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Crustal S-wave velocity structure across the northeastern South China Sea continental margin: implications for lithology and mantle exhumation

WenAi Hou Chun-Feng Li XiaoLi Wan MingHui Zhao XueLin Qiu

地球与行星物理（英文）2019，Vol.3Issue(4)：314-329,16.
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地球与行星物理（英文）2019，Vol.3Issue(4)：314-329,16.DOI:10.26464/epp2019033

Crustal S-wave velocity structure across the northeastern South China Sea continental margin: implications for lithology and mantle exhumation

Crustal S-wave velocity structure across the northeastern South China Sea continental margin: implications for lithology and mantle exhumation

WenAi Hou 1Chun-Feng Li 1XiaoLi Wan 2MingHui Zhao 3XueLin Qiu4

作者信息

  • 1. Institute of Marine Geology and Resources, Zhejiang University, Zhoushan Zhejiang 316021, China
  • 2. Laboratory for Marine Mineral Resources, Qingdao National Laboratory for Marine Science and Technology, Qingdao 266237, China
  • 3. State Key Laboratory of Marine Geology, Tongji University, Shanghai 200092, China
  • 4. South China Sea Institute of Oceanology, Chinese Academy of Sciences, Guangzhou 510301, China
  • 折叠

摘要

关键词

South China Sea/continental margin/crustal structure/converted S-wave/VP/VS ratio/lithology/serpentinization

Key words

South China Sea/continental margin/crustal structure/converted S-wave/VP/VS ratio/lithology/serpentinization

引用本文复制引用

WenAi Hou,Chun-Feng Li,XiaoLi Wan,MingHui Zhao,XueLin Qiu..Crustal S-wave velocity structure across the northeastern South China Sea continental margin: implications for lithology and mantle exhumation[J].地球与行星物理（英文）,2019,3(4):314-329,16.

基金项目

We thank South China Sea Institute of Oceanology (SCSIO) for providing R/V Shiyan-2 to carry out this experiment, sponsored by Oceanographic Research Vessel Sharing Plan (NORC2016-08) of National Natural Science Foundation of China. We thank all re-searchers and sailors on Shiyan-2 for collecting the OBS and MCS data. We also thank chief scientist Hongbo Zheng, and team lead-er Enyuan He for their important contributions to this voyage. Comments from two anonymous reviewers helped improved this paper. This research is also funded by National Natural Science Foundation of China (Grant Nos. 41776057, 41761134051, 91858213, 41730532 and 91428039). Data processing and map-ping is supported by GMT (Wessel and Smith, 1998), RayInvr (Zelt and Smith, 1992), and Tomo2D (Korenaga et al., 2000). （SCSIO）

地球与行星物理（英文）

OACSCD

2096-3955

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