TY - JOUR
T1 - Subslab heterogeneity and giant megathrust earthquakes
AU - Fan, Jianke
AU - Zhao, Dapeng
N1 - Funding Information:
We thank the data centres of the Japanese seismic networks and the JMA Unified Earthquake Catalog for providing the high-quality waveform and arrival-time data used for the study of the Japan subduction zone. P.-L. Wang kindly provided her Cascadia slip model. T. Gou provided his Alaska tomographic model. This work was financially supported by the Strategic Priority Research Program of the Chinese Academy of Sciences (XDB42000000) and the National Natural Science Foundation of China (grant no. 41876043, to J.F.) and the Japan Society for the Promotion of Science (grant no. 19H01996, to D.Z.).
Publisher Copyright:
© 2021, The Author(s), under exclusive licence to Springer Nature Limited.
PY - 2021/5
Y1 - 2021/5
N2 - The nucleation and rupture processes of giant megathrust earthquakes (M ≥ 9.0) in subduction zones are still controversial. Most previous studies have focused on the subducting plate interface, and the structure beneath the subducting slab and its influence on earthquake generation remain unclear. Here, we present high-resolution seismic velocity tomography beneath six regions where giant earthquakes have occurred. Subslab low-velocity (slow) anomalies are revealed, which may reflect hot mantle upwelling. The giant earthquake hypocentres are generally located above the edges of the slow anomalies or above the gaps between them. Large coseismic slips of the giant earthquakes mainly occurred above gaps between the slow anomalies. We suggest that differential buoyancy force between the slow anomalies and their gaps may be an important factor for earthquake nucleation, and the rupture extent of a giant earthquake may be constrained by the slow anomalies. Hence, it is necessary to conduct seismic tomography to investigate the detailed subslab structure, which may help to pinpoint the potential location and damage zone of a future giant earthquake.
AB - The nucleation and rupture processes of giant megathrust earthquakes (M ≥ 9.0) in subduction zones are still controversial. Most previous studies have focused on the subducting plate interface, and the structure beneath the subducting slab and its influence on earthquake generation remain unclear. Here, we present high-resolution seismic velocity tomography beneath six regions where giant earthquakes have occurred. Subslab low-velocity (slow) anomalies are revealed, which may reflect hot mantle upwelling. The giant earthquake hypocentres are generally located above the edges of the slow anomalies or above the gaps between them. Large coseismic slips of the giant earthquakes mainly occurred above gaps between the slow anomalies. We suggest that differential buoyancy force between the slow anomalies and their gaps may be an important factor for earthquake nucleation, and the rupture extent of a giant earthquake may be constrained by the slow anomalies. Hence, it is necessary to conduct seismic tomography to investigate the detailed subslab structure, which may help to pinpoint the potential location and damage zone of a future giant earthquake.
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U2 - 10.1038/s41561-021-00728-x
DO - 10.1038/s41561-021-00728-x
M3 - Article
AN - SCOPUS:85105129206
SN - 1752-0894
VL - 14
SP - 349
EP - 353
JO - Nature Geoscience
JF - Nature Geoscience
IS - 5
ER -