EGU24-2767, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-2767
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Origins of the high-amplitude magnetic anomaly zone in the northern South China Sea continental margin

Wen-Bin Doo, Yin-Sheng Huang, and Hsueh-Fen Wang
Wen-Bin Doo et al.
  • National Central University, Taoyuan, Taiwan (wenbindoo@gmail.com)

Similar to the feature in the U.S. East Coast, an obvious roughly NE-SW trending high-amplitude magnetic belt (NSCSMA) appears in the northern South China Sea (SCS) continental margin, which extends from southwest Taiwan to the area about 114.5°E and 20°N. The likely cause of this magnetic high is important and interesting but still controversial. This study uses wavelet spectrum analysis, 2-D magnetic modeling, and compact inversion to constrain its causative sources. Our analysis results show the evidence indicating that the geometry and depth of the causative magnetic sources were varied along the strike of the NSCSMA (~15 km in the east and ~25 km in the west). Based on our findings and previous studies, we proposed that the major causative source of the NSCSMA could be the serpentinized upper mantle material.

How to cite: Doo, W.-B., Huang, Y.-S., and Wang, H.-F.: Origins of the high-amplitude magnetic anomaly zone in the northern South China Sea continental margin, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-2767, https://doi.org/10.5194/egusphere-egu24-2767, 2024.