Shoujin Liu, Jian Lin, Zhiyuan Zhou, Fan Zhang. Large along-axis variations in magma supply and tectonism of the Southeast Indian Ridge near the Australian-Antarctic Discordance[J]. Acta Oceanologica Sinica, 2020, 39(1): 118-129. doi: 10.1007/s13131-019-1518-z
Citation: Shoujin Liu, Jian Lin, Zhiyuan Zhou, Fan Zhang. Large along-axis variations in magma supply and tectonism of the Southeast Indian Ridge near the Australian-Antarctic Discordance[J]. Acta Oceanologica Sinica, 2020, 39(1): 118-129. doi: 10.1007/s13131-019-1518-z

Large along-axis variations in magma supply and tectonism of the Southeast Indian Ridge near the Australian-Antarctic Discordance

doi: 10.1007/s13131-019-1518-z
Funds:  The National Key R&D Program of China under contract Nos 2018YFC0310105 and 2018YFC0309800; the China Ocean Mineral Resources R&D Association under contract No. DY135-S2-1-04; the National Natural Science Foundation of China under contract Nos 41890813, 91628301, 41976066, 41706056, 41976064, 91858207 and U1606401; the Chinese Academy of Sciences under contract Nos Y4SL021001, QYZDY-SSW-DQC005 and 133244KYSB20180029; the Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou) under contract No. GML2019ZD0205.
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  • Corresponding author: E-mail: zyzhou@scsio.ac.cn
  • Received Date: 2018-10-08
  • Accepted Date: 2018-11-23
  • Available Online: 2020-04-21
  • Publish Date: 2020-01-20
  • We analyzed seafloor morphology and geophysical anomalies of the Southeast Indian Ridge (SEIR) to reveal the remarkable changes in magma supply along this intermediate fast-spreading ridge. We found systematic differences of the Australian-Antarctic Discordance (AAD) from adjacent ridge segments with the residual mantle Bouguer gravity anomaly (RMBA) being more positive, seafloor being deeper, morphology being more chaotic, M factors being smaller at the AAD. These systematic anomalies, as well as the observed Na8.0 being greater and Fe8.0 being smaller at AAD, suggest relatively starved magma supply and relatively thin crust within the AAD. Comparing to the adjacent ridges segments, the calculated average map-view M factors are relatively small for the AAD, where several Oceanic Core Complexes (OCCs) develop. Close to 30 OCCs were found to be distributed asymmetrically along the SEIR with 60% of OCCs at the northern flank. The OCCs are concentrated mainly in Segments B3 and B4 within the AAD at ~124°–126°E, as well as at the eastern end of Zone C at ~115°E. The relatively small map-view M factors within the AAD indicate stronger tectonism than the adjacent SEIR segments. The interaction between the westward migrating Pacific mantle and the relatively cold mantle beneath the AAD may have caused a reduction in magma supply, leading to the development of abundant OCCs.
  • †These authors contributed equally to this work.
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