Is there a big mantle wedge under eastern Tibet?

Jianshe Lei, Dapeng Zhao, Xiwei Xu, Yi Gang Xu, Mofei Du

Research output: Contribution to journalArticlepeer-review

28 Citations (Scopus)

Abstract

The big mantle wedge (BMW) model was originally proposed to explain the origin of the intraplate Changbaishan volcano in NE China where the subducting Pacific slab becomes stagnant in the lower part of the mantle transition zone (MTZ). The BMW is defined as a broad region in the upper mantle and upper part of the MTZ overlying the long stagnant Pacific slab. Under eastern Tibet, prominent low-velocity (low-V) anomalies are revealed in the upper mantle, whereas an obvious and broad high-velocity (high-V) anomaly is imaged in the MTZ from the Burma arc northward to the Kunlunshan fault zone and eastward to the Xiaojiang fault zone. In addition, receiver-function analyses clearly illustrate a thickened MTZ in a similar area. Hence we conclude that there is a BMW structure under eastern Tibet, which can explain the deep origin of the Tengchong volcano and generation of large crustal earthquakes in the region. The Tengchong volcano is caused by hot and wet mantle upwelling in the BMW and fluids from dehydration reactions of the stagnant Indian slab in the MTZ. The 2008 Wenchuan earthquake (Ms 8.0) took place in a transitional belt from the low-V Songpan-Ganzi block to the high-V Sichuan basin, suggesting that the occurrence of the Wenchuan earthquake was affected by the BMW structure. These results shed new light on the mantle structure and dynamics under eastern Tibet.

Original languageEnglish
Pages (from-to)100-113
Number of pages14
JournalPhysics of the Earth and Planetary Interiors
Volume292
DOIs
Publication statusPublished - 2019 Jul

Keywords

  • Big mantle wedge
  • Earthquakes
  • Eastern Tibet
  • Receiver-function analysis
  • Seismic velocity
  • Tengchong volcano

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Geophysics
  • Physics and Astronomy (miscellaneous)
  • Space and Planetary Science

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