Abstract
How fault geometry controls the rupture propagation and segmentation of a strike-slip event is an open question. Deciphering the relationship between the geometric fault complexity and seismic kinematics is essential for both understanding the seismic hazard posed by a particular fault and gaining insights into the fundamental mechanics of earthquake rupture. Here we integrate the finite-fault inversion of synthetic aperture radar observations and back projection of high-frequency teleseismic array waveforms to investigate the rupture geometry of the 2023 Mw 7.8 and Mw 7.6 Kahramanmaraş (southeastern Turkey) earthquake doublet and its impact on the kinematics and slip distribution. We find that large slip asperities are separated by fault bends, whereas intense high-frequency (~1 Hz) sources occur near the branching junctions, suggesting that geometric barriers could decelerate rupture propagation and enhance high-frequency wave radiations. In addition, supershear rupture propagating along the relatively high-velocity material is prone to occur on geometrically simple and smooth faults with relatively few aftershocks. These kinematic characteristics highlight that the geometric complexity of the fault system may be a key factor in the irregular cascading rupture process.
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Data availability
The Sentinel-1 Synthetic Aperture Radar (SAR) data are made available by the European Space Agency and can be accessed at http://scihub.copernicus.eu/dhus. The GNSS raw data are provided by Türkiye Ulusal Sabit GNSS Ağı-Aktif (TUSAGA-Active) System (https://www.tusaga-aktif.gov.tr/Web/DepremVerileri.aspx). All seismograms are available online. The seismic data are provided by the Incorporated Research Institutions for Seismology (IRIS, www.iris.edu) and the Data Management Center of China National Seismic Network at the Institute of Geophysics, China Earthquake Administration (SEISDMC, https://doi.org/10.7914/SN/CB, https://data.earthquake.cn/index.html). The catalogue of relocated aftershocks of the 2023 Turkey earthquake doublet is available at https://github.com/YijianZhou/Seismic-Catalog/blob/main/ding-zhou_eqs-2023_tk-palm_v4.ctlg. The geodetic data, slip models and datasets relevant to BP results can be downloaded from https://doi.org/10.5281/zenodo.8271589. Detailed README files are available, providing summaries of the data and data formats.
Code availability
The open-source GMTSAR software can be accessed at https://github.com/gmtsar/gmtsar. The PRIDE PPP-AR is available at https://github.com/PrideLab/PRIDE-PPPAR. The SDM code can be found at ftp://ftp.gfz-potsdam.de/pub/home/turk/wang/. The MATLAB code of SEBP is available at https://github.com/lsmeng/MUSICBP/tree/SEBP. Figures in this study were generated using GMT59. All other codes used in this study are available upon request.
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Acknowledgements
H.S. was supported by the Strategic Priority Research Program of the Chinese Academy of Sciences (XDB 41000000). R.G. and X.T. were supported by the State Key Laboratory of Geodesy and Earth’s Dynamics (S22L620104). Y. Zhang, R.G., X.T. and J.W. were supported by the Open Fund of Wuhan Gravitation and Solid Earth Tides National Observation and Research Station (WHYWZ202210). Y. Zheng and D.L. were supported by the NSFC grants (42274082, 42030108). The teleseismic waveforms of the China array are provided by the Data Management Center of China National Seismic Network at the Institute of Geophysics, China Earthquake Administration. T.T. and T.E. acknowledge the Istanbul Technical University Research Fund (ITU-BAP) and the Alexander von Humboldt Foundation Research Fellowship Award for providing computing facilities through the Humboldt-Stiftung Follow-Up Program.
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R.G. conceived and led the study. Y. Zhang and D.L. performed the uniform SEBP and regional SEBP. X.T. performed the InSAR analysis and finite-fault inversion. Y. Zhang, X.T., D.L., R.G., T.T., T.E., Y. Zheng, J.W. and H.S. wrote the paper and participated in the interpretation of the results.
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Nature Geoscience thanks Lei Zhang and the other, anonymous, reviewer(s) for their contribution to the peer review of this work. Primary Handling Editor: Tamara Goldin, in collaboration with the Nature Geoscience team.
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Extended data
Extended Data Fig. 1 Mapping fault traces.
Sentinel-1 wrapped interferograms of the descending (a) and ascending (d) tracks. Unwrapped deformation of the descending (b) and ascending (e) tracks. Range pixel offset results of the 2023 Kahramanmaraş earthquake doublet along the descending (c) and ascending (f) tracks. Red and blue colors mean that the displacements move toward and away from the satellite, respectively. The black lines represent the mapped traces of the seismogenic faults. The red and green stars are the epicenters of the Mw 7.8 earthquake and the Mw 7.6 earthquake, respectively.
Extended Data Fig. 2 Estimation of the potential impact of postseismic deformation.
GNSS time series of ANTE (a) and EKZ1 (b) sites. LOS postseismic deformation along the ascending (c) and descending (d) track. Yellow triangles show the locations of ANTE and EKZ1, respectively. The beachball indicates the focal mechanism of the Mw 6.3 aftershock on February 20, 2023 (USGS). Other symbols are the same as Extended Data Fig. 1.
Extended Data Fig. 3 Search results of our preferred model.
(a) The trade-off between the data misfit and model roughness. (b) The search for dip of the Mw 7.6 earthquake. The red circle indicates the optimal dip of 76°.
Extended Data Fig. 4 InSAR fittings.
Observations of the ascending (a) and descending (d) orbits. Predictions along ascending (b) and descending (e) tracks. (c) and (f) Associated residuals.
Extended Data Fig. 5 Checkerboard test results.
(a) The input of slip distribution. (b) The recovered slip distribution using the same inversion strategies.
Extended Data Fig. 6 Station distribution.
Telesesimic arrays for back-projection analysis of the 2023 Mw 7.8 (a) and Mw 7.6 (b) Kahramanmaraş earthquake doublet. The colored triangles represent the seismic stations from arrays in Alaska (AK) and China (CN). The red and green stars denote the locations of the Mw 7.8 and Mw 7.6 earthquakes in the 2023 Kahramanmaraş earthquake doublet.
Extended Data Fig. 7 Spatial bias of BPs.
Spatial biases of the Mw 7.8 earthquake for the AK array, before (a) and after (b) the regional SEBP calibration.
Extended Data Fig. 8 Background seismicity.
Seismic activity in southeastern Türkiye during 1900–2018 from ref. 38. (a) Distribution of background seismicity and the 2023 Kahramanmaraş earthquake doublet. The red and green stars indicate the locations of the epicenters of the Mw 7.8 and Mw 7.6 earthquakes. The red dots indicate earthquakes of small magnitude (1 < M < 5.5) while yellow stars indicate earthquakes of larger magnitude (5.5 < M < 8.0). The black lines indicate the mapped fault traces. The green lines represent the depth profiles of earthquakes. (b) Cross-section of the earthquake locations for profiles AB and BC. (c) Cross-section of the earthquake locations for profile DE.
Extended Data Fig. 9 Lateral variation of the isotropic Vp images resolved at three depth layers.
At the central top of each map, the layer depth is given: (a) 4, (b) 12, and (c) 21 km. Relatively high and low Vp perturbations from ref. 46 are represented by the blue and red colors, respectively. The red and green stars indicate the locations of the epicenters of the Mw 7.8 and Mw 7.6 events. The black lines indicate the mapped fault traces.
Supplementary information
Supplementary Information
Supplementary Tables 1–5.
Supplementary Video 1
BP movie for the Mw 7.8 earthquake.
Supplementary Video 2
BP movie for the Mw 7.6 earthquake.
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Zhang, Y., Tang, X., Liu, D. et al. Geometric controls on cascading rupture of the 2023 Kahramanmaraş earthquake doublet. Nat. Geosci. 16, 1054–1060 (2023). https://doi.org/10.1038/s41561-023-01283-3
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DOI: https://doi.org/10.1038/s41561-023-01283-3