Journal of Tropical Oceanography ›› 2017, Vol. 36 ›› Issue (6): 1-11.doi: 10.11978/2016119CSTR: 32234.14.2016119

Special Issue: 海上丝绸之路专题

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Magmatic and tectonic extension at the Southwest Indian Ridge between 14°E and 25°E

Caicai ZHA1,3, Jian LIN2,1   

  1. 1. CAS Key Laboratory of Ocean and Marginal Sea Geology, South China Sea Institute of Oceanology, Guangzhou 510301, China
    2. Department of Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA
    3. University of Chinese Academy of Sciences, Beijing 100049, China
  • Received:2016-11-19 Revised:2017-02-02 Online:2017-11-30 Published:2018-01-18
  • About author:Author:QIU Chunhua.E-mail: qiuchh3@mail. sysu.edu.cn
  • Supported by:
    Chinese Academy of Sciences Project (QYZDY-SSW-DQC005, Y4SL021001, YZ201325, YZ201534);National Natural Science Foundation of China (91628301, U1606401, 41676044)

Abstract:

In this study we used the high-resolution shipboard multibeam bathymetry and gravity data to investigate the tectonic and magmatic characteristics of the Southwest Indian Ridge (SWIR) between 14#cod#x000b0;and 25#cod#x000b0;E. First, we filtered the original bathymetry to obtain a short-wavelength bathymetry map (wavelength less than 20 km), which was used together with the topographic slope map to identify surface normal faults. We also obtained a long-wavelength bathymetry map (wavelength more than 20 km) that was used to calculate across-ridge axis topographic relief. We also calculated the fraction of plate separation accommodated by magmatic accretion, i.e., the M factor. We then calculated the Residual Mantle Bouguer Anomaly (RMBA) by removing from the free-air gravity anomaly the gravitational effects of water/crust and crust/mantle interfaces as well as lithospheric plate cooling, assuming a reference crustal thickness of 6 km. Finally, we calculated the M factor, the mean values of RMBA, and fault throws within 10-km- wide running windows along profiles across the ridge axis and investigated the correlations among these parameters. We found that the magma supply varied significantly in time and space at the SWIR between 14#cod#x000b0;and 25#cod#x000b0;E and the axial relief showed strong asymmetry between conjugate ridge flanks that seemed to be controlled by the mean M factor near the ridge axis. Regionally-averaged tectonic extensional strains (i.e., 1-M) were about 20%~50% and the southern flank underwent greater average tectonic extensional strains. Areas with thicker crust (i.e., more negative RMBA) are often associated with greater M values and smaller fault throws, indicating episodes of increased local 3D magma supply at this ultraslow spreading ridge.

Key words: Southwest Indian Ridge, tectonism, magmatism, M factor, multibeam bathymetry, Residual Mantle Bouguer Anomaly

CLC Number: 

  • P736.1