Abstract. Sea surface salinity is one of the most important parameters to
reconstruct in paleoclimatology, reflecting amongst other things the hydrological
cycle, paleodensity, ice volume, and regional and global circulation of
water masses. Recent culture studies and a Red Sea field study revealed a
significant positive relation between salinity and Na incorporation within
benthic and planktonic foraminiferal shells. However, these studies reported
varying partitioning of Na between and within the same species. The latter
could be associated with ontogenetic variations, most likely spine loss.
Varying Na concentrations were observed in different parts of foraminiferal
shells, with spines and regions close to the primary organic
sheet being especially enriched in Na. In this study, we unravel the Na composition of
different components of the planktonic foraminiferal shell wall using
electron probe micro-analysis (EPMA) and solution ICP-MS. A model is
presented to interpret EPMA data for spines and spine bases to
quantitatively assess differences in composition and contribution to whole-shell Na∕Ca signals. The same model can also be applied to other spatial
inhomogeneities observed in foraminiferal shell chemistry, like elemental
(e.g., Mg, Na, S) banding and/or hotspots. The relative contribution of shell
carbonate, organic linings, spines and spine bases to whole-shell Na
chemistry is considered quantitatively. This study shows that whereas the
high Na areas may be susceptible to taphonomic alterations, the Na chemistry
of the shell itself seems relatively robust. Comparing both shell and spine
Na∕Ca values with salinity shows that shell chemistry records salinity,
albeit with a very modest slope.