Maximum Magnitude of Induced Earthquakes in Rate and State Friction Framework
Abstract
We analyze the evolution of the rupture radius and maximum magnitude (M_(max)) of injection-induced earthquakes on faults obeying rates and state friction. We define the radii of two different slip modes, aseismic (R^a) and seismic slip (R^s), and derive an expression for maximum magnitude evolution. If the flow rate is sufficiently high, the seismic moment grows with the scaled injection volume, Qt/wS, as M∼C_f(Qt/wS)^(3/2), in which C_f depends on the initial stress level, S is storage coefficient, and w is the thickness of the reservoir. These findings are confirmed using numerical simulations conducted with varied initial states. The simulations show that R^s behaves as a rupture arrest radius and R^a behaves as the minimum possible radius of aseismic creep at a given injection volume. The M_(max) evolution curve can be steeper if the fault is slightly critically stressed. A high-flow rate results in frequent seismic events, starting at relatively low-injected volume, which helps track the evolution of M_(max), providing a way to anticipate the risk of a large event. Conversely, a low-flow rate allows for a larger volume injection without seismic events but may lead to sudden large events without precursory events.
Copyright and License
© 2025 Seismological Society of America.
Acknowledgement
The authors thank two anonymous reviewers for their insightful and constructive evaluations and Alexis Sáez for valuable discussions. This study was supported by the National Science Foundation (NSF; Award Number 1822214) via the Industry‐University Cooperative Research (IUCR) center Geomechanics and Mitigation of Geohazards.
Data Availability
All simulation results in this article are generated by Quake‐DFN. The simulator and source code are provided on GitHub (https://github.com/limkjae/Quake-DFN) and the Geomechanics and Mitigation of Geohazards (GMG) center webpage (https://gmg.caltech.edu). Both websites were last accessed in December 2024.
Additional details
- National Science Foundation
- 1822214
- Available
-
2024-12-18Published online
- Caltech groups
- Center for Geomechanics and Mitigation of Geohazards (GMG), Seismological Laboratory, Division of Geological and Planetary Sciences (GPS)
- Publication Status
- Published