Published October 24, 2019 | Version Supplemental Material
Journal Article Open

Similar scaling laws for earthquakes and Cascadia slow-slip events

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon University of Cambridge
  • 3. ROR icon Laboratoire de Géologie de l'École Normale Supérieure
  • 4. ROR icon Jet Propulsion Lab
  • 5. ROR icon École Polytechnique

Abstract

Faults can slip not only episodically during earthquakes but also during transient aseismic slip events, often called slow-slip events. Previous studies based on observations compiled from various tectonic settings have suggested that the moment of slow-slip events is proportional to their duration, instead of following the duration-cubed scaling found for earthquakes. This finding has spurred efforts to unravel the cause of the difference in scaling. Thanks to a new catalogue of slow-slip events on the Cascadia megathrust based on the inversion of surface deformation measurements between 2007 and 2017, we find that a cubic moment–duration scaling law is more likely. Like regular earthquakes, slow-slip events also have a moment that is proportional to A^(3/2), where A is the rupture area, and obey the Gutenberg–Richter relationship between frequency and magnitude. Finally, these slow-slip events show pulse-like ruptures similar to seismic ruptures. The scaling properties of slow-slip events are thus strikingly similar to those of regular earthquakes, suggesting that they are governed by similar dynamic properties.

Additional Information

© The Author(s), under exclusive licence to Springer Nature Limited 2019. Received: 31 August 2018. Accepted: 1 August 2019. Published online: 23 October 2019. This study was funded by NSF award EAR-1821853. S.M. is currently supported by a postdoctoral fellowship from CNES. We thank J. Gomberg for discussion and for providing a revised version of the catalogue of tremor durations presented in ref. 10. We thank R. Burgmann for comments that helped to improve the study. Author Contributions: S.M., A.G. and J.-P.A. designed the study, interpreted the results and wrote the manuscript; S.M. and A.G. performed the computations. J.-P.A. defined the scope of the study. Data availability: The durations and moments estimated in this study are listed in Extended Data Table 1 and in the Source Data of Fig. 3. The slip model of Michel et al., which is used as input in this study is available at: ftp://ftp.gps.caltech.edu/pub/avouac/Cascadia_SSE_Nature/Data_for_Nature/ The authors declare no competing interests. Peer review information: Nature thanks Roland Burgmann, Ken Creager and the other, anonymous, reviewer(s) for their contribution to the peer review of this work.

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Additional details

Identifiers

Eprint ID
97594
Resolver ID
CaltechAUTHORS:20190801-132601461

Funding

NSF
EAR-1821853
Centre National d'Études Spatiales (CNES)

Dates

Created
2019-10-23
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Division of Geological and Planetary Sciences (GPS)