
- CC Attribution (CC BY)
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