Cv. Grazzini et al., FERTILITY TRACERS AND MONSOON FORCING AT AN EQUATORIAL SITE OF THE SOMALI BASIN (NORTHWEST INDIAN-OCEAN), Marine micropaleontology, 26(1-4), 1995, pp. 137-152
Temporal changes in biological and isotopic tracers have successfully
been used to monitor monsoon variability in the Arabian Sea. Convincin
g evidence that fertility indicators, such as the relative abundance o
f the planktic foraminifer Globigerina bulloides, and SiO2 and Ba flux
es, can monitor monsoon changes, has also been published. Time series
of the C-13 content of the thermocline foraminifer Neogloboquadrina du
tertrei, and of an Upwelling Radiolarian Index (URI), have been used t
o reconstruct upwelling changes in the Somali Basin at 5 degrees N for
the last 160 kyr. In order to establish a reference site for comparis
on with other upwelling and/or fertility records from the same area, a
time series of 8 climatic and fertility proxies (C-13 content of N. d
utertrei and Globorotalia menardii, percentages of G. bulloides and of
a thermocline foraminiferal group, minimal delta(18)O values of Globi
gerinoides sacculifer, N. dutertrei and G. menardii) are investigated
in the spectral domain for the last 360 kyr, at a site located at the
equator and outside the Somali upwelling centers (Core MD 85668). Chro
nostratigraphies for these records are developed by correlation of oxy
gen isotope record of G. sacculifer to the Martinson standard stacked
benthic oxygen isotope record. The temporal resolution of the data, is
between 2 and 5 kyr. Cross spectral comparisons with ETP (Eccentricit
y + Tilt + Precession-composite signal) were used to estimate coherenc
es in conjunction with phase relationships and to quantify relationshi
ps between fertility and climatic indicators. The timing of fertility
indicator cycles at the equator shows little (obliquity band) or no (o
ther orbital bands) coincidence with monsoon proxies of the Arabian Se
a. At the equator, fertility responses are dissociated, and present im
portant leads or lags with ETP signal at the three orbital bands (with
the exception of the thermocline foraminifera, in phase with maximum
eccentricity). Due to significant leads with ETP in the timing of C-13
minima and URI cycles, no relationships with the Northern Hemisphere
radiation can be deduced. At the obliquity and precessional frequency
bands, thermocline foraminifera cycles display significant lag with ET
P and ice volume minima, which suggests that radiation is not the sole
forcing mechanism. Global climatic and ice volume changes may be an i
mportant forcing mechanism for these fertility proxies. The G. bulloid
es record is more complicated with cycles in phase with Arabian Sea mo
nsoon proxies at the obliquity band, and O-18 minima at the precession
frequency. It appears that, at the equator, the southwest monsoon win
ds are not the main force driving radiolarian and foraminiferal produc
tivity.