Ground Motion Characteristics of Subshear and Supershear Ruptures in the Presence of Sediment Layers
Abstract
We investigate the impact of sediment layers on ground motion characteristics during subshear and supershear rupture growth. Our findings suggest that sediment layers may lead to local supershear propagation, affecting ground motion, especially in the fault parallel (FP) direction. In contrast to homogeneous material models, we find that in the presence of sediment layers, a larger fault normal (FN) compared to fault parallel (FP) particle velocity jump, reflects shear propagation at depth but does not rule out shallow supershear propagation. Conversely, a large fault parallel (FP) compared to fault normal (FN) particle velocity jump indicates supershear propagation at depth. In the presence of a shallow layer, we also uncover a non-monotonic behavior in the sediment's influence on supershear transition and ground motion characteristics. During supershear propagation at depth we observe that sediment layers contribute to enhancing FP velocity pulses while minimally affecting the FN component. Furthermore, in the limit of global supershear propagation we identify local supersonic propagation within the sediment layers that significantly alters the velocity field around the rupture tip as observed on the free surface, creating both dilatational and shear Mach cones. In all our models with sediments we also find a significant enhancement in the fault vertical component of ground velocity. This could have particular implications for hazard assessments, such as in applications related to linear infrastructure, or a higher propensity to tsunami wave generation. Our research unravels the importance of considering heterogeneous subsurface material distribution in our physical models as they can have drastic implications on earthquake source physics.
Copyright and License
Acknowledgement
We thank Editor Sidao Ni, Suli Yao and an anonymous reviewer for their insightful reviews that helped improve the manuscript. MA would like to thank Eric Dunham for insightful discussions. The authors would also like to thank Grigorios Lavrentiadis for sharing the scripts used to characterize the ground motion. AJR and MA acknowledges support by the Caltech/MCE Big Ideas Fund (BIF), as well as the Caltech Terrestrial Hazard Observation and Reporting Center (THOR). The simulations conducted in this study were possible thanks to the support of Amazon, through the AI4Science initiative. AE acknowledge support by the National Science Foundation CAREER award No. 1753249 for modelling complex fault zones. The authors acknowledge support from the Southern California Earthquake Center through a collaborative agreement between NSF. Grant Number: EAR0529922 and USGS. Grant Number: 07HQAG0008.
Data Availability
The software used to conduct the dynamic rupture model is open access and can be obtained at https://github.com/wqseis/drdg3d.
Files
Name | Size | Download all |
---|---|---|
md5:0581e536f8a8cc3eb74780c404b099d4
|
4.7 MB | Preview Download |
Additional details
- California Institute of Technology
- Caltech/MCE Big Ideas Fund
- California Institute of Technology
- Caltech Terrestrial Hazard Observation and Reporting Center (THOR)
- Amazon (United States)
- AI4Science Initiative
- National Science Foundation
- EAR-1753249
- Southern California Earthquake Center
- National Science Foundation
- EAR0529922
- United States Geological Survey
- 07HQAG0008
- Accepted
-
2024-11-21Accepted
- Available
-
2024-11-27Published
- Available
-
2024-12-18Corrected and typeset
- Caltech groups
- GALCIT
- Publication Status
- Published