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<p>Abstract Census counts of benthic foraminifera were studied from the \SW\ Iberian Margin to reconstruct past changes in deep-water hydrography across Terminations I and II. Detailed benthic faunal data (\&gt; 125 μm size-fraction) allow us to evaluate the limitations imposed by taphonomic processes and restricted size-fractions. The comparison of recent (mudline) and fossil assemblages at \.IODP\ Site \U1385\ indicates the quick post-mortem disintegration of shells of astrorhizoid taxa (\&nbsp; 80\% of the present-day fauna), resulting in impoverished fossil assemblages. While the application of quantitative proxy methods is problematic under these circumstances, the fossil assemblages can still provide a qualitative palaeoenvironmental signal that, while most fully expressed in the 125\textendash212 μm size-fraction, is nonetheless also expressed to some degree in the \&gt; 212 μm size-fraction. Variations in the benthic foraminiferal assemblages reveal information about changing organic matter supply, deep-water oxygenation and temperature. \MIS\ 2 is generally characterized by an elevated trophic state and variable oxic conditions, with oxygenation minima culminating in the Younger Dryas (YD) and Heinrich Stadials (HS) 1, 2 and 3. Low oxic conditions coincide with decreased water-temperature and lower benthic δ13C, pointing to the strong influence of a southern sourced water-mass during these periods. \HS\ 1 is the most extreme of these intervals, providing further evidence for a severe temporary reduction or even shutdown of AMOC. With the inception of \MIS\ 1, organic matter supply reduced and a better ventilated deep-water environment bathed by \NEADW\ is established. For Termination II, clear indications of southern-sourced water are limited to the early phase of \HS\ 11. During the latter part of \HS\ 11, the deep-water environment seems to be determined by strongly increased supply of organic matter, potentially explaining the decoupling of benthic δ13C and Mg/Ca records of earlier studies as a phytodetritus effect on the carbon isotope signal. However, the presence of a warm, nutrient-rich and poorly oxygenated water-mass cannot be ruled out. With the inception of interglacial \MIS\ 5e trophic conditions are reduced and ventilation by \NEADW\ increases.</p>

Year of Publication
2015
Journal
Global and Planetary Change
Volume
131
Number of Pages
174-191
ISSN Number
0921-8181
URL
http://www.sciencedirect.com/science/article/pii/S0921818115001125
DOI
http://dx.doi.org/10.1016/j.gloplacha.2015.06.002
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