EGU24-11002, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-11002
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Simulating normal fault interactions during complex seismic sequences in the southern Apennines

Constanza Rodriguez Piceda1, Zoë K. Mildon1, Yifan Yin2, Billy J. Andrews1, Claudia Sgambato3, Martijn van den Ende4, and Jean Paul Ampuero4
Constanza Rodriguez Piceda et al.
  • 1University of Plymouth, School of Geography, Earth and Environmental Sciences, Plymouth, United Kingdom of Great Britain – England, Scotland, Wales (constanza.rodriguezpiceda@plymouth.ac.uk)
  • 2MIT Department of Earth, Atmospheric and Planetary Science, Cambridge, United States
  • 3Birkbeck University of London, London, United Kingdom
  • 4Université Côte d'Azur, Observatoire de la Côte d'Azur, IRD, CNRS, Géoazur, Valbonne, France

Active faults with low extension rates can generate large magnitude earthquakes with severe damages, as exemplified in the southern Apennines (Italy) by the Irpinia earthquake (Mw 6.8) in 1980 and the Val D’Agri earthquake (Mw 7.1) in 1857. These earthquakes occur within a network of faults, and geological evidence (e.g. paleoseismic trenching) suggest that earthquake activity varies from decennial to millennial time scales on such fault systems. Therefore, improving our understanding and forecasting capabilities of seismic sequences in these areas is crucial. However, studying fault behaviour in slowly deforming regions can often prove challenging due to the long recurrence intervals and low slip rates of these faults, which results in limited instrumental, historical and paleoseismological records.

To address this issue, we use physics-based numerical models, since they allow for controlled experiments that can span thousands of years with relatively low computational costs, thus they are valuable tools to investigate the causal dynamics between seismic events. Here, we model a system of NW-SE oriented normal faults in the southern Apennines, accounting for the variable slip rates and geometry of the faults. The study region is characterized by areas with variable number of across-strike faults, thus it is suitable to study the effects of fault network geometry (across-and along-strike interaction) on the seismic cycle and earthquake statistics (e.g. recurrence time, coefficient of variation) of a geologically realistic fault network. We use the boundary-element code QDYN which incorporates rate-and-state friction and elastic interactions to examine relevant inputs for seismic hazard assessment, including inter-event time within and between faults, magnitude-frequency distribution, and nucleation location. We are able to simulate spontaneous ruptures following power-law relationships of frequency-magnitude distribution. Differences in the recurrence time (periodic vs. aperiodic cycles) and rupture extent (characteristic vs. non-characteristic seismicity) in the fault planes seem to correlate with the number of faults that exist across strike. Our simulations demonstrate how quasi-dynamic earthquake simulators can provide insights into how fault network geometry impacts earthquake occurrence and seismic hazard assessment.

How to cite: Rodriguez Piceda, C., Mildon, Z. K., Yin, Y., Andrews, B. J., Sgambato, C., van den Ende, M., and Ampuero, J. P.: Simulating normal fault interactions during complex seismic sequences in the southern Apennines, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-11002, https://doi.org/10.5194/egusphere-egu24-11002, 2024.