L. Labeyrie et al., HYDROGRAPHIC CHANGES OF THE SOUTHERN-OCEAN (SOUTHEAST INDIAN SECTOR) OVER THE LAST 230 KYR, Paleoceanography, 11(1), 1996, pp. 57-76
Hydrographical changes of the southern Indian Ocean over the last 230
kyr, is reconstructed using a 17-m-long sediment core (MD 88 770; 46 d
egrees 01'S 96 degrees 28'E, 3290m). The oxygen and carbon isotopic co
mposition of planktonic (N, pachyderma sinistra and G. bulloides) and
benthic (Cibicidoidies wuellerstorfi, Epistominella exigua, and Meloni
s barleeanum) foraminifera have been analysed. Changes in sea surface
temperatures (SST) are calculated using diatom and foraminiferal trans
fer functions. A new core top calibration for the Southern Ocean allow
s an extension of the method developed in the North Atlantic to estima
te paleosalinities (Duplessy et al., 1991). The age scale is built usi
ng accelerator mass spectrometry (AMS) C-14 dating of N. pachyderma s.
for the last 35 kyr, and an astronomical age scale beyond. Changes in
surface temperature and salinity clearly lead (by 3 to 7 kyr) deep wa
ter variations. Thus changes in deep water circulation are not the cau
se of the early response of the surface Southern Ocean to climatic cha
nges. We suggest that the early warming and cooling of the Southern Oc
ean result from at least two processes acting in different orbital ban
ds and latitudes: (1) seasonality modulated by obliquity affects the h
igh-latitude ocean surface albedo (sea ice coverage) and heat transfer
to and from the atmosphere; (2) low-latitude insolation modulated by
precession influences directly the atmosphere dynamic and related prec
ipitation/ evaporation changes, which may significantly change heat tr
ansfer to the high southern latitudes, through their control on latitu
dinal distribution of the major frontal zones and on the conditions of
intermediate and deep water formation.