Rupture process models of the Yangbi and Maduo earthquakes that struck the eastern Tibetan Plateau in May 2021

Rupture process models of the Yangbi and Maduo earthquakes that struck the eastern Tibetan Plateau in May 2021
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2021年5月青藏高原东部漾濞地震和玛多地震破裂过程模型

DOI:
10.1016/j.scib.2021.11.009
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发表时间:
2021
期刊:
影响因子:
18.9
通讯作者:
Zhenxing Yao
Zhenxing Yao
中科院分区:
综合性期刊1区
文献类型:
--
作者:
Wei-Min Wang;Jiankun He;Xun Wang;Yun Zhou;Jinlai Hao;Lian-Feng Zhao;Zhenxing Yao

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An M6. 4 earthquake struck Yangbi County, Dali Prefecture, Yunnan Province, on May 21, 2021, at 21: 48 Beijing Time (2021-05-21 13: 48: 37 UTC). Soon thereafter, at 2: 04 UTC on May 22, 2021 (2021-05-21 18: 04: 13 UTC), an M7. 4 earthquake struck Madou County, Guoluo Prefecture, Qinghai Province. These two earthquakes occurred in the southeastern edge and in high-altitude hinterland of the eastern Tibetan Plateau respectively (Fig. 1a), and both caused human casualties and property damage, triggering earthquake emergency response efforts. The occurrence of strong earthquakes at different sites within 5 h of each other indicates continuous tectonic movements and violent seismic activity on the Tibetan Plateau under the collisional convergence between the Indian and Eurasian continental plates [3]. Observations of crustal motion expose clockwise rotational deformation in the eastern Tibetan Plateau along the axis of the eastern Himalayan syntaxis [2, 4]. Furthermore, studies combining tectonic and historical seismic data with numerical simulations reveal that the shear effect of the eastward flow of crustal material within the Tibetan Plateau leads to active sinistral strike-slip faulting in the northern part of the plateau and dextral strike-slip faulting in the south [1, 3, 5]. The source mechanisms of these two events (Fig. S1 online) suggest that both earthquakes occurred in response to the strain induced by the current crustal deformation, which is consistent with the above deformation pattern of the Tibetan Plateau. Accordingly, studying the deformation mechanisms in and around the Tibetan Plateau, being the largest zone of tectonic deformation on Earth, is a major focus of ongoing geoscience research. Nevertheless, the main views of the two predominant intraplate deformation models, the ‘‘block model” and the ‘‘continuum model”, cannot perfectly explain the observed deformation and seismic activity across the Tibetan Plateau [2], indicating that further work is needed. In this context, we developed models of the spatiotemporal source rupture processes of these two strong earthquakes by jointly inverting seismic waveforms and coseismic deformation data, thereby revealing the corresponding tectonic motion characteristics. These findings can provide new insights into and constraints on the deformation mechanisms on the Tibetan Plateau. Additionally, the proposed source models, as fundamental components of seismological research, can provide a scientific basis for seismic hazard mitigation and earthquake risk assessment.We downloaded waveform records acquired at globally distributed digital seismic stations through the Incorporated Research Institutions for Seismology (IRIS) Data Management Center to rapidly invert the focal mechanisms and source rupture processes of these two strong earthquakes. Based on the preliminary results, we gathered additional observations to construct a finite fault model and accurately obtained the corresponding source processes by a joint inversion. The data used to study the Yangbi earthquake source process are regional three-component waveforms (downloaded from the China National Digital Seismic Network), far-field P and SH waveforms, and coseismic deformation data (interferometric synthetic aperture radar, InSAR) obtained from the European Space Agency (ESA) Sentinel satellites, whose radar images cover the pre-and postearthquake source area (Table S1 online). To study the Maduo earthquake source process, due to the lack of near-source seismic records, we used far-field P and SH waveforms and coseismic line-of-sight (LOS) displacements obtained from the ESA Sentinel …