EGU25-2135, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-2135
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Wednesday, 30 Apr, 14:05–14:15 (CEST)
 
Room 0.16
Source Spectra for Global Shallow Large Earthquakes from 2000 to 2024
Zhou Jiangcheng and Zhang Yong
Zhou Jiangcheng and Zhang Yong
  • Peking University, School of Earth and Space Sciences, Institute of Theoretical and Applied Geophysics, Beijing, China (zhang-yong@pku.edu.cn)

The kinematic characteristics of an earthquake source offer insights into its physical properties, with macroscopic parameters such as seismic moment and radiated energy serving as key indicators for describing seismic hazards. In this study, we explored the characteristics of earthquake sources in the frequency domain. Specifically, we introduced a hybrid method using teleseismic P-wave data to derive source spectra for over 200 large (MW > 7) shallow (depth < 70 km) earthquakes from 2000 to 2024. Our analysis reveals that in a simple ω-n model, the power exponent n is consistently less than 2 when the corner frequency aligns with the earthquake's total duration. To further characterize earthquake source properties, we defined the centroid frequency (fe) as the centroid of the energy spectral density which can represent the dimension of asperities on the fault plane. We also proposed the ratio between observed radiated energy and that predicted by the ω-² decay model as a metric for quantifying rupture heterogeneity (RH). Relationships of fe and RH with focal mechanism, magnitude, and centroid depth were analyzed within the conventional asperity model framework. Our source spectra dataset can also provide a robust foundation for future investigations into earthquake sources.

How to cite: Jiangcheng, Z. and Yong, Z.: Source Spectra for Global Shallow Large Earthquakes from 2000 to 2024, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2135, https://doi.org/10.5194/egusphere-egu25-2135, 2025.