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Late Quaternary surface circulation of the Southern Indian Ocean and its relationship to orbital variations


Howard, W and Prell, WL, Late Quaternary surface circulation of the Southern Indian Ocean and its relationship to orbital variations, Paleoceanography, 7, (1) pp. 79-117. ISSN 0883-8305 (1992) [Refereed Article]

DOI: doi:10.1029/91PA02994


The paleoceanographic history of the Southern Indian Ocean is reflected by the movement of two prominent dynamical features of the Southern Ocean: the Subtropical Convergence (STC) and the Antarctic Polar Front (APF). These fronts, and their associated sea surface temperature (SST) signatures, are well delineated by planktonic foraminiferal faunas in surface sediments of the southern Indian Ocean. Using a transect of piston cores between 42°S and 48°S at about 90°E, we have reconstructed the latitudinal distribution of planktonic foraminiferal faunas over the past 500,000 years. These faunal variations imply changes in the paleolatitudes of the STC and APF and the surface isotherms associated with the fronts. Stratigraphic and chronologic control is provided by δ18O, %CaCO3, and biostratigraphy. Our reconstruction indicates that the STC has been equatorward of its present position (∼40°S) for most of the past 500,000 years and has been poleward of that position for only four relatively brief (∼10,000‐year) intervals during that time. We estimate six equatorward excursions of the APF over the same period, with a maximum total range of about six degrees of latitude. The average paleo‐position of the APF is about 46°S, about 4°north of its present position (∼50°S). Ice‐rafted debris, another indicator of APF position, occurs as far north as 45°S during glacial intervals. Latitudinal gradients in SST show little glacial‐interglacial change between 42° and 48°S, suggesting that surface isotherms were displaced uniformly or that compression of SST gradients occurred outside the transect. Time series analyses of the SST records in this transect reveal statistically significant concentrations of variance in the primary orbital frequency bands. SST variations in these bands are coherent with orbital variations and with changes in δ18O. SST in the subantarctic Indian Ocean slightly precedes changes in δ18O occurring in the eccentricity, obliquity, and precession bands, and lag orbital variations in the obliquity and precession bands. These results place important constraints on possible mechanisms of interhemispheric climatic timing. The similarities in temporal patterns and timing among Southern Ocean SST, atmospheric CO2, and relative flux of North Atlantic Deep Water implicate atmospheric carbon dioxide and deep water circulation as possible interhemispheric pacing mechanisms. Copyright 1992 by the American Geophysical Union.

Item Details

Item Type:Refereed Article
Research Division:Earth Sciences
Research Group:Geology
Research Field:Geology not elsewhere classified
Objective Division:Expanding Knowledge
Objective Group:Expanding knowledge
Objective Field:Expanding knowledge in the earth sciences
UTAS Author:Howard, W (Associate Professor William Howard)
ID Code:35725
Year Published:1992
Web of Science® Times Cited:179
Deposited By:CRC-Antarctic Climate & Ecosystems
Deposited On:2005-08-26
Last Modified:2011-08-30

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