4.7 Article

Millennial/centennial-scale thermocline ventilation changes in the Indian Ocean as reflected by aragonite preservation and geochemical variations in Arabian Sea sediments

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GEOCHIMICA ET COSMOCHIMICA ACTA
卷 73, 期 22, 页码 6771-6788

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PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.gca.2009.08.028

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  1. CNRS
  2. ANR
  3. Gary Comer Science and Education Foundation
  4. European Community [HPRN-CT-2002-0221]

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The formation and temporal variability of the oxygen minimum zone (OMZ) of the Arabian Sea is a subject of intense research. We contribute to the discussion by studying modern seawater profiles of the Indian Ocean (salinity, O-2, pH, aragonite saturation, nitrate deficit, nutrients), which show that Subantarctic Mode and Antarctic Intermediate Waters (SAMW-AAIW) have a strong influence on the OMZ characteristics of the Arabian Sea. To obtain a better grasp of the range of possible OMZ variations, we studied a 50-kyr record in the NE Arabian Sea (core MD042876) from a site at 828 m water depth within the thermocline. In this core, aragonite is preserved during North Atlantic Heinrich events (HEs) and Dansgaard-Oeschger (DO) stadials, while it is absent during DO interstadials and most of the Holocene. Considering the excellent correlation between aragonite content and Sr/Ca ratio, as well as the presence of. ne-grained aragonitic needles and the isotopic composition (delta C-13) of carbonates in the. ne fraction, we infer that essentially all aragonite originates as. ne Sr-rich debris from shallow water. A comparison with other records from the NE Arabian Sea (Sr/Ca, delta N-15) indicates that aragonite variability in the cores is rather controlled by OMZ intensity variations as forcing mechanism while changes in aragonite supply seem to play a minor role. The strong correlation of aragonite content with changes in millennial-scale ventilation of the Indian Ocean, as well as a comparison with modern oceanographic conditions, supports the theory that OMZ intensity variations are controlled by changes in the formation of SAMW-AAIW, and are not only due to monsoonal changes. Thus, during HEs and DO stadials, the thermocline Arabian Sea experienced a strengthened influx of O-2-rich SAMW-AAIW. On the other hand, OMZ conditions during DO interstadials and the Holocene seem best explained by analogy with the present-day situation: low supply of O-2 combined with elevated O-2 demand controlled by monsoon-related productivity. (C) 2009 Elsevier Ltd. All rights reserved.

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