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  <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-13-317-2017</article-id><title-group><article-title>Freshening of the Labrador Sea as a trigger for <?xmltex \hack{\break}?> Little Ice Age development</article-title>
      </title-group><?xmltex \runningtitle{Freshening of the Labrador Sea as a trigger for Little Ice Age development}?><?xmltex \runningauthor{M.~Alonso-Garcia et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2 aff3">
          <name><surname>Alonso-Garcia</surname><given-names>Montserrat</given-names></name>
          <email>montserrat.alonso@ipma.pt</email>
        <ext-link>https://orcid.org/0000-0002-0241-2178</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Kleiven</surname><given-names>Helga (Kikki) F.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4956-6182</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>McManus</surname><given-names>Jerry F.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Moffa-Sanchez</surname><given-names>Paola</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Broecker</surname><given-names>Wallace S.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff7">
          <name><surname>Flower</surname><given-names>Benjamin P.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>College of Marine Science, University of South Florida, St. Petersburg, FL, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Instituto Português do Mar e da Atmosfera (IPMA), Div. de Geologia e Georecursos Marinhos, Lisbon, Portugal</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Centro de Ciencias do Mar (CCMAR), Universidade do Algarve, Faro, Portugal</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>University of Bergen and Bjerknes Centre for Climate Research, Postboks 7803, 5020 Bergen, Norway</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Earth and Environmental Sciences, Lamont-Doherty Earth Observatory of Columbia University, <?xmltex \hack{\break}?> Palisades, NY 10964-8000, USA</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>School of Earth and Ocean Sciences, Cardiff University, Park Place, CF10 3YE, Cardiff, UK</institution>
        </aff>
        <aff id="aff7"><label>†</label><institution>deceased</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Montserrat Alonso-Garcia (montserrat.alonso@ipma.pt)</corresp></author-notes><pub-date><day>7</day><month>April</month><year>2017</year></pub-date>
      
      <volume>13</volume>
      <issue>4</issue>
      <fpage>317</fpage><lpage>331</lpage>
      <history>
        <date date-type="received"><day>10</day><month>July</month><year>2016</year></date>
           <date date-type="rev-request"><day>2</day><month>August</month><year>2016</year></date>
           <date date-type="rev-recd"><day>20</day><month>January</month><year>2017</year></date>
           <date date-type="accepted"><day>3</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/13/317/2017/cp-13-317-2017.html">This article is available from https://cp.copernicus.org/articles/13/317/2017/cp-13-317-2017.html</self-uri>
<self-uri xlink:href="https://cp.copernicus.org/articles/13/317/2017/cp-13-317-2017.pdf">The full text article is available as a PDF file from https://cp.copernicus.org/articles/13/317/2017/cp-13-317-2017.pdf</self-uri>


      <abstract>
    <p>Arctic freshwater discharges to the Labrador Sea from melting glaciers and
sea ice can have a large impact on ocean circulation dynamics in the North
Atlantic, modifying climate and deep water formation in this region. In this
study, we present for the first time a high resolution record of ice rafting
in the Labrador Sea over the last millennium to assess the effects of
freshwater discharges in this region on ocean circulation and climate. The
occurrence of ice-rafted debris (IRD) in the Labrador Sea was studied using
sediments from Site GS06-144-03 (57.29<inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 48.37<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W;
3432 m water depth). IRD from the fraction 63–150 <inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> shows
particularly high concentrations during the intervals
<inline-formula><mml:math id="M4" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1000–1100, <inline-formula><mml:math id="M5" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1150–1250, <inline-formula><mml:math id="M6" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1400–1450,
<inline-formula><mml:math id="M7" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1650–1700 and <inline-formula><mml:math id="M8" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1750–1800. The first two
intervals occurred during the Medieval Climate Anomaly (MCA), whereas the
others took place within the Little Ice Age (LIA). Mineralogical
identification indicates that the main IRD source during the MCA was SE
Greenland. In contrast, the concentration and relative abundance of
hematite-stained grains reflects an increase in the contribution of Arctic
ice during the LIA.</p>
    <p>The comparison of our Labrador Sea IRD records with other climate proxies
from the subpolar North Atlantic allowed us to propose a sequence of
processes that led to the cooling that occurred during the LIA, particularly
in the Northern Hemisphere. This study reveals that the warm climate of the
MCA may have enhanced iceberg calving along the SE Greenland coast and, as a
result, freshened the subpolar gyre (SPG). Consequently, SPG circulation
switched to a weaker mode and reduced convection in the Labrador Sea,
decreasing its contribution to the North Atlantic deep water formation and,
thus, reducing the amount of heat transported to high latitudes. This
situation of weak SPG circulation may have made the North Atlantic climate
more unstable, inducing a state in which external forcings (e.g. reduced
solar irradiance and volcanic eruptions) could easily drive periods of
severe cold conditions in Europe and the North Atlantic like the LIA. This
analysis indicates that a freshening of the SPG may play a crucial role in
the development of cold events during the Holocene, which may be of key
importance for predictions about future climate.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>The last millennium is an important target in palaeoclimate studies since
this interval allows us to reconstruct the climate variability of our recent
history and its impact on the development of our society. Moreover, climate
reconstructions of the last millennium combined with instrumental records
constitute a framework to obtain a comprehensive understanding of the
mechanisms that drive the Earth's climate and improve future climate
predictions. The climate of the last millennium is characterized by a warm
period called the Medieval Climate Anomaly (MCA) or Medieval Warm Period
(<inline-formula><mml:math id="M9" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 800–1200), a cold interval called the Little Ice Age
(LIA, <inline-formula><mml:math id="M10" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1350–1850) and the 20th century warming
trend (e.g. Mann et al., 2009; Wanner et al., 2011). According to
historical records, these climate oscillations affected human development in
Europe, in particular the Norse expansion and demise in the North Atlantic
(Ogilvie et al., 2000). The warm conditions of the
MCA promoted the colonization of Iceland and Greenland by the Norse and the
exploration of North America during the 9th to 12th centuries, whereas their
maladaptation to climate deterioration at the beginning of the LIA led them
to abandon the Greenland settlements by the end of the 15th century
(Dugmore et al., 2012; Kuijpers et al., 2014; Ogilvie et al., 2000).</p>
      <p>Reconstructions of ocean and land temperature show the LIA cooling was
neither spatially nor temporally uniform (Bradley et al., 2003; PAGES 2k
Consortium, 2013; Wanner et al., 2011, 2015), and therefore
there is an open debate on the forcings that may have triggered these
climate oscillations. Reduced solar irradiance and the occurrence of
explosive volcanic eruptions are the two most commonly examined forcings
(e.g. Bond et al., 2001; Miller et al., 2012) due to the impact they may
have on atmospheric dynamics. Other forcings such as the internal dynamics
of the oceanic and atmospheric systems (such as the North Atlantic
Oscillation, NAO; Arctic Oscillation, AO; Atlantic Multidecadal
Oscillation, AMO; El Niño–Southern Oscillation, ENSO; or the monsoonal
regimes) have also been considered to play a major role driving climate
oscillations during the last century (see review in Wanner et
al., 2011). Freshwater discharge to the North Atlantic may also be a driver of
climate change by impacting sea surface circulation and deep water
convection, which in turn may slow down the Atlantic Meridional Overturning
Circulation (AMOC) (Manabe and Stouffer, 1995). The Labrador Sea is
particularly sensitive to increases in freshwater and sea ice input. Deep
water formation in the Labrador Sea contributes 30 % of the volume
transport of the deep limb of the AMOC (Rhein et al., 2002;
Talley, 2003), and freshwater input to this region can potentially reduce
oceanic deep convection, slowing down the Atlantic circulation and its
related oceanic heat transport (Born et al., 2010; Moreno-Chamarro et
al., 2015). The decrease in heat export from low to high latitudes modifies
regional climate by cooling the western North Atlantic, which, in turn,
influences the climate of the whole North Atlantic (Born et al.,
2010). A recent example of this phenomenon may be the “Great Salinity
Anomaly” event that occurred between 1968 and 1982 (Dickson
et al., 1988). During this interval, vast amounts of Arctic sea ice and
freshwater were delivered to the Labrador Sea, mainly via the East Greenland
Current (EGC), freshening the subpolar gyre (SPG) and decreasing winter
convection and deep water production. A recent study of the last 50 years
also shows a close relationship between freshwater fluxes from the Arctic
and reductions in deep water formation in the Labrador Sea
(Yang et al., 2016).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p><bold>(a)</bold> Location of multicore GS06-144-03 (red star) and other sites in
the northern North Atlantic whose records have been used to support the
discussion proposed in this work. General North Atlantic circulation is
shown according to Schmitz and McCartney (1993). The location of Norse
settlements in Greenland is shaded and indicated with ES (eastern
settlement) and WS (western settlement). <bold>(b)</bold> Temperature and salinity
profiles of the first 1000 m at site GS06-144-03 obtained through Ocean Data
View (<uri>https://odv.awi.de/</uri>) from the World Ocean Atlas 2013 (Locarnini
et al., 2013; Zweng et al., 2013).</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://cp.copernicus.org/articles/13/317/2017/cp-13-317-2017-f01.jpg"/>

      </fig>

      <p>Recently, attention has been given to the dynamics of the SPG and its
relationship with climate (e.g. Born and Stocker, 2014).
Instrumental records and modern observations show a close link between
decadal climate variability and SPG dynamics (e.g. Hakkinen
and Rhines, 2004; Sarafanov, 2009), and rapid climate change reconstructions
of the Holocene and the last interglacial period have been interpreted as a
consequence of changes in the SPG dynamics (Moffa-Sanchez et al., 2014a;
Mokeddem and McManus, 2016; Mokeddem et al., 2014; Moros et al., 2012;
Thornalley et al., 2009). Variations in the strength and shape of the SPG
also impact deep convection in the Labrador Sea, therefore influencing deep
water production and Atlantic circulation (Böning et al., 2006; Hatun
et al., 2005; Moreno-Chamarro et al., 2015), which eventually affects
climate through the reduction of heat transported from low to high
latitudes. A shift to weak SPG circulation has been inferred using deep-sea
corals after AD 1250 (Copard et al., 2012), and
model simulations suggested this weakening of the SPG was the main driver of
the LIA due to the decrease in meridional heat transport to the subpolar
North Atlantic (Moreno-Chamarro et al., 2017). Moreover, the
occurrence of unusually cold winters in Europe during the last 100 years has
been associated with atmospheric blocking events in the North Atlantic,
which are high-pressure systems that alter the normal westerly wind
circulation in this region (Häkkinen et al., 2011). These events are
associated with negative AO, may modify surface circulation in the North
Atlantic, and are linked to cold winter temperature in western Europe
(Shabbar et al., 2001). Periods of intense and persistent atmospheric
blocking events very likely developed during the LIA due to the influence of
low solar irradiance and weak SPG circulation, causing decadal intervals of
severe cooling in Europe (Moffa-Sanchez et al., 2014a).</p>
      <p>In this work we used a sediment core from the Eirik Drift, in the Labrador
Sea, to reconstruct ice-rafting occurrence during the last 1200 years and
examine its impact on SPG dynamics and climate. The presence of ice-rafted
debris (IRD) is a proxy for iceberg and sea ice discharges. Our IRD record
from the Eirik Drift indicates ice export to the Labrador Sea and allows us
to infer periods of enhanced freshwater discharges. Previous Holocene
multi-proxy records (including IRD records) from the North Atlantic pointed
to the linkage between cooling events and low solar irradiance values
(Bond et al., 2001). However, this hypothesis has been challenged
by the observation that ice-rafting reconstructions in the northern North
Atlantic show different trends between the eastern and western regions
during the Holocene (Moros et al., 2006). The combination of our
IRD data with other records from Eirik Drift as well as other subpolar North
Atlantic sites allows us to present a comprehensive reconstruction of the
transition from the MCA to the LIA. This study reveals the importance of ice
discharges in modifying surface circulation in the SPG, as a driver of
oscillations in climatic patterns and deep water production in the past, and
perhaps again in the future.</p>
</sec>
<sec id="Ch1.S2">
  <title>Geological and oceanographic setting</title>
      <p>Site GS06-144-03 (57.29<inline-formula><mml:math id="M11" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 48.37<inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W; 3432 m water
depth) is located in the southern tip of Greenland at the Eirik drift (Fig. 1).
The site is placed in the northwest part of the SPG, a very sensitive
area to climatic and oceanographic changes given that the upper North
Atlantic deep water forms in this region (Schmitz and
McCartney, 1993). The SPG boundary currents are formed by the North Atlantic
Current (NAC); the Irminger Current, which is the western branch of the NAC
and flows towards Greenland; the East Greenland Current (EGC); and the
Labrador Current (Fig. 1). The Irminger Current brings warm and high-salinity
water to the Labrador Sea, whereas the EGC and Labrador Current transport
colder and lower salinity water and frequently carry icebergs and sea ice
from the Arctic area.</p>
      <p>Oscillations in the amount of ice transported by the EGC and Labrador
Current may result in freshening of the SPG affecting the strength of SPG
circulation. Fluctuations in the SPG circulation have been suggested as the
driver of oscillations in decadal deep water production and climate
variability in the North Atlantic and surrounding continents (Böning
et al., 2006; Hakkinen and Rhines, 2004; Hatun et al., 2005). Two states of
equilibrium have been described depending on the strength of the SPG
circulation: (1) when the circulation is strong, more salty water is
advected to the centre of the gyre, favouring deep water formation in this
area, whereas (2) when the circulation is weak more salty water is advected
northeastward to the Nordic Seas and the SPG water gets fresher, which
prevents deep convection in the Labrador Sea (Born and Stocker,
2014). However, some increased convection may occur in the Irminger Basin
and Nordic Seas, counterbalancing the lack of Labrador Sea convection.
Changes in the dynamics of the SPG are mainly driven by cyclonic winds and
buoyancy forcing (Born and Stocker, 2014); therefore,
freshwater input via iceberg discharges may be a critical factor modifying
the circulation in the SPG and deep water formation in the Labrador Sea.</p>
</sec>
<sec id="Ch1.S3">
  <title>Materials and methods</title>
      <p>Sediments from core GS06-144-03 MC-A were drilled using a multicore device
during a cruise on the R/V <italic>G.O. Sars</italic> (Dokken and Ninnemann, 2006). A
robust chronology has been developed based on 12 accelerator mass
spectrometry (AMS) <inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C dates performed on the calcareous shells of the
planktonic foraminifer <italic>Neogloboquadrina pachyderma</italic> sinistral and <inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb measurements at the top of
the core. The dates were analysed on the accelerator mass spectrometer at
the Leibniz Labor für Altersbestimmung und Isotopenforschung in Kiel,
Germany. Radiocarbon ages have been converted into calendar years using the
CALIB (rev 5.0.1) software (Stuiver and Reimer, 1993) in conjunction
with the Marine04 calibration dataset (Hughen et al., 2004). All dates
were calibrated with a constant surface reservoir age of 400 years. The
sample at 0 cm showed erroneous age because of severe addition of more than
100 % modern carbon (pMC) and is assumed to be post-AD 1962 (relative to
the increase in bomb radiocarbon levels in the North Atlantic region). The
core was collected in 2006 and the cesium spike and <inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb measurements
in the upper 12 cm of the core sediments confirms post-AD 1964 age. Table 1
shows the uncorrected <inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C ages and calibrated ages.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>Site GS06-144-03 MC-A chronology, based on 12 accelerator mass
spectrometry (AMS) <inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C dates performed on the calcareous shells of the
planktonic foraminifera <italic>Neogloboquadrina pachyderma</italic> sinistral.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="7">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="41pt"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="35pt"/>
     <oasis:colspec colnum="4" colname="col4" align="justify" colwidth="55pt"/>
     <oasis:colspec colnum="5" colname="col5" align="justify" colwidth="45pt"/>
     <oasis:colspec colnum="6" colname="col6" align="left"/>
     <oasis:colspec colnum="7" colname="col7" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Lab code<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col2">Core depth <?xmltex \hack{\hfill\break}?>(cm)</oasis:entry>  
         <oasis:entry colname="col3">Species<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col4">Uncorrected <inline-formula><mml:math id="M25" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C age <?xmltex \hack{\hfill\break}?>(years) <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> <?xmltex \hack{\hfill\break}?>error</oasis:entry>  
         <oasis:entry colname="col5">Calibrated age (AD)<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula> <?xmltex \hack{\hfill\break}?>(median probability)</oasis:entry>  
         <oasis:entry colname="col6">1<inline-formula><mml:math id="M28" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> age range</oasis:entry>  
         <oasis:entry colname="col7">Remarks</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">KIA34239</oasis:entry>  
         <oasis:entry colname="col2">0</oasis:entry>  
         <oasis:entry colname="col3">Nps</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:mn mathvariant="normal">145</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> BP<inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5">1984</oasis:entry>  
         <oasis:entry colname="col6">2006–1962</oasis:entry>  
         <oasis:entry colname="col7">Bomb <inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">KIA41679</oasis:entry>  
         <oasis:entry colname="col2">2</oasis:entry>  
         <oasis:entry colname="col3">Nps</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mn mathvariant="normal">555</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> BP</oasis:entry>  
         <oasis:entry colname="col5">1739</oasis:entry>  
         <oasis:entry colname="col6">1701–1776</oasis:entry>  
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">KIA43514</oasis:entry>  
         <oasis:entry colname="col2">4.5</oasis:entry>  
         <oasis:entry colname="col3">Nps</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mn mathvariant="normal">640</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> BP</oasis:entry>  
         <oasis:entry colname="col5">1669</oasis:entry>  
         <oasis:entry colname="col6">1647–1690</oasis:entry>  
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">KIA43515</oasis:entry>  
         <oasis:entry colname="col2">5.5</oasis:entry>  
         <oasis:entry colname="col3">Nps</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mn mathvariant="normal">740</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> BP</oasis:entry>  
         <oasis:entry colname="col5">1563</oasis:entry>  
         <oasis:entry colname="col6">1526–1600</oasis:entry>  
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">KIA41681</oasis:entry>  
         <oasis:entry colname="col2">8</oasis:entry>  
         <oasis:entry colname="col3">Nps</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:mn mathvariant="normal">760</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> BP</oasis:entry>  
         <oasis:entry colname="col5">1540</oasis:entry>  
         <oasis:entry colname="col6">1497–1582</oasis:entry>  
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">KIA36383</oasis:entry>  
         <oasis:entry colname="col2">10</oasis:entry>  
         <oasis:entry colname="col3">Nps</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mn mathvariant="normal">815</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> BP</oasis:entry>  
         <oasis:entry colname="col5">1490</oasis:entry>  
         <oasis:entry colname="col6">1466–1514</oasis:entry>  
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">KIA36384</oasis:entry>  
         <oasis:entry colname="col2">12</oasis:entry>  
         <oasis:entry colname="col3">Nps</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mn mathvariant="normal">890</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> BP</oasis:entry>  
         <oasis:entry colname="col5">1447</oasis:entry>  
         <oasis:entry colname="col6">1428–1465</oasis:entry>  
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">KIA36385</oasis:entry>  
         <oasis:entry colname="col2">18</oasis:entry>  
         <oasis:entry colname="col3">Nps</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mn mathvariant="normal">1140</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> BP</oasis:entry>  
         <oasis:entry colname="col5">1266</oasis:entry>  
         <oasis:entry colname="col6">1241–1291</oasis:entry>  
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">KIA36386</oasis:entry>  
         <oasis:entry colname="col2">22</oasis:entry>  
         <oasis:entry colname="col3">Nps</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mn mathvariant="normal">1225</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">35</mml:mn></mml:mrow></mml:math></inline-formula> BP</oasis:entry>  
         <oasis:entry colname="col5">1192</oasis:entry>  
         <oasis:entry colname="col6">1145–1238</oasis:entry>  
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">KIA36387</oasis:entry>  
         <oasis:entry colname="col2">28</oasis:entry>  
         <oasis:entry colname="col3">Nps</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mn mathvariant="normal">1460</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> BP</oasis:entry>  
         <oasis:entry colname="col5">948</oasis:entry>  
         <oasis:entry colname="col6">910–986</oasis:entry>  
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">KIA41682</oasis:entry>  
         <oasis:entry colname="col2">32</oasis:entry>  
         <oasis:entry colname="col3">Nps</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mn mathvariant="normal">1440</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> BP</oasis:entry>  
         <oasis:entry colname="col5">968</oasis:entry>  
         <oasis:entry colname="col6">926–1009</oasis:entry>  
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">KIA34241</oasis:entry>  
         <oasis:entry colname="col2">36</oasis:entry>  
         <oasis:entry colname="col3">Nps</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mn mathvariant="normal">1600</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> BP</oasis:entry>  
         <oasis:entry colname="col5">777</oasis:entry>  
         <oasis:entry colname="col6">734–819</oasis:entry>  
         <oasis:entry colname="col7"/>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p><inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula> KIA – Leibniz Labor für Altersbestimmung und
Isotopenforschung, Kiel, Germany.<?xmltex \hack{\\}?><inline-formula><mml:math id="M19" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula> Nps – <italic>Neogloboquadrina pachyderma</italic> sinistral.<?xmltex \hack{\\}?><inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C ages were converted into calendar ages with the CALIB Rev
6.1.0 software and the MARINE09 calibration dataset, applying a standard
400a reservoir age correction.<?xmltex \hack{\\}?><inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula> Sample marked with an asterisk had levels of more than 100 % modern
carbon (pMC) and is assumed to be post-AD 1962 (relative to the increase in
bomb radiocarbon levels in the North Atlantic region). Core was collected in
2006.</p></table-wrap-foot></table-wrap>

      <p>Sediment samples were taken continuously every 0.5 cm (0–41.5 cm), and the
high sedimentation rate at this site allows us to reconstruct the
ice-rafting history of the past 1200 years at a decadal-scale resolution (mean
sedimentation rate of 0.029 cm yr<inline-formula><mml:math id="M43" 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>, on average <inline-formula><mml:math id="M44" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 17 years between
samples). Samples were soaked in distilled water and shaken for 12 h in
order to disperse the sediment. Then they were wet-sieved and separated into
size fractions of &gt; 150, 63–150 and &lt; 63 <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>
and subsequently dried in an oven.</p>
      <p>In order to study the IRD content we use the 63–150 <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> fraction. This
size fraction is coarse enough to be delivered to the open ocean primarily
by drifting ice rather than wind or currents (Fillon et al.,
1981; Ruddiman, 1977), yet lends itself to detailed petrographic analysis
(Bond and Lotti, 1995). Bond's technique (Bond et al.,
1997) was robustly tested using several multicores in the polar–subpolar
region and it was compared to counts in the &gt; 150 <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>
fraction. We acknowledge that grains &gt; 250 <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> are the best
fraction to claim transport by icebergs and sea ice because wind and deep
currents can be confidently ruled out (Andrews, 2000).
Unfortunately, the samples of our study interval do not contain enough
grains in this fraction to develop a sound analysis to show trends in
coarser IRD. We will need larger amounts of bulk sediment to perform
significant counts of IRD &gt; 250 <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>. Even though it has
been suggested that within the 63–150 <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> fraction some grains might
be transported by other means (see discussion in
Andrews et al., 2014), given the location of the study site (in the outer
part of Eirik Drift) we think meltwater plumes are very unlikely and deep
currents hardly transport sediments &gt; 63 <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>. Therefore, we
can assume the 63–150 <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> fraction we studied is mainly composed of
IRD grains.</p>
      <p>Each sample was split with a microsplitter to obtain an aliquot with about
200 IRD grains. The aliquots were placed in a transparent gridded tray and
counted using a high-magnification stereomicroscope which incorporates a
light source from the bottom, similar to the transmitted light, and a light
source from the top which emulates reflected light. Using aliquots in a
transparent tray instead of smear slides offers the possibility of moving
the grains independently, thus allowing for a better identification.
Additionally, the use of a transparent tray is a key factor to improve the
identification of quartz and feldspar hematite-stained grains (HSGs) by the
introduction of a white paper below the tray which enhances the contrast
between the hematite-stained portion and the rest of the grain. This
technique is similar to that described in Bond et al. (1997);
however, the use of aliquots presents the advantage that IRD concentrations
in the bulk sediment can be calculated to obtain the total number of IRD
(and IRD types) per gram of bulk sediment. A minimum of 200 grains were
counted in each sample and the calculated errors for the replicated samples
are below 3.2 %. The identification of different groups of minerals such
as HSGs of quartz and feldspar, unstained quartz and feldspar, and brown and
white volcanic glass (VG) allows us to calculate the relative abundance of
each type of IRD, which may be useful to identify the sources of the
drifting ice that transported the IRD (e.g. Alonso-Garcia et al., 2013;
Bailey et al., 2012). SEM X-ray diffraction was performed on selected grains
with an energy dispersive spectroscopy (EDS) equipment at the facilities of
the College of Marine Science (University of South Florida). The EDS
equipment used is an EDAX X-ray microanalysis system with an Apollo 10
silicon drift detector.</p>
      <p>Stable isotope analyses (<inline-formula><mml:math id="M53" 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) were performed on planktonic
foraminifer shells of <italic>N. pachyderma</italic> sin to reconstruct near-surface water properties.
Samples for isotopes were also taken every 0.5 cm. <italic>N. pachyderma</italic> sin was picked from the
150–250 <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> size fraction. Before performing the analyses, the
foraminiferal shells were ultrasonically rinsed for 20 s in methanol
to remove fine-grained particles. Stable isotope ratios were obtained at the
stable isotope laboratory at Department of Earth Sciences and the Bjerknes
Centre for Climate Research at the University of Bergen, using Nier-type
(gas source) mass spectrometers. The <inline-formula><mml:math id="M55" 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 analyses of samples
from 0–15.5 cm in the core were carried out on a Finnigan MAT251 mass
spectrometer, while the rest of the samples (15.5–41.5 cm) were analysed on
a MAT253 mass spectrometer. All planktonic samples were run in four
replicates. The stable isotope results are expressed as the average of the
replicates and reported relative to Vienna Pee Dee Belemnite (VPDB),
calibrated using NBS-19. Long-term analytical precision (1<inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> of the
standards over a time interval of several months is 0.1 ‰
for the MAT253 system and &lt; 0.08 ‰ for the MAT251
system.</p>
</sec>
<sec id="Ch1.S4">
  <title>Results</title>
      <p>The total concentration of IRD (Fig. 2d) ranges from <inline-formula><mml:math id="M57" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 9000
to 116 000 grains per gram of sediment (grains g<inline-formula><mml:math id="M58" 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>), which means that icebergs
and sea ice reached the studied area during the entire interval examined in
this work. The highest peak of IRD concentration was reached at the end of
the MCA (AD 1169) and the intervals with highest IRD concentration
occurred approximately at AD 1000–1100, 1150–1250, 1400–1450, 1650–1700 and
1750–1800, with mean values above 50 000 grains g<inline-formula><mml:math id="M59" 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>. The first two of
these five intervals of high ice rafting occurred during the MCA, whereas
the other three intervals of high IRD concentration took place during the
LIA.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p>Ice-rafted debris (IRD) records from site GS06-144-03. <bold>(a)</bold> Coal
grains relative abundance; <bold>(b)</bold> hematite-stained grains (HSGs) relative
abundance; <bold>(c)</bold> total volcanic glass (VG) relative abundance (brown line) and
white VG relative abundance (shaded area); <bold>(d)</bold> total IRD concentration in
each sediment sample (black line), and IRD concentration not including the
white volcanic glass (shaded area); <bold>(e)</bold> concentration of HSGs;
<bold>(f)</bold> concentration of total VG (brown line) and white VG (shaded
area); and
<bold>(g)</bold> Northern Hemisphere sulphate aerosol injection by volcanic eruptions (after
Gao et al., 2008, revised in 2012) and non-sea-salt sulfur from the NEEM
Greenland ice core (Sigl et al., 2015). Blue horizontal lines indicate mean
values for the intervals they encompass. The approximate standard duration
of the Little Ice Age (LIA) and Medieval Warm Period (MWP) has been depicted
in blue and red squares respectively.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/13/317/2017/cp-13-317-2017-f02.jpg"/>

      </fig>

      <p>Volcanic glass (VG) is one of the main components of IRD, with relative
abundances up to 59 % (Fig. 2c). This group includes brown VG fragments,
usually not vesicular, and white VG fragments, which are very light and often with
vesicular aspect. The concentration of the total VG shows a similar pattern
to the total IRD concentration with the highest values during the same
intervals (Fig. 2). The relative abundance of VG shows high values during
the intervals of high total IRD concentration. The relative abundance of
white VG is generally lower than 20 % and does not show clear periods of
high abundance that can be correlated with the records of volcanic eruptions
(Gao et al., 2008; Sigl et al., 2015).</p>
      <p>HSG relative abundance ranges between 2 and 30 %, reaching higher values
than those observed at MC52 in the eastern North Atlantic (Fig. 3b,
Bond et al., 2001). The record of HSG concentration shows a different
pattern from the total IRD and VG records, with higher concentration from
AD 1400 to 1900 (Fig. 2e). The relative abundance of HSGs is also higher
after AD 1400, with mean values increasing to over 15 % from near 5 %
before AD 1400. This range of variability is comparable to previous
observations across the Atlantic in the late Holocene (Bond et al., 1997;
2001).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>LIA shift at <inline-formula><mml:math id="M60" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1400 (green vertical bar) in
several records compared to site GS06-144-03 IRD records. <bold>(a)</bold> SE Greenland
April sea ice concentration (Miettinen et al., 2015); <bold>(b)</bold> SE Greenland April
sea surface temperature (Miettinen et al., 2015); <bold>(c)</bold> Na<inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> record from
GISP2 (Meeker and Mayewski, 2002); <bold>(d)</bold> HSG record from Eirik Drift (red line)
and from Feni Drift in the NE Atlantic (black dashed line; Bond et al.,
2001); <bold>(e)</bold> total IRD concentration; and <bold>(f)</bold> HSG concentration. The main events in
Norse colonization and abandonment of settlements are depicted at the top of
the figure, according to Ogilvie et al. (2000).</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/13/317/2017/cp-13-317-2017-f03.jpg"/>

      </fig>

      <p>Among the selected grains to perform X-ray analysis we separated a group of
black unclassified minerals. According to the SEM X-ray diffraction
analysis, those grains are mainly composed of carbon, and we interpreted
them as coal fragments. Those minerals occurred in higher abundance during
the MCA and the end of the LIA.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S5">
  <title>Discussion</title>
<sec id="Ch1.S5.SS1">
  <title>IRD sources and significance</title>
      <p>The mineralogy found at Site GS06-144-03 suggests several lithological
sources for the IRD which may be associated with icebergs or sea ice
originated from different areas. Volcanic rocks mainly outcrop surrounding
Denmark Strait, in Iceland and the Geikie Plateau area on the East Greenland
coast (Bailey et al., 2012; Henriksen et al., 2009). Volcanic glass can
also be atmospherically transported after volcanic eruptions and be
ultimately incorporated in the ice as it has been shown in Greenland ice
core records (Grönvold et al., 1995). This is very
likely the case of the white VG fragments found in our record because our
counts of white VG (Fig. 2) do not suggest the presence of any discrete
layer that could be associated with any dated Icelandic eruption (Gao et
al., 2008; Sigl et al., 2015). This type of IRD was probably deposited on
the top of glaciers and sea ice near Iceland and the East Greenland coast
and then transported in the ice through the EGC. Although some of those
volcanic shards ejected to the atmosphere could have fallen directly in the
sea, the preferentially eastward dispersal pattern of Icelandic tephra
follows the predominantly westerly winds in the stratosphere
(Lacasse, 2001) and, hence, the amount of volcanic glass
transported by winds to the study site must be rather small. Previous
studies suggested the significantly low amounts of tephra transported
towards Greenland prevent finding layers that can be associated with
volcanic eruptions (Jennings et al., 2014). After detailed geochemical
studies Jennings et al. (2014) could not recognize any specific layer that
could be used as a tephrochronological event in the SE Greenland coast
during the last millennium. Brown VG fragments are generally solid and not
vesicular, suggesting that they are not windblown shards and were more
likely to have been incorporated in the ice from outcrops in Greenland and
Iceland. Similar brown VG fragments were described in Kangerdlugssuaq trough
sediments and were interpreted as coming from the glaciers and sea ice from
the Geikie Plateau area, based on mineralogical and X-ray diffraction
analysis data  (Alonso-Garcia et al., 2013).</p>
      <p>The presence of HSGs in Eirik Drift sediments indicates drift ice (sea ice
and icebergs) coming from NE Greenland and the Arctic, where red sandstones
outcrop (Bond et al., 1997; Henriksen et al., 2009). Most of the glaciers
in NE Greenland and the Arctic develop floating ice tongues in the fjords
where semi-permanent fast ice hinders the icebergs from drifting. As a
result, most of the IRD carried at the base of the icebergs is deposited in
the fjords (Reeh et al., 2001). Our HSG record from the Eirik Drift
shows a significant amount (up to 30 %) of this type of IRD. Therefore,
despite substantial deposition of debris within the fjords, the remainder of
the drifted ice still carries considerable amounts of IRD. We suggest that
some of that IRD may have been wind-blown to the top of the glaciers and/or
sea ice at the NE Greenland and Arctic coasts and fjords, rather than
directly incorporated in the bottom layers of the glacier. Those grains were
then ice-rafted southwards by the EGC when the ice was released from the
fjords. A similar origin was proposed for HSGs deposited at the SE Greenland
coast based on a multi-proxy study (Alonso-Garcia et al., 2013).
In that study, periods of high HSG abundance were associated with strong ice
export from the Arctic via the EGC.</p>
      <p>Variations in Arctic ice export show a significant correlation with Arctic
Oscillation (AO) during the last decades (Mysak, 2001; Rigor et al.,
2002), with higher Arctic ice export during intervals of positive AO,
although this correlation is not so straightforward because Arctic ice
export also depends on the meridional wind components and the position of
the atmospheric pressure centres (Hilmer and Jung, 2000), and
large anomalies in ice export may have a different origin
(Lehner et al., 2013). Darby et al. (2012)
demonstrated that the sources of Arctic sea ice may change following the AO,
and therefore we can observe changes in the mineralogy transported by the
ice in sediment cores influenced by the EGC. During the negative state of
the AO a strong high-pressure system dominates the Beaufort Sea restricting
the Transpolar Drift to the Siberian side of the Arctic Ocean (Mysak,
2001; Rigor et al., 2002), which would bring drift ice with HSGs from the
areas of Severnaya Zemlya and Franz Josef Land. The increase in HSG relative
abundance and concentration at Eirik Drift after AD 1400 (Fig. 3) may be
driven by an intensification in ice export from those areas in the Arctic
and northern Greenland rich in HSGs, very likely favoured by atmospheric
changes which promoted higher pressures in the Arctic. The increase in HSGs
coincides with a shift observed in the sodium concentration (Na<inline-formula><mml:math id="M62" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, Fig. 3)
in Greenland ice core GISP2 (Meeker and Mayewski, 2002), which
was interpreted as an increase in storminess by <inline-formula><mml:math id="M63" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1400.
Enhanced storminess favours the transport of icebergs and sea ice through
the EGC as well as the deposition of HSGs in the sea ice and on top of
glaciers, and both processes increase the number of HSGs transported to Eirik
Drift. Greenland temperature also shows a decreasing trend after
<inline-formula><mml:math id="M64" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1400 (Kobashi et al., 2010). The sedimentary
record of Feni Drift (Bond et al., 2001), in the NE Atlantic, also
shows an increase in HSG relative abundance during the LIA interval (Fig. 3).
Colder atmospheric temperatures and the increase in ice drifted from the
Arctic may have contributed to decrease subpolar sea surface temperature,
favouring icebergs to reach areas further south such as Feni Drift
(Bond et al., 2001).</p>
      <p>Coal-bearing sediments are present at many areas around the Arctic such as
Siberia, northern Canada, Greenland and Scandinavia
(Polar Region Atlas, 1978; Petersen et al., 2013)
and contribute to high-latitude IRD deposition (Bischof and Darby, 1997;
McManus et al., 1996). Even though the percentage of coal fragments is
rather low at our study site (under 5 %; see Fig. 2) the higher abundance
of coal fragments in the Labrador Sea during the MCA may be related to an
increase in drift ice from the Canadian Arctic during the positive state of
NAO/AO. However, these fragments might also indicate human-related activity
which increased in the area during the MCA. Further analysis should be
performed to assess the linkage of those grains to any specific source.</p>
      <p>Regardless of the mineralogy of the grains, it is worth noting the high number
of lithics per gram of sediment recorded in several samples during the MCA
(Fig. 2). A recent comprehensive study of the last 2 millennia
(PAGES 2k Consortium, 2013) shows this interval presented
sustained warm temperatures from AD 830 to 1100 in the Northern
Hemisphere, including the Arctic region. The high occurrence of IRD from
AD 1000 to 1250 suggests that during the MCA either a substantial amount
of icebergs drifted to the study area or the drifting icebergs contained
considerable amounts of IRD, or a combination of both explanations. Several
studies on East Greenland glaciers and fjords point to the consistent
relationship between calving rate acceleration and the presence of warm
Atlantic water in East Greenland fjords, brought by the Irminger Current
(Andresen et al., 2012; Jennings and Weiner, 1996). Warm atmospheric
temperatures as well as the presence of Atlantic water prevent the formation
of sea ice in the fjords and in front of the glacier, thus increasing the
calving rate by destabilizing the glacier tongue (Andresen et al., 2012;
Murray et al., 2010). When tidewater glaciers are released from the sea ice,
their speed increases due to the decreased flow resistance and increased
along-flow stresses during the retreat of the ice front, and rapid changes
may be observed in calving rates in response to disequilibrium at the front
(Joughin et al., 2008). At present, Kangerdlugssuaq and Helheim
glaciers, located in the central East Greenland coast, represent the 35 %
of East Greenland's total discharge (Rignot and
Kanagaratnam, 2006). If conditions during the MCA were similar to or warmer
than present, the calving rates of these glaciers may have been even
higher than at present, delivering vast numbers of icebergs to the EGC,
where they would release IRD as they melted. Moreover, during the MCA it is
likely that other fjords, such us Nansen and Scoresby Sund, were also ice
free during the summer, allowing them to contribute considerable numbers of
icebergs to the EGC. The massive diamicton found in Nansen fjord sediments
between AD 730 and 1100 demonstrates that there was continuous iceberg
rafting due to warmer conditions (Jennings and Weiner, 1996). In
this context, we postulate that warm temperatures were the driver of the
increased iceberg calving at Greenland fjords and the high accumulation of
IRD at Eirik Drift during late MCA.</p>
      <p>After AD 1250 several spikes of high IRD abundance occurred during the
intervals AD 1400–1450, 1650–1700 and 1750–1800 (Fig. 2). Because
those intervals occurred within the LIA and under cold conditions, the
trigger of iceberg production must have been slightly different from the
drivers proposed for the MCA ice-rafting events. These intervals of high IRD
accumulation during the LIA are characterized by slightly lower relative
abundance of HSGs and higher relative abundance of volcanic grains and other
fragments. This points to an intensification of SE Greenland production of
icebergs during the LIA intervals of enhanced ice rafting. Therefore, for
the LIA events, we advocate for the same mechanism that was put forward to
explain rapid releases of icebergs in Denmark Strait during the last
150 years
(Alonso-Garcia et al., 2013). During cold periods sea ice
becomes perennial along the Greenland coast, blocking the seaward advance of
glaciers and hindering icebergs from calving, thus leading to the
accumulation of ice mass in the fjords. Based on model simulations, when the
sea ice opens or breaks, the ice flow at the grounding line accelerates very
quickly, triggering a rapid release of the grounded ice stream
(Mugford and Dowdeswell, 2010). In summary, we propose that the
high IRD occurrence during the intervals AD 1350–1450, 1650–1700 and
1750–1800 very likely corresponds to episodes of rapid iceberg release
from SE Greenland fjords. Interestingly, the timing of these intervals of
high IRD deposition coincides with the intervals of most negative
volcanic–solar forcing described by the PAGES 2k Consortium (2013).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>Comparison of IRD records from site GS06-144-03 with subpolar
North Atlantic records of sea surface temperature, ice rafting and sea ice.
<bold>(a)</bold> Atlantic Multidecadal Oscillation (AMO) SST anomaly (Mann et al., 2009);
<bold>(b)</bold> <italic>N. pachyderma </italic>dex <inline-formula><mml:math id="M65" 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 record from the Norwegian Sea (Sejrup et al.,
2010); <bold>(c)</bold> <italic>T. quinqueloba</italic> <inline-formula><mml:math id="M66" 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 record from site RAPiD-35-25B at Eirik Drift;
<bold>(d)</bold> HSG relative abundance from site GS06-144-03 (solid line, this study) and
from Feni Drift (dashed line; Bond et al., 2001); <bold>(e)</bold> sea ice index (IP25)
from site MD99-2275, NW of Iceland (Massé et al., 2008); <bold>(f)</bold> diatom-based
winter SST from site MD99-2275 (Jiang et al., 2007); <bold>(g)</bold> relative abundance
of the Atlantic waters indicator <italic>Cassidulina teretis</italic> from Nansen Fjord (Jennings and Weiner,
1996); <bold>(h)</bold> relative abundance of <italic>N. pachyderma</italic> sin from Eirik Drift (Moffa-Sanchez et al.,
2014b); <bold>(i)</bold> planktic foraminifer <inline-formula><mml:math id="M67" 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 Eirik Drift (<italic>G. bulloides</italic> from
Moffa-Sanchez et al., 2014a; <italic>N. pachyderma</italic> sin from this study); <bold>(j)</bold> quartz vs. plagioclase
ratio, a proxy for ice rafting, from MD99-2263 (Andrews et al., 2009); and
<bold>(k)</bold> total IRD concentration from site GS06-144-03 (this study). Light-blue
vertical bars indicate the periods in which IRD concentration is higher at
site GS06-144-03.</p></caption>
          <?xmltex \igopts{width=207.705118pt}?><graphic xlink:href="https://cp.copernicus.org/articles/13/317/2017/cp-13-317-2017-f04.jpg"/>

        </fig>

</sec>
<sec id="Ch1.S5.SS2">
  <title>Influence of ice rafting on SPG conditions and climate during the last
millennium</title>
      <p>Our IRD records have been compared with other palaeoceanographic and
palaeoclimatic records from Eirik Drift and other subpolar North Atlantic
sites to obtain a better picture of subpolar conditions during the last
millennium. The planktonic foraminifer <inline-formula><mml:math id="M68" 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 record of <italic>N. pachyderma</italic> sin from
Eirik Drift (this study) indicates slightly lower temperatures after AD 1050 (Fig. 4i).
A study from the same region presented a <inline-formula><mml:math id="M69" 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
record of <italic>Globigerina bulloides</italic> (Fig. 4i)
and relative abundance of <italic>N. pachyderma</italic> sinistral (Fig. 4h)
(Moffa-Sanchez et al., 2014a, b), which suggest
a cooling episode during late MCA (<inline-formula><mml:math id="M70" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1100) and a clear
drop in temperature after AD 1200. The coincidence of these temperature
drops with the increasing trend in total IRD concentration at site
GS06-144-03 indicates that the growing iceberg production at East Greenland
fjords, due to the MCA warm conditions, started to cool and freshen Labrador
Sea several centuries before the LIA started. The quartz / plagioclase ratio,
a bulk measure of IRD (Moros et al., 2004), also shows an
increasing trend at the end of the MCA at sites in Denmark Strait
(Andrews et al., 2009; see Fig. 4j) and off northern
Iceland (Moros et al., 2006), providing further evidence for the
intensification of iceberg calving at this time. Colder winter sea surface
conditions have also been recorded off N Iceland after AD 1200
(Jiang et al., 2007; see Fig. 4f), although sea surface
conditions were not cold enough to generate long seasons of severe sea ice
until <inline-formula><mml:math id="M71" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1300 (Massé et al., 2008;
see Fig. 4e), when annual SST had substantially decreased
(Sicre et al., 2008). SE Greenland sea ice and SST proxies
(Fig. 3a and b) indicate an increase in sea ice and SST decrease at
<inline-formula><mml:math id="M72" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1200 (Miettinen et al., 2015). The reduction
in the relative abundance of the benthic foraminifer <italic>Cassidulina teretis</italic> between AD 1000 and 1300
in Nansen fjord indicates a weaker influence of Atlantic water at the
East Greenland coast (Jennings and Weiner, 1996). This decline in
Atlantic water may be explained by a weakening in the northern branch of the
Irminger current which would have favoured the SST decrease and sea ice
formation in SE Greenland coast and in Denmark Strait and north of Iceland.
Blindheim and Malmberg (2005) associated the northern Irminger
current weakening with high pressure over Greenland and weaker northerly
winds. In addition, the mineralogical composition and biomarker study of the
last 2000 years in several sites in Denmark Strait and north of Iceland
indicate a change to cold conditions at <inline-formula><mml:math id="M73" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1250 very
likely associated with an intensification of the high pressure over
Greenland and the strengthening of N and NW winds, which led to progressive
presence of sea ice exported from the Arctic during winter and spring
(Andrews et al., 2009).</p>
      <p>The anomalously high Atlantic temperatures recorded during the interval
<inline-formula><mml:math id="M74" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 950–1100 (Mann et al., 2009) may indicate
SPG circulation was in the strong mode during that time interval (Figs. 4a
and 5c). Strong SPG circulation enhances the supply of warm Atlantic
Intermediate water to the East Greenland coast, which promotes calving and,
subsequently, increases the ice input in the Labrador Sea region. Switches
from weak to strong SPG circulation may happen naturally due to external or
internal forcings, and these changes are currently a matter of debate
because of their influence on North Atlantic climate (e.g.
Hakkinen and Rhines, 2004). According to model simulations, freshwater input
(i.e. ice input) to the SPG may trigger weakening of SPG circulation, and
this may be amplified successively by positive feedbacks resulting in
further weakening and freshening of the gyre due to the attenuation of the
Irminger Current (Born et al., 2010, 2016; Moreno-Chamarro
et al., 2017). Specifically for this time interval, it is important that the
main freshwater input reached the Labrador Sea, affecting deep water
formation, because a freshwater input into the Nordic Seas may have driven
the opposite effect (Born and Stocker, 2014). Our IRD record
demonstrates an increase in the amount of ice transported by the EGC to the
Labrador Sea from AD 1000 to 1250, with a potential main source in SE
Greenland. This input of freshwater to the SPG potentially drove a slowdown
of deep convection in this area and weakened the SPG circulation. A recent
study also points to enhanced input of the Labrador Current to the Labrador
Sea from <inline-formula><mml:math id="M75" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1000 to 1300
(Sicre et al., 2014), which indicates calving
intensified in SW Greenland and Baffin Bay regions as well. It is likely that ice
from both sources, East and West Greenland, directly affected the salinity
balance of Labrador Sea water and deep convection in this region. However,
even though the freshwater input started at <inline-formula><mml:math id="M76" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1000, the
SPG circulation only started to weaken after <inline-formula><mml:math id="M77" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1250, as
suggested by a record of deep-sea corals from the NE Atlantic
(Copard et al., 2012). Moreover, our IRD data show
a lag between the first temperature drops at Eirik Drift and the decrease in
ice rafting (Fig. 4), indicating a delay between SPG weakening and Irminger
Current slowdown. It seems the SPG entered in the weak mode, because of the
reduced convection, but warm intermediate water remained in the fjords for
several years, allowing continued iceberg calving. Also, the response of
calving may be slower, particularly if SSTs were relatively warm and the
fjords were not perennially covered by sea ice. However, simulations to
reconstruct past climate changes normally are not detailed enough to
characterize the impact of direct freshwater input from Greenland to the
ocean, and its consequences after several years to decades, which would be very
interesting to better understand past climate events as the LIA.</p>
      <p>As the strength of Irminger Current input declined, the areas of SE
Greenland, Denmark Strait and north of Iceland cooled, and coastal sea ice
became perennial after AD 1450, according to the sea ice index IP<inline-formula><mml:math id="M78" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">25</mml:mn></mml:msub></mml:math></inline-formula>
(Massé et al., 2008). The <inline-formula><mml:math id="M79" 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 of <italic>N. pachyderma</italic>
sinistral (Fig. 4i, this study) and <italic>Turborotalita quinqueloba</italic> (Fig. 4c) from Eirik Drift
(Moffa-Sanchez et al., 2014b) indicate a shift to colder summer
SST in the SPG after AD 1400 (Fig. 4), which coincides with the increase
in Arctic ice export reflected by the HSGs, and the storminess
intensification (Fig. 3c), recorded by the Na<inline-formula><mml:math id="M80" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> content in the
Greenland ice core GISP (Meeker and Mayewski, 2002). Planktic
<inline-formula><mml:math id="M81" 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 and Mg <inline-formula><mml:math id="M82" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Ca from sites in the Norwegian Sea (Fig. 4b)
display an initial decrease in temperature at AD 1200, and a subsequent
distinct downward shift at <inline-formula><mml:math id="M83" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1400, which suggests not
only SST cooling but also a decline in the stratification of the water
column, very likely linked to changes in the upper-ocean conditions in this
region as well (Nyland et al., 2006; Sejrup et al., 2010).</p>
      <p>It is clear that sea surface conditions in the SPG were rather different
before and after <inline-formula><mml:math id="M84" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1200. The freshening of the SPG and
the increase in sea ice along the Greenland and Iceland coasts may have been
associated with a change in atmospheric conditions, weakening winter
circulation over the Arctic and promoting more storminess in the subpolar
area and the development of atmospheric blocking events
(Moreno-Chamarro et al., 2017). Model simulations point to the
development of frequent and persistent atmospheric blocking events, induced
by low solar irradiance, as one of the main drivers to develop the
consecutive cold winters documented in Europe during the LIA (Barriopedro
et al., 2008; Moffa-Sanchez et al., 2014a). Atmospheric blocking events
derive from instabilities of the jet stream which divert or block the
pathway of the westerly winds (Häkkinen et al., 2011). These events
typically predominate during winter and occur linked to high pressure in the
Arctic and a weak polar vortex. The cold SST events recorded at the subpolar
area during the last millennium (Moffa-Sanchez et al., 2014a, b;
Sejrup et al., 2010) suggest that atmospheric
blocking events affected the entire North Atlantic regional climate.</p>
</sec>
<sec id="Ch1.S5.SS3">
  <title>Implications for LIA origin and Norse colonies</title>
      <p>It is worth noting that our IRD record shows two types of ice-rafting
events: ice rafting related to warm temperatures (during the MCA), and
ice rafting linked to rapid releases of the ice accumulated in the fjords
due to cold conditions (during the LIA). During the LIA, the events of
maximum ice rafting are coherent with the minimum values of solar irradiance
(Steinhilber et al., 2009), particularly with the Wolf,
Spörer, and Maunder minima (Fig. 5). Ice-rafting events in our record
tend to happen during intervals of low solar irradiance and cold
temperatures in the SPG, often with also significantly cold summer SST (Fig. 4c and i).
The reconstruction of radiative forcing based on solar
irradiance and volcanic eruptions
(Sigl et al., 2015) also shows
low values during the main events of high IRD occurrence (Fig. 5).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p>Sequence of events during the transition from the MCA to LIA and
linkage to potential forcings. <bold>(a)</bold> Hematite-stained grains (HSGs) relative
abundance at site GS06-144-03; <bold>(b)</bold> Na<inline-formula><mml:math id="M85" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> record from GISP2 (Meeker and
Mayewski, 2002); <bold>(c)</bold> Atlantic Multidecadal Oscillation (AMO) SST anomaly
(Mann et al., 2009); <bold>(d)</bold> SE Greenland April sea ice concentration (Miettinen
et al., 2015); <bold>(e)</bold> total IRD concentration at site GS06-144-03;
<bold>(f)</bold> reconstruction of total solar irradiance based on <inline-formula><mml:math id="M86" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula>Be isotopes from
ice cores (Steinhilber et al., 2009); and <bold>(g)</bold> radiative forcing based on volcanic
eruption reconstructions (Sigl et al., 2015). During the interval shaded in
red SPG circulation was stronger, according to the interpretations of this
work, whereas during the interval shaded in blue SPG circulation was weaker.
The letters in the solar irradiance record indicate the minima of solar
irradiance named Oort (O), Wolf (W), Spörer (S), Maunder (M), and Dalton
(D).</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/13/317/2017/cp-13-317-2017-f05.jpg"/>

        </fig>

      <p>Solar irradiance has been put forward as the main trigger for the Holocene
cold events because low solar irradiance induces an atmospheric
reorganization in the polar region which affects not only the North Atlantic
but also the mid-latitudes of the Northern Hemisphere (e.g. Bond et
al., 2001). Several records from the high-latitude North Atlantic support
this hypothesis, displaying cold temperatures at times of solar irradiance
minima during the last millennium (Moffa-Sanchez et al., 2014a; Sejrup et
al., 2010). However, the role of solar irradiance on forcing cooling events
has been questioned during the last decade. A comprehensive review on the
topic proposed that a combination of internal climate variability and
external forcings contributed to drive Holocene cold events, including the
LIA (Wanner et al., 2011). Volcanic activity is also commonly
put forward as the main driver of atmospheric reorganizations which derived
in cooling events. Precisely dated records of ice-cap growth from Arctic
Canada and Iceland (Miller et al., 2012) showed that
LIA summer cooling and ice growth, potentially linked to volcanic forcing,
began abruptly between AD 1275 and 1300, followed by a substantial
intensification at AD 1430–1455. Moreover, a recent study about the role
of radiative forcings and climate feedbacks on global cooling over the last
millennium also concluded that the volcanic forcing is the factor that
contributed the most (Atwood et al., 2016).</p>
      <p>According to our observations, the increase in Greenland calving during the
MCA (Fig. 5e) took place before the ice caps started to grow, during an
interval of high solar irradiance (Fig. 5f), high temperatures in the
Northern Hemisphere (Fig. 5c), and low volcanic activity (Fig. 5g). This
indicates that the ice-rafting events of the MCA were not related to the
fluctuations driven by solar–volcanic forcing. Alternatively, we interpret
these events as resulting from the acceleration of calving rates in SE
Greenland glaciers, driven by warm temperatures. We postulate that the
increase in calving rates during the MCA induced a decrease in the Labrador
Sea salinity, which may have triggered the weakening of SPG circulation and
reduced convection. A decline in Labrador Sea convection reduces deep water
formation in one of the key areas of the North Atlantic, which weakens North
Atlantic circulation and, in turn, decreases oceanic heat transport to this
area (Born et al., 2010; Moreno-Chamarro et al., 2017). Once
the SPG entered in the weak mode, this area received less heat and became
more sensitive to external forcings which may have generated further
cooling. This interpretation is in agreement with recent model simulations
which suggest that a weakening of the SPG circulation could have induced the
LIA cooling, and this shift from strong to weak circulation may have been
triggered by freshwater input to the Labrador Sea (Moreno-Chamarro et
al., 2017). Subsequently, low solar irradiance intervals, possibly combined
with volcanic emissions, promoted atmospheric reorganizations which gave
rise to a weakening of the polar vortex and promoted atmospheric blocking
events, enhancing cold temperatures in the subpolar area and leading to ice
sheet growth in the Arctic region during the LIA. The development of
atmospheric blocking events in the North Atlantic, as suggested by
Moffa-Sanchez et al. (2014a), probably propagated the atmospheric cooling
across Europe and the Nordic Seas. Indeed, the first strong minimum of solar
irradiance during the last millennium (Wolf, <inline-formula><mml:math id="M87" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1300)
occurred when the Labrador Sea was already fresher and SPG circulation was
weak (Fig. 5), according to our interpretations and to Copard et al. (2012)
deep-sea corals record. The reconstructions of solar and volcanic forcings
(Fig. 5f and g) shows a trend of lower values after AD 1450 with a first
step of low values during the Wolf minimum, indicating that volcanic forcing
may also have played an important role in modifying the atmospheric
conditions. However, we consider that the decrease in Labrador Sea salinity
prior to the Wolf minimum was crucial to produce changes in SPG circulation.
Once the SPG entered the weak mode, the effects of solar and volcanic
forcing possibly produced a deeper impact on North Atlantic climate. It is
likely that the LIA would not have been such a cold and widespread event if
the SPG circulation was strong and deep convection was active at the time.</p>
      <p>The results of this study can be linked to the expansion and demise of the
Norse colonies. According to historical data, the Norse expansion and
colonization of Iceland and Greenland occurred during the warmer climate
conditions of the MCA which favoured fishing and farming in these regions
(Kuijpers et al., 2014; Ogilvie et al., 2000; Ogilvie and Jónsson,
2001; see Fig. 3). Our study indicates that, even though calving intensified
after the settlement of the Norse colonies in Greenland, climatic conditions
during the late MCA were still favourable because the strong circulation in
the SPG supplied relatively warm water to SE Greenland coast. Therefore, the
fjords were not perennially covered by sea ice and it is likely that a
rather continuous calving may have helped hunting. However, after several
decades of intense calving and melting of Greenland glaciers, the Labrador
Sea became fresher and the SPG circulation started to weaken, triggering a
change in oceanic and atmospheric conditions. The reduction of deep
convection decreased the transport of heat to the NW subpolar area and
enhanced sea ice occurrence in the fjords, which deteriorated the living
conditions in Greenland. The subsequent cooling and increase in storminess
brought by the shift in atmospheric conditions (increase in atmospheric
blocking events) very likely favoured the abandonment of the Greenland Norse
settlements at the beginning of the LIA (Dugmore et al., 2012; Ogilvie et
al., 2000, Fig. 3).</p>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <title>Conclusions</title>
      <p>Sediments from Eirik Drift were studied in order to examine the variations
in ice rafting during the last millennium and its linkage to LIA
development. IRD in the 63–150 <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> fraction shows the highest
concentration during the intervals <inline-formula><mml:math id="M89" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> AD 1000–1100,
<inline-formula><mml:math id="M90" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1150–1250, <inline-formula><mml:math id="M91" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1400–1450, <inline-formula><mml:math id="M92" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1650–1700 and <inline-formula><mml:math id="M93" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1750–1800. The identification of
different minerals allowed us to link the IRD with potential sources and
better interpret the ice-rafting events. The main IRD source was along the
SE Greenland coast, although during the LIA the greater concentration and
relative abundance of HSGs support an increase in the contribution of ice
exported from the Arctic region and NE Greenland via the EGC. Two different
types of ice-rafting events have been recognized: (1) ice rafting recorded
during the MCA, which we interpret as being related to the acceleration of
calving rates in SE Greenland glaciers driven by warm oceanic and
atmospheric temperature and (2) ice rafting events during the LIA, which
have been linked to rapid releases of the ice accumulated in the fjords due
to the perennial sea ice developed in the Greenland coast during cold
periods.</p>
      <p>The comparison of our IRD records with other North Atlantic reconstructions
of ice rafting, sea surface, and deep ocean conditions provides a better
picture of the development of the LIA in the subpolar region. We postulate
that the enhanced ice discharge during the MCA, due to warm conditions,
decreased sea surface salinity in the Labrador Sea, which in turn reduced
Labrador Sea convection and weakened SPG circulation. The reduction in
convection in the Labrador Sea, one of the key areas of deep water formation
in the North Atlantic, potentially weakened the North Atlantic circulation
and decreased oceanic heat transport to the high latitudes, particularly to
the Labrador Sea region. In other words, the reduced convection also
diminished the arrival of warm water from the NAC to SE Greenland coasts,
inducing perennial sea ice occurrence and cooling the atmosphere which
promoted ice sheet growth in the Arctic. The subsequent atmospheric and
oceanographic reorganizations induced by external forcings, such as solar
and volcanic forcing, generated extremely cold conditions in the North
Atlantic during the LIA, with the development of atmospheric blocking events
which boosted further cooling and harsh conditions across Europe and the
Nordic Seas, and led the Norse to abandon their colonies in Greenland around
AD 1400 because of their maladaptation to cold climate conditions
(Dugmore et al., 2012).</p>
      <p>This study puts forward the idea that the development of the exceptionally
cold conditions during the LIA may be better explained by the previous
freshening of the Labrador Sea due to enhanced ice rafting during the MCA
and the subsequent weakening of the SPG circulation. This finding may be
fundamental to model future climate conditions given that calving in the SE
Greenland glaciers has been increasing during the last decade (Andresen
et al., 2012; Straneo et al., 2013).</p>
</sec>

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

      <p>Data can be obtained from Pangaea at <uri>https://doi.pangaea.de/10.1594/PANGAEA.874286</uri>
(Alonso-Garcia, 2017).</p>
  </notes><notes notes-type="competinginterests">

      <p>The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p>This project was funded by NSF grants OCE-0961670 and
OCE-1258984, and the Comer Science and Education Foundation grant CP75.
The authors would like to thank the reviewers and editor for their insightful comments which contributed to improving the
manuscript. Tony Greco is acknowledged for analytical support with the SEM analysis. M. Alonso-Garcia
would like to acknowledge the support from A. E. Shevenell, J. Dixon, and D. Hollander
during her postdoc at USF, and funding from Portuguese National
Science and Technology Foundation (FCT) through the postdoctoral fellowship
SFRH/BPD/96960/2013 and CCMAR funds UID/Multi/04326/2013.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: A. Dutton<?xmltex \hack{\newline}?>
Reviewed by: J. Andrews and two anonymous referees</p></ack><ref-list>
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    <!--<article-title-html>Freshening of the Labrador Sea as a trigger for  Little Ice Age development</article-title-html>
<abstract-html><p class="p">Arctic freshwater discharges to the Labrador Sea from melting glaciers and
sea ice can have a large impact on ocean circulation dynamics in the North
Atlantic, modifying climate and deep water formation in this region. In this
study, we present for the first time a high resolution record of ice rafting
in the Labrador Sea over the last millennium to assess the effects of
freshwater discharges in this region on ocean circulation and climate. The
occurrence of ice-rafted debris (IRD) in the Labrador Sea was studied using
sediments from Site GS06-144-03 (57.29° N, 48.37° W;
3432 m water depth). IRD from the fraction 63–150 µm shows
particularly high concentrations during the intervals
 ∼  AD 1000–1100,  ∼  1150–1250,  ∼  1400–1450,
 ∼  1650–1700 and  ∼  1750–1800. The first two
intervals occurred during the Medieval Climate Anomaly (MCA), whereas the
others took place within the Little Ice Age (LIA). Mineralogical
identification indicates that the main IRD source during the MCA was SE
Greenland. In contrast, the concentration and relative abundance of
hematite-stained grains reflects an increase in the contribution of Arctic
ice during the LIA.</p><p class="p">The comparison of our Labrador Sea IRD records with other climate proxies
from the subpolar North Atlantic allowed us to propose a sequence of
processes that led to the cooling that occurred during the LIA, particularly
in the Northern Hemisphere. This study reveals that the warm climate of the
MCA may have enhanced iceberg calving along the SE Greenland coast and, as a
result, freshened the subpolar gyre (SPG). Consequently, SPG circulation
switched to a weaker mode and reduced convection in the Labrador Sea,
decreasing its contribution to the North Atlantic deep water formation and,
thus, reducing the amount of heat transported to high latitudes. This
situation of weak SPG circulation may have made the North Atlantic climate
more unstable, inducing a state in which external forcings (e.g. reduced
solar irradiance and volcanic eruptions) could easily drive periods of
severe cold conditions in Europe and the North Atlantic like the LIA. This
analysis indicates that a freshening of the SPG may play a crucial role in
the development of cold events during the Holocene, which may be of key
importance for predictions about future climate.</p></abstract-html>
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