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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" dtd-version="3.0"><?xmltex \makeatother\@nolinetrue\makeatletter?>
  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">CP</journal-id>
<journal-title-group>
<journal-title>Climate of the Past</journal-title>
<abbrev-journal-title abbrev-type="publisher">CP</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Clim. Past</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1814-9332</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/cp-13-345-2017</article-id><title-group><article-title><inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C decreases in the upper western South Atlantic during Heinrich
Stadials 3 and 2</article-title>
      </title-group><?xmltex \runningtitle{$\delta^{{13}}$C decreases in the upper western South Atlantic}?><?xmltex \runningauthor{M. C. Campos et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Campos</surname><given-names>Marília C.</given-names></name>
          <email>marilia.carvalho.campos@usp.br</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Chiessi</surname><given-names>Cristiano M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3318-8022</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Voigt</surname><given-names>Ines</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff4">
          <name><surname>Piola</surname><given-names>Alberto R.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Kuhnert</surname><given-names>Henning</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Mulitza</surname><given-names>Stefan</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>School of Arts, Sciences and Humanities, University of São Paulo,
São Paulo, 03828-000, Brazil</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>MARUM – Center for Marine Environmental Sciences, University of
Bremen, Bremen, 28359, Germany</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Servicio de Hidrografia Naval (SHN), Buenos Aires, C1270ABV, Argentina</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Dept. Ciencias de la Atmósfera y los Océanos, FCEN,
Universidad de Buenos Aires, C1428 EHA, and Instituto
Franco–Argentino sobre Estudios de Clima y sus Impactos,
CNRS/CONICET, C1428EGA, Argentina</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Marília C. Campos (marilia.carvalho.campos@usp.br)</corresp></author-notes><pub-date><day>18</day><month>April</month><year>2017</year></pub-date>
      
      <volume>13</volume>
      <issue>4</issue>
      <fpage>345</fpage><lpage>358</lpage>
      <history>
        <date date-type="received"><day>1</day><month>June</month><year>2016</year></date>
           <date date-type="rev-request"><day>20</day><month>June</month><year>2016</year></date>
           <date date-type="rev-recd"><day>22</day><month>February</month><year>2017</year></date>
           <date date-type="accepted"><day>16</day><month>March</month><year>2017</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://cp.copernicus.org/articles/13/345/2017/cp-13-345-2017.html">This article is available from https://cp.copernicus.org/articles/13/345/2017/cp-13-345-2017.html</self-uri>
<self-uri xlink:href="https://cp.copernicus.org/articles/13/345/2017/cp-13-345-2017.pdf">The full text article is available as a PDF file from https://cp.copernicus.org/articles/13/345/2017/cp-13-345-2017.pdf</self-uri>


      <abstract>
    <p>Abrupt millennial-scale climate change events
of the last deglaciation (i.e. Heinrich Stadial 1 and the Younger Dryas)
were accompanied by marked increases in atmospheric CO<inline-formula><mml:math id="M2" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (CO<inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
and decreases in its stable carbon isotopic ratios (<inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C),
i.e. <inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M6" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>, presumably due to outgassing from the
ocean. However, information on the preceding Heinrich Stadials during the
last glacial period is scarce. Here we present <inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C records
from two species of planktonic foraminifera from the western South Atlantic
that reveal major decreases (up to 1 ‰) during Heinrich
Stadials 3 and 2. These <inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C decreases are most likely related
to millennial-scale periods of weakening of the Atlantic
meridional overturning circulation and the consequent increase (decrease) in
CO<inline-formula><mml:math id="M9" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. We hypothesise two mechanisms
that could account for the decreases observed in our records, namely
strengthening of Southern Ocean deep-water ventilation and weakening of the
biological pump. Additionally, we suggest that air–sea gas
exchange could have contributed to the observed <inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C decreases.
Together with other lines of evidence, our data are consistent with the
hypothesis that the CO<inline-formula><mml:math id="M13" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> added to the atmosphere during abrupt
millennial-scale climate change events of the last glacial period
also originated in the ocean and reached the atmosphere by outgassing. The
temporal evolution of <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C during Heinrich Stadials 3 and 2 in
our records is characterized by two relative minima separated by a relative
maximum. This “w structure” is also found in North Atlantic and
South American records, further suggesting that such a structure is a
pervasive feature of Heinrich Stadial 2 and, possibly, also Heinrich Stadial 3.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>Heinrich Stadials (HS) are abrupt millennial-scale climate change
events marked by an anti-phase interhemispheric temperature pattern, which is
usually termed the bipolar seesaw (Broecker, 1998). One widely accepted
mechanism for the bipolar seesaw is related to changes in the strength of
the Atlantic meridional overturning circulation (AMOC), likely caused by
freshwater input into high latitudes of the North Atlantic (Mix et al.,
1986; Crowley, 1992; Stocker, 1998). During HS, a weak AMOC occurred
simultaneously with cooling in the high latitudes of the surface North
Atlantic (Sachs and Lehman, 1999; Bard et al., 2000), warming of the surface
South Atlantic (Barker et al., 2009; Chiessi et al., 2015), a southward
migration of the Intertropical Convergence Zone (ITCZ) (Arz et al., 1998;
Deplazes et al., 2013), strengthening of the South American monsoon system
(SAMS) (Cruz et al., 2006; Kanner et al., 2012), and an increase in
atmospheric CO<inline-formula><mml:math id="M15" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (CO<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> (Ahn and Brook, 2008,
2014). This increase in CO<inline-formula><mml:math id="M17" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> was accompanied by a decrease in its
stable carbon isotopic composition (<inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, at least
for some HS (Eggleston et al., 2016). It has been suggested that the origin
of the CO<inline-formula><mml:math id="M20" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> rise and the associated <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M22" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>
decrease was ocean-sourced (Schmittner and Galbraith, 2008;
Anderson et al., 2009; Denton et al., 2010; Mariotti et al., 2016; Eggleston
et al., 2016; Hertzberg et al., 2016). The occurrence of stable carbon
isotope (<inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C) minima during HS1 (last deglaciation) in
planktonic foraminiferal records from the Indo-Pacific Ocean,
Southern Ocean, and South Atlantic Ocean (Oppo and Fairbanks, 1989;
Ninnemann and Charles, 1997; Mulitza et al., 1999; Spero and Lea, 2002)
suggests that the signal originated from the ocean region most directly
connected to all major oceanic basins, i.e. the Southern Ocean (Ninnemann
and Charles, 1997). Under a weak AMOC, wind-driven upwelling of
the Circumpolar Deep Water (CDW) in the Southern Ocean would become
stronger, reducing the stratification of the Southern Ocean and enhancing
outgassing of low-<inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C CO<inline-formula><mml:math id="M25" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to the atmosphere
(Anderson et al., 2009; Denton et al., 2010; Tschumi et al., 2011; Bauska et al., 2016). However, model experiments (e.g. Schmittner and Galbraith, 2008;
Schmittner and Lund, 2015) and records from different ocean basins (e.g.
Tessin and Lund, 2013; Lund et al., 2015; Curry and Oppo, 2005; Hertzberg et
al., 2016) suggest that the increase in CO<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and decrease in
<inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> during HS1 are instead related to the weakening
of the global oceanic biological pump and the consequent accumulation of
<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula>C-depleted CO<inline-formula><mml:math id="M30" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the upper water column. Such
anomalously low <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> would then reach the
atmosphere via air–sea gas exchange.</p>
      <p>The reduction of the upper water column <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C caused by one or
both of the mechanisms described above may be a common feature of other HS
as well but so far planktonic foraminiferal <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C records
corroborating this assumption often only cover the abrupt
millennial-scale climate change events of the last deglaciation
(i.e. HS1 and the Younger Dryas), while high-temporal-resolution information
on the HS of the last glacial period is still scarce (Oppo and Fairbanks,
1989; Ninnemann and Charles, 1997; Spero and Lea, 2002; Hertzberg et al.,
2016). Here we investigate this issue for HS3 and HS2 using planktonic
foraminiferal (<italic>Globigerinoides ruber </italic>white (<italic>G. ruber </italic>w) and <italic>Globorotalia inflata</italic> (<italic>G. inflata</italic>)) <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C data from a high
temporal resolution marine sediment core (GeoB6212-1), collected near
32<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S off southeastern South America (SESA). Our data
suggest that HS3 and HS2 were also marked by significant <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
decreases in the upper water column.</p>
</sec>
<sec id="Ch1.S2">
  <title>Regional setting</title>
      <p>The upper water column of the study area is dominated by the southward-flowing Brazil Current (BC), which forms the western branch of the South
Atlantic subtropical gyre. The BC is one of the weakest western boundary
currents in the world ocean (Peterson and Stramma, 1991), carrying warm,
saline, and nutrient-depleted subtropical waters southward (Olson
et al., 1988). The BC originates near 10–15<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S from the
bifurcation of the Southern South Equatorial Current as it approaches the
western slope of the Brazil Basin (Stramma et al., 1990; Peterson and
Stramma, 1991). Around 38<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S the BC encounters the northward-flowing Malvinas Current (MC), where the opposing flows turn
southeast and flow offshore, the so-called Brazil–Malvinas
Confluence. The Brazil–Malvinas Confluence is characterized by intense
mesoscale variability. After collision and considerable mixing, the
warm and salty BC fractions flow eastward as the South Atlantic
Current (Olson et al., 1988; Peterson and Stramma, 1991), while the majority
of the cold and fresh MC waters veer southeastward to rejoin the Antarctic
Circumpolar Current.</p>
      <p>In the study area, the BC transports Tropical Surface Water (TW), South Atlantic Central Water (SACW), and Antarctic
Intermediate Water (AAIW). TW occupies the mixed layer, i.e. the upper ca.
100 m of the water column, with a mean temperature of 20 <inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and a
mean salinity of 36 psu (Tsuchiya et al., 1994). TW originates in the
tropic–subtropic transition region by subduction, creating a subsurface
salinity maximum capping the central waters (Mémery et al., 2000; Tomczak
and Godfrey, 2003) (Fig. 1).</p>
      <p>SACW occupies the permanent thermocline from ca. 100 to 500 m water depth.
Its temperature ranges from 6 to 20 <inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and its salinity spans
from 34.6 to 36 psu (Mémery et al., 2000). Two types of SACW have been
identified (Stramma et al., 2003). The low-density type of SACW
that is mainly found in the South Atlantic subtropical gyre is formed by
subduction of a low-density type of Subantarctic Mode Water (SAMW)
along the southern edge of the gyre (Stramma and England, 1999). The denser
variety of SACW originates in the southern Indian Ocean and is brought into the
South Atlantic by the Agulhas Current (Sprintall and Tomczak, 1993) (Fig. 1).</p>
      <p>Just below the permanent thermocline, AAIW occupies the water column from
ca. 500 to 1200 m water depth (Stramma and England, 1999). AAIW is
characterized as a cold and low-salinity water mass (Piola and Georgi, 1982;
Tomczak and Godfrey, 2003). Around the southern tip of South America, AAIW
originates from subduction of cold and fresh Antarctic Surface Water across
the Antarctic Polar Front and from contribution of a dense type of SAMW that
originates from deep winter convection in the Subantarctic Zone (Molinelli,
1981; Naveira Garabato et al., 2009). AAIW is advected eastward through the
Drake Passage by the Antarctic Circumpolar Current and turns northwards with
the MC into the South Atlantic (Piola and Gordon, 1989). Since AAIW
circulation follows the anticyclonic flow of the subtropical gyre, the
majority of the northward flow at mid-latitude occurs in the eastern basin
(McCartney, 1977; Stramma and England, 1999; Tomczak and Godfrey, 2003).
However, intense mixing in the Brazil–Malvinas Confluence also leads to
direct northward flow in the western South Atlantic that can, to some
extent, influence the dissolved inorganic carbon <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C (<inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in the formation region of SACW (e.g. Piola and Georgi,
1982) (Figs. 1 and 2).</p>
      <p>In the modern South Atlantic, the distribution of <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M46" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula>
allows the identification of its major water masses. TW and SACW show high
<inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M48" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula> values of ca. 2 ‰. AAIW
presents <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M50" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula> values of ca. 0.7 ‰.
North Atlantic Deep Water (NADW) derives from the North Atlantic and shows <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M52" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula>
values of ca. 1 ‰. In the southwest South Atlantic, NADW
is sandwiched between Upper and Lower CDW, which present <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M54" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula> values of ca. 0.4 ‰ (Kroopnick, 1985).
Since planktonic foraminiferal <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C reflects the <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M57" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula> of the ambient seawater, we use it as a proxy for the past
oceanic carbon system (Mulitza et al., 1999; Spero, 1992). However, other
factors such as calcification temperature, carbonate ion concentration,
symbiont activity, and air–sea gas exchange may also influence
planktonic foraminiferal <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C with modification by vital
effects (Lynch-Stieglitz et al., 1995; Spero and Lea, 1996; Spero et al.,
1997; Bemis et al., 2000).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Schematic representation of the large-scale circulation
of South Atlantic Central Water (SACW) (Stramma and England, 1999). The main
SACW source region is depicted by the gridded green ellipse, and the main
source region of Tropical Surface Water (TW) is indicated by the dotted
yellow ellipse. Mean annual temperature at 300 m water depth is shown by the
colour shading (Locarnini et al., 2013) (<uri>http://odv.awi.de</uri>).</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/13/345/2017/cp-13-345-2017-f01.png"/>

      </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>Accelerator mass spectrometer radiocarbon dates and
calibrated ages used to construct the age model of core GeoB6212-1.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.95}[.95]?><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1">Core</oasis:entry>  
         <oasis:entry colname="col2">Lab ID</oasis:entry>  
         <oasis:entry colname="col3">Species</oasis:entry>  
         <oasis:entry colname="col4">Radiocarbon age</oasis:entry>  
         <oasis:entry colname="col5">Calibrated</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">depth (cm)</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M61" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1<inline-formula><mml:math id="M62" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> error (a BP)</oasis:entry>  
         <oasis:entry colname="col5">ages (cal a BP)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">8</oasis:entry>  
         <oasis:entry colname="col2">Poz-47236<inline-formula><mml:math id="M63" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3"><italic>G. ruber</italic></oasis:entry>  
         <oasis:entry colname="col4">5250 <inline-formula><mml:math id="M64" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 40</oasis:entry>  
         <oasis:entry colname="col5">5929</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">33</oasis:entry>  
         <oasis:entry colname="col2">382580<inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3"><italic>G. ruber</italic></oasis:entry>  
         <oasis:entry colname="col4">9440 <inline-formula><mml:math id="M66" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 40</oasis:entry>  
         <oasis:entry colname="col5">10 047</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">58</oasis:entry>  
         <oasis:entry colname="col2">Poz-47237<inline-formula><mml:math id="M67" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3"><italic>G. ruber</italic></oasis:entry>  
         <oasis:entry colname="col4">10 250 <inline-formula><mml:math id="M68" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 50</oasis:entry>  
         <oasis:entry colname="col5">11 395</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">113</oasis:entry>  
         <oasis:entry colname="col2">382581<inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Planktonic forams</oasis:entry>  
         <oasis:entry colname="col4">12 870 <inline-formula><mml:math id="M70" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 50</oasis:entry>  
         <oasis:entry colname="col5">14 342</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">158</oasis:entry>  
         <oasis:entry colname="col2">Poz-47238<inline-formula><mml:math id="M71" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Planktonic forams</oasis:entry>  
         <oasis:entry colname="col4">13 050 <inline-formula><mml:math id="M72" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 70</oasis:entry>  
         <oasis:entry colname="col5">15 247</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">253</oasis:entry>  
         <oasis:entry colname="col2">382582<inline-formula><mml:math id="M73" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Planktonic forams</oasis:entry>  
         <oasis:entry colname="col4">15 750 <inline-formula><mml:math id="M74" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 50</oasis:entry>  
         <oasis:entry colname="col5">18 620</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">323</oasis:entry>  
         <oasis:entry colname="col2">382583<inline-formula><mml:math id="M75" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Planktonic forams</oasis:entry>  
         <oasis:entry colname="col4">17 560 <inline-formula><mml:math id="M76" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 60</oasis:entry>  
         <oasis:entry colname="col5">20 748</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">363</oasis:entry>  
         <oasis:entry colname="col2">Poz-47239<inline-formula><mml:math id="M77" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Planktonic forams</oasis:entry>  
         <oasis:entry colname="col4">18 610 <inline-formula><mml:math id="M78" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 140</oasis:entry>  
         <oasis:entry colname="col5">21 834</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">478</oasis:entry>  
         <oasis:entry colname="col2">382584<inline-formula><mml:math id="M79" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Planktonic forams</oasis:entry>  
         <oasis:entry colname="col4">19 810 <inline-formula><mml:math id="M80" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 70</oasis:entry>  
         <oasis:entry colname="col5">23 537</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">578</oasis:entry>  
         <oasis:entry colname="col2">Poz-47240<inline-formula><mml:math id="M81" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Planktonic forams</oasis:entry>  
         <oasis:entry colname="col4">21 750 <inline-formula><mml:math id="M82" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 150</oasis:entry>  
         <oasis:entry colname="col5">25 587</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">623</oasis:entry>  
         <oasis:entry colname="col2">382585<inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Planktonic forams</oasis:entry>  
         <oasis:entry colname="col4">22 320 <inline-formula><mml:math id="M84" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 80</oasis:entry>  
         <oasis:entry colname="col5">26 184</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">668</oasis:entry>  
         <oasis:entry colname="col2">382586<inline-formula><mml:math id="M85" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Planktonic forams</oasis:entry>  
         <oasis:entry colname="col4">22 480 <inline-formula><mml:math id="M86" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 80</oasis:entry>  
         <oasis:entry colname="col5">26 711</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">717</oasis:entry>  
         <oasis:entry colname="col2">424077<inline-formula><mml:math id="M87" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Planktonic forams</oasis:entry>  
         <oasis:entry colname="col4">24 190 <inline-formula><mml:math id="M88" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 110</oasis:entry>  
         <oasis:entry colname="col5">27 850</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">768</oasis:entry>  
         <oasis:entry colname="col2">382587<inline-formula><mml:math id="M89" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Planktonic forams</oasis:entry>  
         <oasis:entry colname="col4">29 520 <inline-formula><mml:math id="M90" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 160</oasis:entry>  
         <oasis:entry colname="col5">31 966</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table><table-wrap-foot><p><inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula> Poz: Poznań Radiocarbon Laboratory, Poznań, Poland.<?xmltex \hack{\\}?><inline-formula><mml:math id="M60" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> Beta Analytic Radiocarbon Dating Laboratory, Miami, USA.</p></table-wrap-foot></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p>Schematic representation of ventilation and subduction of water
masses in the Southern Ocean (modified after Anderson et al., 2009).
Wind-driven upwelling south of the latitude of maximum westerlies
brings Circumpolar Deep Water (CDW) to the surface and contributes to
Antarctic Surface Waters. Antarctic Surface Waters represent the dominant
source of the upper and intermediate waters that leave the Southern Ocean.
Antarctic Intermediate Water (AAIW) originates from subduction of cold and
fresh Antarctic Surface Waters across the Antarctic Polar Front (APF) and
enters the South Atlantic mainly via the subtropical gyre. Subantarctic Mode
Water (SAMW) originates from deep winter convection north of the
Subantarctic Front (SAF). A low-density type of SAMW enters the
thermocline of the Southern Hemisphere oceans along the southern edge of the
subtropical gyres where it becomes part of central waters and contributes to
ventilating the thermocline, while a denser type of SAMW formed in the
eastern South Pacific is regarded as a precursor of the AAIW. The Polar
Front Zone (PFZ) and Subantarctic Zone (SAZ) are the regions between the APF
and SAF and between the SAF and Subtropical Front (STF) respectively.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/13/345/2017/cp-13-345-2017-f02.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Age model (left-hand side <inline-formula><mml:math id="M91" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis; red line and black
enveloping curves) and sedimentation rates (right-hand side
<inline-formula><mml:math id="M92" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis; grey line) for marine sediment core GeoB6212-1 produced
with the software Bacon 2.2 (Blaauw and Christen, 2011). For the age model,
the red symbols show calibrated ages, the red line depicts mean ages, and the
upper (lower) black line depicts maximum (minimum) ages. Grey vertical bars
show abrupt millennial-scale climate change events Heinrich
Stadial 3 (HS3) and Heinrich Stadial 2 (HS2) (Goni and Harrison, 2010;
Sarnthein et al., 2001).</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/13/345/2017/cp-13-345-2017-f03.png"/>

      </fig>

      <p>Changes in upper ocean properties and circulation patterns are also closely
associated with changes in the atmospheric circulation. Positive sea surface
temperature (SST) anomalies in the western South Atlantic, likely associated
with changes in the strength of the AMOC (Knight et al., 2005), have been
correlated with positive anomalies in the strength of the SAMS and,
consequently, with the increase in precipitation over SESA (Chaves and
Nobre, 2004). The SAMS and its main components – the ITCZ, the South
Atlantic Convergence Zone (SACZ), and the South American low-level jet
(SALLJ) – are the main atmospheric drivers of the hydroclimate of tropical
and subtropical SESA to the east of the Andes (Garreaud et al., 2009). The
ITCZ is a global convective belt in the equatorial region, and the SACZ is
an elongate NW–SE convective belt that originates in the Amazon Basin and
extends southeastward above the northern portion of SESA and the adjacent
subtropical South Atlantic. The SALLJ is a NW–SE humidity flux from the west
Amazon Basin to the subtropical region of SESA (Zhou and Lau, 1998; Carvalho
et al., 2004). This southward water vapour flux is a crucial source of
precipitation to the Plata River drainage basin (Berbery and Barros, 2002),
which is a source of continental-borne sediments to our core site.</p>
</sec>
<sec id="Ch1.S3">
  <title>Materials and methods</title>
<sec id="Ch1.S3.SS1">
  <title>Marine sediment core</title>
      <p>We investigated sediment core GeoB6212-1 (32.41<inline-formula><mml:math id="M93" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S,
50.06<inline-formula><mml:math id="M94" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W, 1010 m water depth, 790 cm core length) (Schulz et al.,
2001) collected from the continental slope off SESA where the upper water
column is under the influence of the BC, and thus the TW and SACW (Fig. 1).
This gravity core was raised at the Rio Grande Cone, a major sedimentary
feature in the western Argentine Basin. As our study focuses on HS3 and HS2,
we analysed the section from the bottom of the core (768 cm core depth; ca.
32 cal ka BP) up to 290 cm core depth (ca. 20 cal ka BP). Visual core
inspection provided evidence for the presence of sand lenses at 330 and 368 cm core depth (Schulz et al., 2001; Wefer et al., 2001). Therefore, we did
not sample these depths. The section of interest of GeoB6212-1 was sampled
every 2.5 cm with syringes of 10 cm<inline-formula><mml:math id="M95" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>. All samples were wet-sieved,
oven-dried at 50 <inline-formula><mml:math id="M96" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and the fraction larger than 150 <inline-formula><mml:math id="M97" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m was stored in glass vials for subsequent analyses.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Age model</title>
      <p>The age model of core GeoB6212-1 is based on 14 accelerator mass spectrometry radiocarbon ages from
planktonic foraminifera (mixed-layer and thermocline species) (Table 1, Fig. 3). For each sample, we hand-picked under a binocular microscope
around 10 mg of planktonic foraminifera shells from the sediment fraction
larger than 150 <inline-formula><mml:math id="M98" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m. Samples were analysed at the Poznań Radiocarbon
Laboratory, Poland, and at the Beta Analytic Radiocarbon Dating Laboratory,
USA (Table 1). All radiocarbon ages were calibrated with the calibration
curve IntCal13 (Reimer et al., 2013) with the software Bacon 2.2 (Blaauw and
Christen, 2011). A marine reservoir correction of 400 years was applied with
associated error of 100 years (Bard, 1988). All ages are reported as
calibrated years before present (cal a BP; present is 1950 AD). To construct
the age model we used Bayesian statistics in the software Bacon 2.2 (Blaauw
and Christen, 2011). With the exception of mem.mean (set to 0.4) and
acc.shape (set to 0.5), default parameters were used. Radiocarbon ages were
assumed to be <inline-formula><mml:math id="M99" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>-distributed with 9<inline-formula><mml:math id="M100" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> of freedom (<inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>.</mml:mo><mml:mi>a</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">9</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>.</mml:mo><mml:mi>b</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula>).
Mean ages and 95 % error margins were estimated from 10 000 downcore
age–depth realizations at 0.5 cm resolution (Fig. 3).</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S3.SS3">
  <title>Stable carbon isotope analyses</title>
      <p>Around 10 tests of <italic>G. ruber</italic> w sensu stricto (Wang, 2000) within the size range 250–350 <inline-formula><mml:math id="M103" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m
and 8 tests of <italic>G. inflata</italic> non-encrusted with three chambers in the final whorl
(Groeneveld and Chiessi, 2011) within the size range 315–400 <inline-formula><mml:math id="M104" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m were
hand-picked under a binocular microscope every 2.5 cm from 290 to
768 cm core depth. While the first species records the conditions at the top
of the mixed layer (down to ca. 30 m) (Chiessi et al., 2007; Wang, 2000),
the second species records the conditions at the permanent thermocline (ca.
350–400 m) (Groeneveld and Chiessi, 2011), allowing the reconstruction of
the <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C signal of the TW and the SACW respectively. The
<inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C analyses were performed on a Finnigan MAT 252 mass
spectrometer equipped with an automatic carbonate preparation device at the
MARUM – Centre for Marine Environmental Sciences, University of Bremen,
Germany. Isotopic results are reported in the usual delta notation
relative to the Vienna Peedee belemnite. Data were calibrated against the
house standard (Solnhofen limestone), itself calibrated against the NBS19
standard. The standard deviation of the laboratory standard was lower than
0.05 ‰ for the measuring period.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <title>Results</title>
<sec id="Ch1.S4.SS1">
  <title>Age model and sedimentation rates</title>
      <p>Our age model covers the period between 32 and 6 cal ka BP (Table 1, Fig. 3). Sedimentation rates change markedly during this time interval, with
values ranging from 5 to 91 cm ka<inline-formula><mml:math id="M107" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. Three main peaks in sedimentation
rate were identified at ca. 26, 23, and 15 and one minor peak at 11 cal ka BP. The two oldest sedimentation peaks occur within our period of interest
(i.e. from ca. 32 until 20 cal ka BP) (Fig. 3). The mean temporal
resolution of our <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C records is ca. 90 years, with values ranging
from 28 to 195 years.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S4.SS2">
  <?xmltex \opttitle{Stable carbon isotope values of \textit{G. ruber} and \textit{G.
inflata}}?><title>Stable carbon isotope values of <italic>G. ruber</italic> and <italic>G. inflata</italic></title>
      <p>The <italic>G. ruber </italic>w <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C record shows two long-term decreases, from
ca. 32 to 28.2 cal ka BP with an amplitude of ca. 1 ‰,
and from ca. 26.5 to 24.9 cal ka BP also with an amplitude of ca.
1 ‰ (Fig. 4a). These two negative long-term
trends are separated from each other by an abrupt increase of ca.
1.3 ‰ ending at ca. 27.2 cal ka BP. Both
long-term decreases were interrupted by brief positive excursions,
one from 29.3 to 29.1 cal ka BP with an amplitude of ca.
0.7 ‰ and another from ca. 26.2 to 25.8 cal ka BP with an
amplitude of ca. 1 ‰. After the second
long-term decrease, the <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values of <italic>G. ruber</italic> w varied
around 0.7 ‰. Both long-term negative
excursions determine a pattern we refer to as “w structure”.</p>
      <p>The <italic>G. inflata</italic> <inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C record shows four negative excursions departing from
a baseline of ca. 0.8 ‰ (Fig. 4b). The first occurs from
ca. 31.5 to 29.3 cal ka BP with an amplitude of ca. 0.5 ‰
, the second from ca. 28.8 to 28 cal ka BP with the same amplitude, the
third from ca. 26.5 to 26.4 cal ka BP with an amplitude of ca.
0.8 ‰, and the forth from ca. 25.8 to 24.4 cal ka BP
with an amplitude of ca. 0.9 ‰. Also, in the <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C record from <italic>G. inflata</italic> two w structures are present and are
defined by the previously described negative excursions.</p>
      <p>The w structures and the <inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C minima are
synchronous for both species (Fig. 4).</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <title>Discussion</title>
      <p>The synchronous w structures present in the <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
records of both planktonic foraminiferal species analysed here occur
coeval with the millennial-scale event HS2 and, despite the
slight offset that is attributed to age model uncertainties, also with HS3
(Sarnthein et al., 2001; Goni and Harrison, 2010) (Fig. 4). Concomitantly, a
weak AMOC was described based on <inline-formula><mml:math id="M115" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">231</mml:mn></mml:msup></mml:math></inline-formula>Pa <inline-formula><mml:math id="M116" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M117" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">230</mml:mn></mml:msup></mml:math></inline-formula>Th records from the
Bermuda Rise (Ocean Drilling Program (ODP) site 1063; 33.7<inline-formula><mml:math id="M118" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 57.6<inline-formula><mml:math id="M119" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W) (Lippold
et al., 2009) (Fig. 5d). Both events are also marked by pulses of ice-rafted
debris (IRD) (MD99-2331; 42.2<inline-formula><mml:math id="M120" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 9.7<inline-formula><mml:math id="M121" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W) (Eynaud et
al., 2009) and by decreases in SST (SU8118 and MD952042; 37.5<inline-formula><mml:math id="M122" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
10.1<inline-formula><mml:math id="M123" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W) (Bard, 2000) in the northeastern North
Atlantic (Iberian Margin). The Greenland GISP2 ice core (72.6<inline-formula><mml:math id="M124" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
38.5<inline-formula><mml:math id="M125" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W) shows synchronous increases in Ca<inline-formula><mml:math id="M126" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, indicating
changes in atmospheric circulation over Greenland (Mayewski et al., 1997)
(Fig. 5a, b, c). It is noteworthy that the four records (i.e. Fig. 5a, b,
c, d) mentioned above also show a w structure during HS2,
similar to the one shown in our <inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C records. The IRD (Eynaud
et al., 2009) and Ca<inline-formula><mml:math id="M128" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (Mayewski et al., 1997) records also show a
w structure similar to ours during HS3.</p>
      <p>Based on modern conditions, we expect our core site not to be significantly
influenced by changes in the local nutrient content of the upper water
column since the region is dominated by the oligotrophic BC, characteristic
of western boundary currents, and is far from upwelling cells (Brandini et
al., 2000). Thus, it is unlikely that changes in our <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
records are associated with local productive events driven by
nutrient-cycle processes (Mulitza et al., 1999).</p>
      <p>During HS, we expect warmer temperatures to have occurred in the upper water
column of the western South Atlantic (Barker et al., 2009; Chiessi et al., 2015). This would trigger an increase in <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values of the
symbiont-bearing species investigated here if calcification temperature
dominated the <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C signal (Bemis et al., 2000), which is
not the case (Fig. 4a). Additionally, given the lack of regional upper ocean
reconstructions for carbonate ion concentration, we assume that increased
CO<inline-formula><mml:math id="M132" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> that is frequently associated with HS (Ahn and Brook, 2008, 2014) would have been accompanied by a decrease in sea surface
carbonate ion concentration (Broecker and Peng, 1993). This would promote an
increase in the <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M134" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula>, but our records show a negative
<inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C anomaly (Fig. 4). Furthermore, we analysed a
symbiont-bearing and a facultative-symbiont species (i.e. <italic>G. ruber</italic> w and <italic>G. inflata</italic>,
respectively) and both records show a similar pattern (Fig. 4), indicating
that changes in symbiont activity can also be disregarded as a factor
influencing our results (Spero et al., 1997; Bemis et al., 2000). We propose
two primary mechanisms to explain our <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C decreases: (i)
changes in the strength of Southern Ocean deep-water ventilation (detailed
in Sect. 5.1) and (ii) the weakening of the global oceanic biological
pump (detailed in Sect. 5.2). Additionally, air–sea gas exchange
may have acted as a secondary factor contributing to our <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
decreases (detailed in Sect. 5.3).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>Stable carbon isotopic (<inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C) records from sediment
core GeoB6212-1. <bold>(a)</bold> <italic>Globigerinoides ruber</italic> white (<italic>G. ruber</italic> w) <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C and <bold>(b)</bold> <italic>Globorotalia inflata</italic> (<italic>G. inflata</italic>) <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C. Red and green lines represent three-point running
averages for <italic>G. ruber</italic> w and <italic>G. inflata</italic>, respectively. Black symbols at the bottom of the panel
depict calibrated ages. Grey vertical bars show abrupt
millennial-scale climate change events Heinrich Stadial 3 (HS3)
and Heinrich Stadial 2 (HS2) (Goni and Harrison, 2010; Sarnthein et al.,
2001).</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/13/345/2017/cp-13-345-2017-f04.png"/>

      </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F5" specific-use="star"><caption><p>Proxy records from the western South Atlantic, western and eastern
North Atlantic, and tropical South America, spanning Heinrich Stadial 3 (HS3)
and Heinrich Stadial 2 (HS2) (Goni and Harrison, 2010; Sarnthein et al.,
2001). <bold>(a)</bold> Changes in atmospheric circulation over Greenland derived from
Greenland Ice Sheet Project 2 (GISP2) Ca<inline-formula><mml:math id="M141" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> concentration (Mayewski et
al., 1997) plotted versus the Greenland Ice Core Chronology 2005 (GICC05)
(Andersen et al., 2006; Rasmussen et al., 2006) at 72.6<inline-formula><mml:math id="M142" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
38.5<inline-formula><mml:math id="M143" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W. <bold>(b)</bold> Heinrich layers indicated by the presence of
ice-rafted debris (IRD) from the Iberian Margin marine sediment core
MD99-2331 at 42.2<inline-formula><mml:math id="M144" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 9.7<inline-formula><mml:math id="M145" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W (Eynaud et al., 2009). <bold>(c)</bold>
Sea surface temperature (SST, <inline-formula><mml:math id="M146" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) changes from Iberian Margin
marine sediment cores SU8118 and MD952042 at 37.5<inline-formula><mml:math id="M147" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
10.1<inline-formula><mml:math id="M148" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W (Bard, 2000). <bold>(d)</bold> Atlantic meridional overturning
circulation (AMOC) strength derived from Bermuda Rise sedimentary
<inline-formula><mml:math id="M149" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">231</mml:mn></mml:msup></mml:math></inline-formula>Pa <inline-formula><mml:math id="M150" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M151" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">230</mml:mn></mml:msup></mml:math></inline-formula>Th ratio from ODP site 1063 (higher values indicate a
reduced AMOC) at 33.7<inline-formula><mml:math id="M152" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 57.6<inline-formula><mml:math id="M153" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W (Lippold et al.,
2009). <bold>(e)</bold> Position of the Intertropical Convergence Zone (ITCZ) indicated
by reflectance (*L) (higher values indicate decreased precipitation) from
the Cariaco Basin marine sediment core MD03-2621 at 10.7<inline-formula><mml:math id="M154" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
65<inline-formula><mml:math id="M155" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W (Deplazes et al., 2013) (orange line represents a 399-point
running average). <bold>(f)</bold> Strength of western Amazon precipitation indicated by
the <inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O from stalagmite NAR-C collected in the Cueva del
Diamante Cave, western Amazon (more negative values indicate increased
precipitation), at 5.4<inline-formula><mml:math id="M157" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 77.3<inline-formula><mml:math id="M158" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W (Cheng et al., 2013).
<bold>(g)</bold> Presence of palaeolakes indicated by the natural gamma radiation from
Bolivian Altiplano Salar de Uyuni (higher values indicate increased
precipitation) at 20.3<inline-formula><mml:math id="M159" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 67.5<inline-formula><mml:math id="M160" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W (Baker et al., 2001).
<bold>(h)</bold> <italic>Globigerinoides ruber</italic> white (<italic>G. ruber</italic> w) <inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C from marine sediment core GeoB6212-1
collected in the western South Atlantic at 32.4<inline-formula><mml:math id="M162" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S,
50.1<inline-formula><mml:math id="M163" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W (red line represents a three-point running
average, this study). <bold>(i)</bold> Sedimentation rates from marine sediment core
GeoB6212-1 collected in the western South Atlantic at 32.4<inline-formula><mml:math id="M164" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S,
50.1<inline-formula><mml:math id="M165" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W (this study). <bold>(j)</bold> Atmospheric CO<inline-formula><mml:math id="M166" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration (ppm)
from ice core Siple Dome (Ahn and Brook, 2014) plotted versus the Greenland
Ice Core Chronology 2005 (GICC05) (Svensson et al., 2008) at 81.7<inline-formula><mml:math id="M167" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 148.8<inline-formula><mml:math id="M168" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W.</p></caption>
        <?xmltex \igopts{width=170.716535pt}?><graphic xlink:href="https://cp.copernicus.org/articles/13/345/2017/cp-13-345-2017-f05.png"/>

      </fig>

<sec id="Ch1.S5.SS1">
  <title>Millennial-scale changes: AMOC-induced strengthening
of Southern Ocean deep-water ventilation</title>
      <p>A negative excursion during HS1 was described in planktonic foraminiferal
<inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C records from the Indo-Pacific Ocean (Spero and
Lea, 2002), Southern Ocean (Ninnemann and Charles, 1997), and South Atlantic
Ocean (Oppo and Fairbanks, 1989). Ninnemann and Charles (1997) suggested
that the source for this signal was the Southern Ocean.</p>
      <p>In the Southern Ocean, CDW forms from mixing of NADW, Indian Deep Water
(IDW),
and Pacific Deep Water (PDW) and upwells to the south of the Antarctic Polar
Front, driven by the prevailing westerly winds (Marshall and Speer, 2012).
Therefore, the <inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C signature of CDW (ca.
0.4 ‰) (Kroopnick, 1985) lies between that of NADW (ca.
1 ‰) (Kroopnick, 1985) and IDW–PDW (ca. 0.2 to
<inline-formula><mml:math id="M171" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.2 ‰) (Kroopnick, 1985; Oppo and Fairbanks, 1987;
Charles and Fairbanks, 1992). During periods of weak AMOC the inflow of NADW
to the Southern Ocean is reduced (Charles and Fairbanks, 1992), and the
<inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C of CDW should decrease since the latter would have a
relatively larger contribution from low-<inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C IDW and
PDW (Spero and Lea, 2002).</p>
      <p><?xmltex \hack{\newpage}?>Additionally, during periods of reduced AMOC the sub-tropical heat
transport towards the north would decrease, leading to rising temperatures
in the circum-Antarctic region (EPICA Community Members, 2006).
Consequently, models of low resolution suggest that the Southern Hemisphere
westerlies would become stronger and shift southward, strengthening CDW
upwelling (Toggweiler et al., 2006; Tschumi et al., 2011; Lee et al., 2011;
Voigt et al., 2015). Increased upwelling would supply the ocean surface
south of the Antarctic Polar Front with Si(OH)<inline-formula><mml:math id="M174" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>-rich,
low-<inline-formula><mml:math id="M175" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C waters (Anderson et al., 2009; Hendry et
al., 2012). Model experiments (Tschumi et al., 2011; Menviel et al., 2015;
Bauska et al., 2016) corroborate this hypothesis by showing that stronger
Southern Ocean upwelling would promote a weakening of the biological pump in
the Southern Ocean. Since upwelled CDW is hypothesized to be the dominant
source of the upper and intermediate waters that leave the Southern Ocean
(i.e. SAMW and AAIW) (Fig. 2), increased upwelling would transfer the low-<inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C signal as well as the positive Si(OH)<inline-formula><mml:math id="M177" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> anomaly to
those waters (Oppo and Fairbanks, 1989; Ninnemann and Charles, 1997; Spero
and Lea, 2002; Anderson et al., 2009; Hendry et al., 2012). Actually, a
low-density type of SAMW contributes to SACW that spreads into the
South Atlantic (Stramma and England, 1999). Additionally, AAIW also
influences SACW through vigorous eddy mixing at the Brazil–Malvinas
Confluence (Piola and Georgi, 1982). These signals would then propagate
through the thermocline SACW of the South Atlantic and be transferred to
the mixed-layer TW by a vertical exchange process (Tomczak and Godfrey, 2003).</p>
      <p>The reduced stratification of the Southern Ocean and intensification of the
upward transport of the remineralized carbon (<inline-formula><mml:math id="M178" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">12</mml:mn></mml:msup></mml:math></inline-formula>C-enriched
CO<inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> stored for a long period in deep waters (Anderson et al., 2009;
Denton et al., 2010; Jaccard et al., 2016; Mariotti et al., 2016) would
increase CO<inline-formula><mml:math id="M180" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (Siple Dome; 81.7<inline-formula><mml:math id="M181" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 148.8<inline-formula><mml:math id="M182" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W)
(Ahn and Brook, 2014) (Fig. 5j). Despite the low temporal resolution,
the Antarctic <inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M184" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> record of Eggleston et al. (2016) shows
a decrease during HS2. However, the CO<inline-formula><mml:math id="M185" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> peaks occur ca. 1 kyr later
than the initiation of the <inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C decrease in our records. Spero
and Lea (2002) also observed a similar offset between the increase in
CO<inline-formula><mml:math id="M187" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and the decrease in Pacific Ocean planktonic foraminifera
<inline-formula><mml:math id="M188" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C during HS1 and attributed this apparent offset to
uncertainties in the age models of their records.</p>
      <p>Therefore, the negative excursions in our <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C records could be
related to the transfer of a preformed <inline-formula><mml:math id="M190" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C signal from the
subantarctic zone to the western South Atlantic via central and thermocline
waters.</p>
</sec>
<sec id="Ch1.S5.SS2">
  <title>Millennial-scale changes: AMOC-induced weakening of
the biological pump</title>
      <p>Recent model experiments (e.g. Schmittner, 2005; Schmittner and Galbraith,
2008) have shown that AMOC slowdown events may cause a decrease in the
global efficiency of the oceanic biological pump, being an important driver
for the oceanic CO<inline-formula><mml:math id="M191" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> outgassing within HS1 during the last deglaciation
and possibly also during other HS, including HS3 and HS2.</p>
      <p>NADW has low preformed nutrient waters because it is formed by nutrient-depleted surface waters, where the biological pump has efficiently removed
nutrients from surface waters (Marinov et al., 2008). Antarctic Bottom Water (AABW) has high
preformed nutrient waters because it is formed by
nutrient-enriched Southern Ocean surface waters (nutrients have
not been efficiently removed from surface waters). However, during weak
AMOC two factors may alter the nutrient distribution and the global oceanic
biological pump (Schmittner and Galbraith, 2008). First, the reduction in
the NADW formation decreases the input of low-preformed-nutrient (high
<inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M193" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> waters to the ocean interior, which becomes more
dominated by high-preformed-nutrient (low <inline-formula><mml:math id="M194" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
southern component waters (e.g. AABW). Second, the reduction of the
Southern Ocean stratification induced by the decrease in salt input via NADW
formation promotes the strengthening of the upwelling and subsequent sinking
of high-preformed-nutrient (low <inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M197" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> waters to the
ocean interior, thus reducing the capacity of those unutilized nutrients to
sequester carbon via the biological pump. The two factors acting in
conjunction are thought to be responsible for the simulated weakening of the
global efficiency of the biological pump, as well as for the increase in
CO<inline-formula><mml:math id="M198" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and decrease in <inline-formula><mml:math id="M199" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M200" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (Schmittner and
Galbraith, 2008; Schmittner and Lund, 2015; Hertzberg et al., 2016).</p>
      <p>Schmittner and Lund (2015) show that the modelled weakening of the biological
pump, induced by an AMOC slowdown, reduces the ability of the surface ocean
to biologically sequester isotopically light organic carbon (<inline-formula><mml:math id="M201" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">12</mml:mn></mml:msup></mml:math></inline-formula>C),
producing a decrease in the surface ocean <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M203" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula> and an
increase in the intermediate ocean <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M205" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula> (lower
remineralization rate). For HS1, planktonic and benthic foraminiferal
<inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C records (Tessin and Lund, 2013; Lund et al., 2015; Curry
and Oppo, 2005; Hertzberg et al., 2016) from the western South Atlantic (ca.
27<inline-formula><mml:math id="M207" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S) agree with the model output by showing a decrease in
<inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C in the upper water column (SACW) and an increase at
intermediate water depths (AAIW). Thus, the weakening of the global oceanic
biological pump and consequent negative anomaly of the <inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M210" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula> in the upper water column should be captured by the tests
of planktonic foraminifera <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C during calcification (Spero and
Lea, 1996; Bemis et al., 2000). The negative <inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M213" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula>
during HS3 and HS2 revealed by our planktonic foraminifera provide the first
observational evidence supporting the modelling results. Additionally, this
mechanism also provides a possible explanation for the larger negative
<inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C anomaly in <italic>G. ruber</italic> w (mixed-layer dwelling) relative to the
anomaly in <italic>G. inflata</italic> (permanent thermocline dwelling) (Fig. 4).</p>
      <p>It is noteworthy that the mechanism described in Sect. 5.1, although based
on a different driver for the decrease in <inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C, also suggests
that the decreases in <inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C of planktonic foraminifera from the
South Atlantic would be carried by SACW (inherited from its precursor, SAMW)
and thus both mechanisms (described in Sect. 5.1 and here) are not mutually exclusive in this
regard. However, the mechanism described in the
present section goes against the assumption that weakening of the biological
pump is related to stronger upwelling in the Southern Ocean and that the
Southern Ocean would be the source of the low-<inline-formula><mml:math id="M217" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C signal for
the South Atlantic (Lund et al., 2015; Hertzberg et al., 2016).</p>
</sec>
<sec id="Ch1.S5.SS3">
  <title>Millennial-scale changes: the role of air–sea gas
exchange</title>
      <p>The <inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M219" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula> of the surface ocean can also be affected by
air–sea gas exchange (Oppo and Fairbanks, 1989; Charles and
Fairbanks, 1990; Lynch-Stieglitz et al., 1995). Although this process tends
towards isotopic equilibrium (especially in subtropical gyres because of the
longer water residence time in these regions), the CO<inline-formula><mml:math id="M220" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> exchange between
the ocean and the atmosphere does not lead to equilibrium because CO<inline-formula><mml:math id="M221" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
uptake and emission will still occur in different regions and the movement
and replacement of surface waters is faster than required for equilibration
(Lynch-Stieglitz et al., 1995). Since the <inline-formula><mml:math id="M222" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M223" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> is
lighter than <inline-formula><mml:math id="M224" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M225" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula>, at areas of ocean CO<inline-formula><mml:math id="M226" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> uptake
(i.e. water mass formation regions) air–sea gas exchange has the
potential to deplete <inline-formula><mml:math id="M227" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M228" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula> (Lynch-Stieglitz et al.,
1995). Additionally, the isotopic fractionation is inversely correlated with
temperature.</p>
      <p>Therefore, we cannot exclude the possibility that the likely decrease in
<inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M230" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> during AMOC slowdown events (Eggleston et
al.,
2016) (e.g. HS2) could have affected the <inline-formula><mml:math id="M231" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M232" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula> via
air–sea gas exchange, especially in regions of water mass formation. The
formation region of SACW is an area of ocean CO<inline-formula><mml:math id="M233" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> uptake and may
contribute to the <inline-formula><mml:math id="M234" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C anomalies observed in our <italic>G. inflata</italic> record (Fig. 4b). Additionally, since the isotopic fractionation during air–sea gas
exchange is temperature-dependent, the weakening of the AMOC and subsequent
warming of the upper subtropical South Atlantic (Barker et al., 2009; Chiessi
et al., 2015) could have contributed to the observed <inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
anomalies both in the <italic>G. ruber</italic> w and in the <italic>G. inflata</italic> records (Fig. 4). However, the gradient
is too small (<inline-formula><mml:math id="M236" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.1 ‰ <inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C per <inline-formula><mml:math id="M238" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C;
Broecker and Maier-Reimer, 1992) to explain all of the changes observed in
our records. If temperature were the dominant driver, unrealistic changes
between 5 and 13 <inline-formula><mml:math id="M239" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C would be required to explain the full
amplitudes of the <inline-formula><mml:math id="M240" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C variations.</p>
      <p>The <inline-formula><mml:math id="M241" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O records from <italic>G. ruber</italic> w and <italic>G. inflata</italic> from our core (Supplement
Fig. 1) should partially reflect changes in water temperature
(ca. <inline-formula><mml:math id="M242" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.22 ‰ per 1 <inline-formula><mml:math id="M243" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C; e.g. Mulitza et al.,
2003) but show no clear trends across HS3 and HS2. While temperature
changes might be partially obscured in the foraminiferal <inline-formula><mml:math id="M244" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O
records by the influence of synchronous changes in seawater <inline-formula><mml:math id="M245" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, as has been hypothesized for the Holocene (Chiessi et al., 2014)
and HS1 (Chiessi et al., 2015) in the western Atlantic, we consider it
unlikely that temperature changes of the magnitude above would be completely
masked.</p>
</sec>
<sec id="Ch1.S5.SS4">
  <title>Changes in continental climate</title>
      <p>Palaeoclimate records from South America indicate marked hydrological changes
during abrupt millennial-scale climate events (Arz et al., 1998;
Peterson et al., 2000; Baker et al., 2001; Cruz et al., 2006; Stríkis
et al., 2015). Reconstructed SAMS activity suggests strengthening during HS
(Cruz et al., 2006; Kanner et al., 2012; Cheng et al., 2013). Changes in
speleothem oxygen isotopic composition from the western Amazon Basin (NAR-C,
Cueva del Diamante Cave, northern Peru; 5.4<inline-formula><mml:math id="M246" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 77.3<inline-formula><mml:math id="M247" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W)
(Cheng et al., 2013) and changes on gamma radiation records from the
Bolivian Altiplano (Salar de Uyuni; 20.3<inline-formula><mml:math id="M248" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 67.5<inline-formula><mml:math id="M249" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W)
(Baker et al., 2001) (Fig. 5f, g) indicate increased precipitation during
HS3 and HS2. North of the Equator, a reflectance record from the Cariaco
Basin (off northern Venezuela, MD03-2621; 10.7<inline-formula><mml:math id="M250" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 65<inline-formula><mml:math id="M251" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W) (Deplazes et al., 2013) suggests decreased precipitation during the same
millennial-scale events (Fig. 5e). The opposite precipitation
variations at these sites reflect the inter-hemispheric anti-phased response
of tropical precipitation during HS (Wang et al., 2007; Cheng et al., 2013).
During HS3 and particularly HS2 the three above-mentioned records (Fig. 5e,
f, g) show a w structure similar to the one observed in our
<inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C records. Stríkis et al. (2015) reported a similar
w structure during HS1 related to two distinct hydrologic
phases within HS1.</p>
      <p>Periods of intensified SAMS would have strengthened the discharge from the
Plata River drainage basin (Chiessi et al., 2009), increasing the delivery
of terrigenous sediments to the Rio Grande Cone (Lantzsch et al., 2014), our
coring site. Our records present for the first time increased sedimentation
rates during a HS off SESA and corroborate the suggestion of Chiessi et al. (2009) during HS2. Furthermore, GeoB6212-1 sedimentation rates also show a
w structure during HS2 (Fig. 3), hinting at a sensitive
response of the Plata River drainage basin to the increase in activity of
the SAMS. The occurrence of a similar w structure in North
Atlantic records, in South American records, and in our <inline-formula><mml:math id="M253" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C and
sedimentation rate records gives us confidence that such
a w structure is indeed a ubiquitous feature of HS2, and
possibly also HS3 (in this case, only for <inline-formula><mml:math id="M254" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C). However, other
factors like shifts in bottom currents and sea level could also have
produced the observed changes in sedimentation rates. Detailed age models
and more cores from the Rio Grande Cone are necessary to elucidate the main
factors controlling the sedimentation rates in that region.</p>
      <p>The increased continental runoff that led to increased delivery of
terrigenous sediments to our core site could also have enhanced the nutrient
availability and the local primary productivity, affecting our planktonic
foraminiferal <inline-formula><mml:math id="M255" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C records. Some aspects of the regional
response to HS1 are useful for evaluating this possibility. During HS1, ice-volume-corrected seawater <inline-formula><mml:math id="M256" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O from the upper water
column of our core site indicates an increase in salinity (Chiessi et al.,
2015). Thus, despite the increased terrigenous discharge, it seems that
the upper water column of our core site was not affected by an increase in
freshwater discharge from the Plata River during HS1. Since the
precipitation anomaly of HS1 was stronger than that of HS3 and HS2 in the
Plata River drainage basin (Wang et al., 2007), it is unlikely that weaker
precipitation anomalies of HS3 and HS2 would have impacted the upper water
column of our core site more intensely than during HS1. This suggests that
changes in the discharge of the Plata River drainage basin at
millennial scale are not a relevant driver of our <inline-formula><mml:math id="M257" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
decreases and that the buoyant low-salinity waters were advected elsewhere
by winds, while terrigenous sediments were already too deep to be influenced
by the wind.</p>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <title>Conclusions</title>
      <p>Our mixed-layer and permanent thermocline <inline-formula><mml:math id="M258" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C records from the
western South Atlantic show in-phase millennial-scale decreases of
up to 1 ‰ during the HS3 and HS2. We hypothesize that the
low-<inline-formula><mml:math id="M259" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C signal may be related to two
millennial-scale mechanisms. (i) The first mechanism consists of changes in the Southern Ocean
deep-water ventilation. A weak AMOC during HS3 and HS2 would produce
stronger Southern Ocean upwelling, which in turn would supply the surface of
the Southern Ocean with more low-<inline-formula><mml:math id="M260" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C waters as well
as promote increased outgassing of this old and low-<inline-formula><mml:math id="M261" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C respired CO<inline-formula><mml:math id="M262" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. The low-<inline-formula><mml:math id="M263" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C waters at
the surface of the Southern Ocean would be subducted into the central and
thermocline waters and transferred equatorward via the South Atlantic
subtropical gyre circulation and southward along the western boundary
towards our core site. (ii) The second mechanism consists of weakening of the global oceanic biological pump.
A weak AMOC during HS3 and HS2 would promote an accumulation of
<inline-formula><mml:math id="M264" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula>C-depleted CO<inline-formula><mml:math id="M265" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the upper water column of the South
Atlantic. This accumulation would result in a negative anomaly of the
<inline-formula><mml:math id="M266" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M267" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">DIC</mml:mi></mml:msub></mml:math></inline-formula> (as well as of the <inline-formula><mml:math id="M268" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M269" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">atm</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
that in turn would be captured by the tests of planktonic foraminifera at
our core site. We further suggest that changes in air–sea gas
exchange could have contributed to the decreases in <inline-formula><mml:math id="M270" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C via
both mechanisms. Together with other lines of evidence, our data are
consistent with the hypothesis that the CO<inline-formula><mml:math id="M271" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> added to the atmosphere
during abrupt millennial-scale climate change events of the last
glacial period originated in the ocean and reached the atmosphere by
outgassing. Moreover, the occurrence of a similar w structure
during HS2 (and possibly HS3) in North Atlantic and South American records
as well as in our planktonic foraminiferal <inline-formula><mml:math id="M272" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C and
sedimentation rate records gives us confidence that such
a w structure is a pervasive feature that characterizes HS2 (and
possibly HS3).</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability">

      <p>The data reported here will be archived in Pangaea (<uri>https://doi.pangaea.de/10.1594/PANGAEA.874350</uri>, Campos et al., 2017).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p><bold>The Supplement related to this article is available online at <inline-supplementary-material xlink:href="http://dx.doi.org/10.5194/cp-13-345-2017-supplement" xlink:title="pdf">doi:10.5194/cp-13-345-2017-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
        </app-group><notes notes-type="competinginterests">

      <p>The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p>We thank Y. Zhang for help with the Bacon software. Logistic and technical
assistance was provided by the captain and crew of the R/V <italic>Meteor</italic>. We thank
the two anonymous reviewers and A. Schmittner for constructive comments that
greatly improved this paper. M. C. Campos acknowledges the financial
support from FAPESP (grants 2013/25518-2 and 2015/11016-0), and C. M. Chiessi acknowledges the financial support from FAPESP (grant 2012/17517-3)
and CAPES (grants 1976/2014 and 564/2015). H. Kuhnert, S. Mulitza, and I. Voigt were funded through the DFG Research Centre, Cluster of Excellence
“The Ocean in the Earth System”. A. R. Piola was funded by grant CRN3070
from the Inter-American Institute for Global Change Research through the US
National Science Foundation grant GEO-1128040. Sample material was provided
by the GeoB Core Repository at the MARUM – Center for Marine Environmental
Sciences, University of Bremen, Germany.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: Z. Guo<?xmltex \hack{\newline}?>
Reviewed by: two anonymous referees</p></ack><ref-list>
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    </app></app-group></back>
    <!--<article-title-html><i>δ</i><sup>13</sup>C decreases in the upper western South Atlantic during Heinrich Stadials 3 and 2</article-title-html>
<abstract-html><p class="p">Abrupt millennial-scale climate change events
of the last deglaciation (i.e. Heinrich Stadial 1 and the Younger Dryas)
were accompanied by marked increases in atmospheric CO<sub>2</sub> (CO<sub>2atm</sub>)
and decreases in its stable carbon isotopic ratios (<i>δ</i><sup>13</sup>C),
i.e. <i>δ</i><sup>13</sup>CO<sub>2atm</sub>, presumably due to outgassing from the
ocean. However, information on the preceding Heinrich Stadials during the
last glacial period is scarce. Here we present <i>δ</i><sup>13</sup>C records
from two species of planktonic foraminifera from the western South Atlantic
that reveal major decreases (up to 1 ‰) during Heinrich
Stadials 3 and 2. These <i>δ</i><sup>13</sup>C decreases are most likely related
to millennial-scale periods of weakening of the Atlantic
meridional overturning circulation and the consequent increase (decrease) in
CO<sub>2atm</sub> (<i>δ</i><sup>13</sup>CO<sub>2atm</sub>). We hypothesise two mechanisms
that could account for the decreases observed in our records, namely
strengthening of Southern Ocean deep-water ventilation and weakening of the
biological pump. Additionally, we suggest that air–sea gas
exchange could have contributed to the observed <i>δ</i><sup>13</sup>C decreases.
Together with other lines of evidence, our data are consistent with the
hypothesis that the CO<sub>2</sub> added to the atmosphere during abrupt
millennial-scale climate change events of the last glacial period
also originated in the ocean and reached the atmosphere by outgassing. The
temporal evolution of <i>δ</i><sup>13</sup>C during Heinrich Stadials 3 and 2 in
our records is characterized by two relative minima separated by a relative
maximum. This <q>w structure</q> is also found in North Atlantic and
South American records, further suggesting that such a structure is a
pervasive feature of Heinrich Stadial 2 and, possibly, also Heinrich Stadial 3.</p></abstract-html>
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