This study presents the reconstructed evolution of sea surface conditions in
the central-western Mediterranean Sea during the late Holocene (2700 years)
from a set of multi-proxy records as measured on five short sediment cores
from two sites north of Minorca (cores MINMC06 and HER-MC-MR3). Sea surface
temperatures (SSTs) from alkenones and Globigerina bulloides Mg / Ca ratios are combined with
δ18O measurements in order to reconstruct changes in the
regional evaporation–precipitation (E–P) balance. We also revisit the G. bulloides
Mg / Ca–SST calibration and re-adjusted it based on a set of core-top
measurements from the western Mediterranean Sea. Modern regional
oceanographic data indicate that Globigerina bulloides Mg / Ca is mainly controlled by seasonal
spring SST conditions, related to the April–May primary productivity bloom
in the region. In contrast, the alkenone–SST signal represents an integration
of the annual signal.
The construction of a robust chronological framework in the region allows
for the synchronization of the different core sites and the construction of
“stacked” proxy records in order to identify the most significant climatic
variability patterns. The warmest sustained period occurred during the Roman
Period (RP), which was immediately followed by a general cooling trend
interrupted by several centennial-scale oscillations. We propose that this
general cooling trend could be controlled by changes in the annual mean
insolation. Even though some particularly warm SST intervals took place
during the Medieval Climate Anomaly (MCA), the Little Ice Age (LIA) was
markedly unstable, with some very cold SST events mostly during its second
half. Finally, proxy records for the last centuries suggest that relatively
low E–P ratios and cold SSTs dominated during negative North Atlantic
Oscillation (NAO) phases, although SSTs seem to present a positive
connection with the Atlantic Multidecadal Oscillation (AMO) index
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