A Model of Aftershock Migration Driven by Afterslip. Issue 5 (10th March 2018)
- Record Type:
- Journal Article
- Title:
- A Model of Aftershock Migration Driven by Afterslip. Issue 5 (10th March 2018)
- Main Title:
- A Model of Aftershock Migration Driven by Afterslip
- Authors:
- Perfettini, H.
Frank, W. B.
Marsan, D.
Bouchon, M. - Abstract:
- Abstract: Aftershocks region have been extensively reported to expand logarithmically with time. The associated migration velocity is typically of the order of several km/decade but can be much larger, especially when observing early aftershock sequences, seismic swarms, or tremors. We present here a model for the expansion of aftershock zones based on the idea that aftershocks are triggered as afterslip grows with time along the fault. One of the model assumptions is that aftershocks are triggered when a critical level of afterslip is reached. We predict that the migration velocity V p at time t following the mainshock is given by V p = ζ A ′ Δτ × c t, where A ′ is a frictional parameter, Δ τ a characteristic value for the stress perturbation, c the radius of the stress perturbation, and ζ a constant of order unity. The scaling V p ∝ 1 / t implies a logarithmic expansion of the aftershock zone with time. The migration velocities predicted by our model are in quantitative agreement with the observations reported following aftershock sequence of small and large earthquakes in various tectonic settings, seismic swarms, and tremor sequences. Plain Language Summary: Aftershocks are shown to migrate with time away from the rupture area of the mainshock. This migration typically occurs as the logarithm of time. We present here a model based on the idea that afterslip drives aftershocks. The model is able to predict the migration as the logarithm of time, predicting apparentAbstract: Aftershocks region have been extensively reported to expand logarithmically with time. The associated migration velocity is typically of the order of several km/decade but can be much larger, especially when observing early aftershock sequences, seismic swarms, or tremors. We present here a model for the expansion of aftershock zones based on the idea that aftershocks are triggered as afterslip grows with time along the fault. One of the model assumptions is that aftershocks are triggered when a critical level of afterslip is reached. We predict that the migration velocity V p at time t following the mainshock is given by V p = ζ A ′ Δτ × c t, where A ′ is a frictional parameter, Δ τ a characteristic value for the stress perturbation, c the radius of the stress perturbation, and ζ a constant of order unity. The scaling V p ∝ 1 / t implies a logarithmic expansion of the aftershock zone with time. The migration velocities predicted by our model are in quantitative agreement with the observations reported following aftershock sequence of small and large earthquakes in various tectonic settings, seismic swarms, and tremor sequences. Plain Language Summary: Aftershocks are shown to migrate with time away from the rupture area of the mainshock. This migration typically occurs as the logarithm of time. We present here a model based on the idea that afterslip drives aftershocks. The model is able to predict the migration as the logarithm of time, predicting apparent propagation velocities consistent with the observations. The propagation velocity is simply related to the physical parameters of the model. Key Points: Aftershocks are driven by afterslip The model predicts an apparent propagation velocity scales as 1/time We relate the propagation velocity to the physical parameters of the model … (more)
- Is Part Of:
- Geophysical research letters. Volume 45:Issue 5(2018)
- Journal:
- Geophysical research letters
- Issue:
- Volume 45:Issue 5(2018)
- Issue Display:
- Volume 45, Issue 5 (2018)
- Year:
- 2018
- Volume:
- 45
- Issue:
- 5
- Issue Sort Value:
- 2018-0045-0005-0000
- Page Start:
- 2283
- Page End:
- 2293
- Publication Date:
- 2018-03-10
- Subjects:
- aftershocks -- afterslip -- migration -- rate strengthening rheology
Geophysics -- Periodicals
Planets -- Periodicals
Lunar geology -- Periodicals
550 - Journal URLs:
- http://www.agu.org/journals/gl/ ↗
http://onlinelibrary.wiley.com/ ↗ - DOI:
- 10.1002/2017GL076287 ↗
- Languages:
- English
- ISSNs:
- 0094-8276
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 4156.900000
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 17759.xml