2017
DOI: 10.1093/gji/ggx181
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Lithospheric structure beneath the northeastern Tibetan Plateau and the western Sino-Korea Craton revealed by Rayleigh wave tomography

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Cited by 45 publications
(53 citation statements)
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“…A continuous low velocity anomaly in the QOB, an area between the Haiyuan fault and the east Kunlun fault, is generally imaged at periods from 20 to 100 s (Figures a–e). The observation of this low velocity anomaly is consistent with previous Rayleigh wave tomography models (Bao, Song, & Li, ; Li et al, ), while it is partially different from a relatively high velocity in the north QOB obtained from previous Rayleigh and Love wave tomography study (Li et al, , ), which has limited station coverage and crossing ray paths there. The Songpan‐Ganzi terrane (SGT) is characterized by low velocity anomaly at periods less than 50 s (Figures a and b) and relatively high velocity compared with the QOB at periods of 59–100 s. Another interesting feature is the sharp velocity contrast between high phase velocities in the Ordos block (OB) and low phase velocities in the Alxa block (AB) at intermediate‐long periods (>45 s) (Figures c–e).…”
Section: Resultssupporting
confidence: 89%
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“…A continuous low velocity anomaly in the QOB, an area between the Haiyuan fault and the east Kunlun fault, is generally imaged at periods from 20 to 100 s (Figures a–e). The observation of this low velocity anomaly is consistent with previous Rayleigh wave tomography models (Bao, Song, & Li, ; Li et al, ), while it is partially different from a relatively high velocity in the north QOB obtained from previous Rayleigh and Love wave tomography study (Li et al, , ), which has limited station coverage and crossing ray paths there. The Songpan‐Ganzi terrane (SGT) is characterized by low velocity anomaly at periods less than 50 s (Figures a and b) and relatively high velocity compared with the QOB at periods of 59–100 s. Another interesting feature is the sharp velocity contrast between high phase velocities in the Ordos block (OB) and low phase velocities in the Alxa block (AB) at intermediate‐long periods (>45 s) (Figures c–e).…”
Section: Resultssupporting
confidence: 89%
“…In our 3‐D V SH model, a low velocity anomaly is observed in the midlower crust and can be traced down to uppermost mantle beneath the QOB (Figures d–g and ), consistent with the observations of slow P wave velocity (Lei & Zhao, ) and SV wave velocity (Li et al, , ), and inefficient propagation of high frequency Sn (Barron & Priestley, ). Additionally, a diffuse lithosphere asthenosphere boundary from S receiver function suggests small temperature gradient between mantle lithosphere and asthenosphere (Shen, Yuan, & Liu, ).…”
Section: Discussionsupporting
confidence: 90%
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“…Li et al [2013Li et al [ , 2016 suggested that another heat source for the LVZ beneath the KF zone is from asthenosphere upwelling caused by the removal of lithosphere root. The presence of relatively low velocity in upper mantle may account for the mantle flow beneath the WQT [e.g., Guo and Chen, 2017;Li et al, 2016Li et al, , 2017Zheng et al, 2016]. Shear wave splitting measurements also suggested that the asthenosphere mantle flow existed beneath the WQT [e.g., Chang et al, 2017;Yu and Chen, 2016].…”
Section: Origin Of Two Crustal Lvzs In the Northern Sgt Southwesternmentioning
confidence: 99%
“…Most of dispersion data in this study are obtained from local Rayleigh wave tomographic images of NE and SE Tibet (Li, Pan, et al, ; ; Pan et al, ). These local tomography models mainly used earthquake data recorded at the ChinArray seismic stations to produce group and phase velocity maps at periods of 10–60 s and 10–80 s, respectively.…”
Section: Methodsmentioning
confidence: 99%