Abstract. Coccolithophores contribute significantly to marine
primary productivity and play a unique role in ocean biogeochemistry by
using carbon for photosynthesis (soft-tissue pump) and for calcification
(carbonate counter pump). Despite the importance of including
coccolithophores in Earth system models to allow better predictions of the
climate system's responses to planetary change, the reconstruction of
coccolithophore productivity mostly relied on proxies dependent on
accumulation and sedimentation rates and preservation conditions. In this
study we used an independent proxy, based on the coccolith fraction (CF)
Sr∕Ca ratio, to reconstruct coccolithophore productivity. We studied the
marine sediment core MD03-2699 from the western Iberian margin (IbM),
concentrating on glacial–interglacial cycles of Marine Isotopic Stage (MIS)
12 to MIS 9. We found that IbM coccolithophore productivity was controlled
by changes in the oceanographic conditions, such as in sea surface
temperature (SST) and nutrient availability, and by competition with other
phytoplankton groups. Long-term coccolithophore productivity was primarily
affected by variations in the dominant surface water mass. Polar and
subpolar surface waters during glacial substages were associated with
decreased coccolithophore productivity, with the strongest productivity minima
concomitant with Heinrich-type events (HtEs). Subtropical, nutrient-poorer
waters, increased terrigenous input, and moderate to strong upwelling during
the deglaciation and early MIS11 are hypothesized to have attributed a
competitive advantage to diatoms to the detriment of coccolithophores, resulting
in intermediate coccolithophore productivity levels. During the progression
towards full glacial conditions an increasing presence of nutrient-richer
waters, related to the growing influence of transitional surface waters and/or
intensified upwelling, probably stimulated coccolithophore productivity to
maxima following the rapid depletion of silica by diatoms. We present
conceptual models of the carbon and carbonate cycle components for the IbM
in different time slices that might serve as a basis for further
investigation and modelling experiments.