EGU25-11895, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-11895
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Tuesday, 29 Apr, 15:30–15:40 (CEST)
 
Room D2
Detecting hidden seismic swarms using a 300 nodal long-term array
Quentin Higueret1, Florent Brenguier1, Mordret Aurélien2, Yixiao Sheng3, Frank Vernon4, Dan Hollis4, Coralie Aubert1, and Yehuda Ben-Zion5
Quentin Higueret et al.
  • 1ISTerre, University Grenoble Alpes, France
  • 2Geological Survey of Denmark and Greenland (GEUS), Denmark
  • 3USTC, University of Science and Technology of China, China
  • 4Scripps Institution of Oceanography, University of California, United States
  • 5Department of Earth Sciences, University of Southern California, United States

Earthquake swarms may be driven by slow processes within fault zones, such as fluid migration, or silent slip events. A prominent example is the 2024 Mw 7.5 Noto earthquake in Japan, which was preceded by a significant seismic swarm, likely triggered by upward fluid migration (Wang et al. 2024). These swarms provide insights into dynamic fault processes, and there is thus a need to detect smaller earthquakes for a clearer understanding of the temporal evolution of seismicity and the mechanisms driving fault activity (Shearer et al., 2022).
To address these challenges, we used a dense array of 300 seismic nodes deployed for three years at the Piñon Flat Observatory (South.Cal.) along the San Jacinto Fault, one of the most seismically active areas in California. Using advanced slant stacking techniques tuned to the fault geometry at crustal P- and S-wave velocities, we significantly enhanced our detection capabilities down to approximately magnitude -2. By detecting four times as many events as the standard USGS catalog, this allowed us to highlight three distinct swarm episodes that were not identified before. These episodes exhibit a characteristic progression: an initial activation phase, a steady state culminating in a peak, followed by a final decay.
We further investigate the magnitude distribution and spatial migration to propose a possible driving mechanism. This approach can be extended to other fault zones to unveil hidden fault activity.

How to cite: Higueret, Q., Brenguier, F., Aurélien, M., Sheng, Y., Vernon, F., Hollis, D., Aubert, C., and Ben-Zion, Y.: Detecting hidden seismic swarms using a 300 nodal long-term array, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11895, https://doi.org/10.5194/egusphere-egu25-11895, 2025.