1. On the Scale‐Dependence of Fault Surface Roughness.
- Author
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Beeler, N. M.
- Subjects
- *
SURFACE roughness , *SHEAR zones , *ANDERSON localization , *FAULT zones , *SURFACE analysis , *EXTRAPOLATION - Abstract
Defining roughness as the ratio of height to length, the standard approach to characterize amplitudes of single fault, joint and fracture surfaces is to measure average height as a function of profile length. Empirically, this roughness depends strongly on scale. The ratio is approximately 0.01 at a few mm but 10× smaller at a few tens of meters. Surfaces are rougher at small scales. However, these conclusions are metric‐dependent. If instead height is averaged over wavelength, roughness is nearly Brown spatial noise, having almost scale‐independent apparent surface height to wavelength ratio. The small deviation from scale‐independence is of the opposite sense than found using the standard metric; surfaces are slightly rougher at long wavelengths. Some natural surfaces may be Brownian within the measurement uncertainties. These contradictions are curiosities of surfaces that have Hurst exponents between 0.5 and 1, as natural fault surfaces do. The wavelength‐based analysis of roughness and how it changes with scale are straight‐forward; a normalized Fourier transform approximately preserves amplitude and its scale dependence in the wavelength domain. Among the conclusions from reconsideration of scale dependence are that the scale dependence is weak and much smaller than that of other fault and shear zone properties. Background and aftershock seismicity, jogs and step‐overs indicate strong localization (smoothing) with slip and scale. The lack of strong scale dependence to surface roughness suggests it is not the dominant control on brittle shear zone evolution. Plain Language Summary: "Surface roughness" is amplitude relative to length of a single surface. Surface roughness is thought to contribute significantly to shear strength. When defined as a ratio of average height to profile length, this roughness of exhumed surfaces is strongly scale dependent. It is approximately 0.01 at a few mm but more than 10× smaller at 10 m. If instead surface roughness is an amplitude to wavelength ratio, the conclusions are different. This ratio is nearly wavelength‐independent; exhumed natural surfaces are nearly Brown spatial noise and are slightly smoother at short wavelength. The apparent contradiction from these two different ratios is a curiosity of surface roughness between self‐similar (scale‐independent height to profile length) and Brownian (scale‐independent height to wavelength). Practically all natural surfaces are in this range. Analysis of surface roughness, its scaling and its extrapolation in scale are straight‐forward with the amplitude to wavelength ratio; a normalized Fourier transform approximately preserves scale dependence and the actual amplitudes and in the spectral domain. When compared with other fault and shear zone properties that indicate localization (smoothing) with slip and scale, the lack of scale dependence to surface roughness suggests it is not the dominant control on shear zone evolution. Key Points: Over the range of observed scales fault surface roughness (a ratio of surface height to length) is not well‐described by a purely fractal modelAmplitude/wavelength of exhumed surfaces is nearly Brown spatial noise, and can be easily extrapolated over large spatial scalesSurface roughness may not be the dominant control on changes in fault properties with scale or slip [ABSTRACT FROM AUTHOR]
- Published
- 2023
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