Group B, Poster #062, Stress and Deformation Over Time (SDOT)
Characteristic Slow‐Slip Events on the Superstition Hills Fault
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Poster Presentation
2024 SCEC Annual Meeting, Poster #062, SCEC Contribution #14010 VIEW PDF
the following months. Analysis of interferometric synthetic aperture radar (InSAR) data indicates that the event initiated on the northern portion of the fault, prior to detection by the creepmeters, and subsequently propagated north and south over the following days. Fault offsets obtained from both field and InSAR measurements illuminate a skewed, bi-modal surface rupture. Slip on the southern section of the fault was approximately twice as large as that on the northern section. In addition, slip on the southern section is highly localized (< 100 m), while the northern section is characterized by distributed deformation over a ~500-1200 m zone. Kinematic slip models obtained from inversions of InSAR data constrain the depth extent of slip to 2-4 km; while the entire event is confined to the shallow sedimentary layer, there are additional systematic contrasts in slip depth between the northern and southern halves of the fault. Comparisons of the slip models and surface offsets reveal a remarkable similarity between the 2023 SSE and past events occurring in 1999, 2006, and 2010, which indicates that the SHF exhibits at least one style of characteristic rupture. Our updated time-averaged rates of shallow creep along the SHF implies that the long-term fault slip rate is underestimated, which is consistent with previous work that has suggested the SHF is structurally connected to the main San Jacinto Fault strand.
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