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

被引:53
作者
Boening, Philipp [1 ]
Bard, Edouard [1 ]
机构
[1] Univ Aix Marseille 3, CNRS, Coll France, UMR6635,CEREGE, F-13545 Aix En Provence 4, France
关键词
INTERMEDIATE WATER CIRCULATION; WESTERN CONTINENTAL-SHELF; CALCIUM-CARBONATE; OXYGEN-MINIMUM; DEEP-SEA; CLIMATE; DISSOLUTION; DENITRIFICATION; HALIMEDA; MONSOON;
D O I
10.1016/j.gca.2009.08.028
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
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.
引用
收藏
页码:6771 / 6788
页数:18
相关论文
共 102 条
[1]   Holocene coastal carbonates and evaporites of the southern Arabian Gulf and their ancient analogues [J].
Alsharhan, AS ;
Kendall, CGS .
EARTH-SCIENCE REVIEWS, 2003, 61 (3-4) :191-243
[2]   The effect of millennial-scale changes in Arabian Sea denitrification on atmospheric CO2 [J].
Altabet, MA ;
Higginson, MJ ;
Murray, DW .
NATURE, 2002, 415 (6868) :159-162
[3]   Wind-Driven Upwelling in the Southern Ocean and the Deglacial Rise in Atmospheric CO2 [J].
Anderson, R. F. ;
Ali, S. ;
Bradtmiller, L. I. ;
Nielsen, S. H. H. ;
Fleisher, M. Q. ;
Anderson, B. E. ;
Burckle, L. H. .
SCIENCE, 2009, 323 (5920) :1443-1448
[4]  
[Anonymous], 2006, ORNLCDIAC105 US DOE
[5]   Dominant Northern Hemisphere climate control over millennial-scale glacial sea-level variability [J].
Arz, Helge W. ;
Lamy, Frank ;
Ganopolski, Andrey ;
Nowaczyk, Norbert ;
Paetzold, Juergen .
QUATERNARY SCIENCE REVIEWS, 2007, 26 (3-4) :312-321
[6]  
Arz HW, 2001, GEOLOGY, V29, P239, DOI 10.1130/0091-7613(2001)029<0239:MSCOSA>2.0.CO
[7]  
2
[8]  
BARD E, 1989, RADIOCARBON, V31, P510
[9]   SEA-SURFACE TEMPERATURE FROM CORAL SKELETAL STRONTIUM CALCIUM RATIOS [J].
BECK, JW ;
EDWARDS, RL ;
ITO, E ;
TAYLOR, FW ;
RECY, J ;
ROUGERIE, F ;
JOANNOT, P ;
HENIN, C .
SCIENCE, 1992, 257 (5070) :644-647
[10]   SOLUBILITY OF CALCITE AND ARAGONITE IN SEAWATER AT ATMOSPHERIC-PRESSURE AND 34.5PERCENT SALINITY [J].
BERNER, RA .
AMERICAN JOURNAL OF SCIENCE, 1976, 276 (06) :713-730