EGU22-879, updated on 26 Mar 2022
https://doi.org/10.5194/egusphere-egu22-879
EGU General Assembly 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

Imaging evolution of Cascadia slow-slip event using high-rate GPS

Yuji Itoh1, Yosuke Aoki2, and Junichi Fukuda2
Yuji Itoh et al.
  • 1Earthquake Research Institute, The University of Tokyo, Japan (itoh.yuji.86u@kyoto-u.jp)
  • 2Earthquake Research Institute, The University of Tokyo, Japan

The short-term slow slip event (SSE), a class of slow earthquakes which has duration of a few to tens of days, is typically detected and modeled from daily static Global Positioning System (GPS) data. However, the daily GPS data cannot image the sub-daily SSE processes, so underlying mechanisms of SSEs have been still elusive. By processing the raw GPS observables in the kinematic analysis approach, we can obtain surface deformation field at the subdaily interval, which has great potential to overcome the time resolution issue present in the daily static GPS data. Although the kinematic GPS coordinates are known much noisier (~ cm) than the daily static coordinates (~ a few mm), recent applications to postseismic deformation studies achieved identifying sub-cm deformation. Motivated by them, we for the first time applied the kinematic GPS coordinates to model the short-term SSE.

We chose one Cascadia SSE in March – April 2017, which has been already reported from daily GNSS data, and performed the kinematic GPS analysis at a 30-second interval for observations during the event occurrence. Although the obtained raw coordinate series were quite noisy, we were able to discern the transient motion of a few mm during the event after carefully removing non-tectonic position fluctuation such as multipath effects, common mode errors and outliers.

Then, we inverted the cleaned data at a 30-minute interval using a Kalman-filter based method to infer spatiotemporal evolution of slip. The obtained spatiotemporal slip distribution exhibits a multi-stage evolution consisting of an isotropic growth of SSE and subsequent along-strike migration and termination. The transition of the slip growth mode occurs when the slip area fills the rheologically permitted down-dip width for the SSE occurrence. As conceptualized by Gomberg et al. (2016, GRL), this is analogous to the rupture growth of regular great earthquakes, so it implies the presence of common mechanical factors behind the two distinct slip phenomena. The inferred moment rate has two peaks, which are consistent with the daily tremor counts in this region.

We carried out another slip inversion using the daily static GPS data recorded during the same period and the same inversion method to investigate the performance and limitation of our kinematic GPS data. A moment rate inferred from the daily data has also two peaks, so our 30-minute inversion result has the comparable time resolution to that derived from the widely-used daily data. This is an astonishing result given the long-believed low signal-to-noise ratio of the kinematic GPS. Our results strongly highlight the importance of better understanding of the non-tectonic noise in the kinematic GPS analysis, which will further improve the temporal resolution of SSE.

How to cite: Itoh, Y., Aoki, Y., and Fukuda, J.: Imaging evolution of Cascadia slow-slip event using high-rate GPS, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-879, https://doi.org/10.5194/egusphere-egu22-879, 2022.

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