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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Earth Sci.</journal-id>
<journal-title>Frontiers in Earth Science</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Earth Sci.</abbrev-journal-title>
<issn pub-type="epub">2296-6463</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.3389/feart.2017.00084</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Earth Science</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Evidence of Poor Bottom Water Ventilation during LGM in the Equatorial Indian Ocean</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name><surname>Chandana</surname> <given-names>K. R.</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
<xref ref-type="author-notes" rid="fn001"><sup>&#x0002A;</sup></xref>
<uri xlink:href="http://loop.frontiersin.org/people/417789/overview"/>
</contrib>
<contrib contrib-type="author">
<name><surname>Bhushan</surname> <given-names>Ravi</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
<uri xlink:href="http://loop.frontiersin.org/people/263952/overview"/>
</contrib>
<contrib contrib-type="author">
<name><surname>Jull</surname> <given-names>A. J. T.</given-names></name>
<xref ref-type="aff" rid="aff2"><sup>2</sup></xref>
<uri xlink:href="http://loop.frontiersin.org/people/486368/overview"/>
</contrib>
</contrib-group>
<aff id="aff1"><sup>1</sup><institution>Geosciences Division, Physical Research Laboratory</institution>, <addr-line>Ahmedabad</addr-line>, <country>India</country></aff>
<aff id="aff2"><sup>2</sup><institution>NSF Arizona AMS Laboratory, University of Arizona</institution>, <addr-line>Tucson, AZ</addr-line>, <country>United States</country></aff>
<author-notes>
<fn fn-type="edited-by"><p>Edited by: David K. Wright, Seoul National University, South Korea</p></fn>
<fn fn-type="edited-by"><p>Reviewed by: Nadia Solovieva, University College London, United Kingdom; Nicolas Tribovillard, Lille University of Science and Technology, France</p></fn>
<fn fn-type="corresp" id="fn001"><p>&#x0002A;Correspondence: Chandana K. R. <email>chandana9murthy&#x00040;gmail.com</email></p></fn>
<fn fn-type="other" id="fn002"><p>This article was submitted to Quaternary Science, Geomorphology and Paleoenvironment, a section of the journal Frontiers in Earth Science</p></fn></author-notes>
<pub-date pub-type="epub">
<day>24</day>
<month>10</month>
<year>2017</year>
</pub-date>
<pub-date pub-type="collection">
<year>2017</year>
</pub-date>
<volume>5</volume>
<elocation-id>84</elocation-id>
<history>
<date date-type="received">
<day>04</day>
<month>08</month>
<year>2017</year>
</date>
<date date-type="accepted">
<day>05</day>
<month>10</month>
<year>2017</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#x000A9; 2017 Chandana, Bhushan and Jull.</copyright-statement>
<copyright-year>2017</copyright-year>
<copyright-holder>Chandana, Bhushan and Jull</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/"><p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p></license>
</permissions>
<abstract>
<p>Multi-proxy approach for the reconstruction of paleo-redox conditions is attempted on a radiocarbon (<sup>14</sup>C) dated sediment core near the equatorial Indian Ocean. Based on the behavior and distribution of redox sensitive and productivity proxies, study demonstrates prevalence of anoxic bottom water conditions during LGM due to poorly ventilated bottom waters augmented by high surface productivity resulting in better preservation of organic carbon (OC). During early Holocene, the equatorial Indian Ocean witnessed high sedimentation rates resulting in high organic carbon (OC) with depleted redox sensitive elements thereby causing better preservation of OC. The study underscores poor bottom water ventilation during LGM and preservation of OC as a result of high sedimentation rate in early Holocene.</p>
</abstract>
<kwd-group>
<kwd>LGM</kwd>
<kwd>anoxic bottom water</kwd>
<kwd>holocene period</kwd>
<kwd>redox sensitive elements</kwd>
<kwd>organic carbon</kwd>
<kwd>GEOTRACES</kwd>
</kwd-group>
<counts>
<fig-count count="6"/>
<table-count count="1"/>
<equation-count count="0"/>
<ref-count count="77"/>
<page-count count="10"/>
<word-count count="7261"/>
</counts>
</article-meta>
</front>
<body>
<sec sec-type="intro" id="s1">
<title>Introduction</title>
<p>The depositional conditions in the marine environment can be oxic, suboxic and anoxic based on the presence or absence of oxygen at the sediment-water interface. Redox sensitive elements have demonstrated their potential in deciphering the past bottom water anoxic condition in the oceanic basin. The elemental concentrations in marine sediments are mainly controlled by various processes such as terrestrial influx, biological processes, <italic>in-situ</italic> precipitation, and/or by hydrothermal activity (Pattan and Pearce, <xref ref-type="bibr" rid="B47">2009</xref>). The oxygen concentration in bottom water plays an important role in altering oxygen gradients in the sedimentary column and this in turn depends upon change in deep water circulation during the past glacial-interglacial period (Bareille et al., <xref ref-type="bibr" rid="B9">1998</xref>; Ahmad et al., <xref ref-type="bibr" rid="B3">2008</xref>; Pattan and Pearce, <xref ref-type="bibr" rid="B47">2009</xref>).</p>
<p>Based on the dissolved oxygen (O<sub>2</sub>) and/or hydrogen sulfide (H<sub>2</sub>S) concentrations, the sedimentary environment has been categorized as oxic (&#x0003E;2.0 ml O<sub>2</sub> l<sup>&#x02212;1</sup>), suboxic/dysoxic (2.0&#x02013;0.2 ml O<sub>2</sub> l<sup>&#x02212;1</sup>), and anoxic/euxinic (0.2&#x02013;0 ml O<sub>2</sub> l<sup>&#x02212;1</sup>) (Tyson and Pearson, <xref ref-type="bibr" rid="B74">1991</xref>). In addition to oxygen concentration, the labile organic matter (OM) also controls the redox element cycling in the bottom water. Under oxic conditions, aerobic bacteria utilizes dissolved oxygen for OM degradation, while with decrease in dissolved O<sub>2</sub>, the degradation continues using secondary oxidant sources leading to oxygen deficient conditions in the water column. Redox sensitive elements are often portrayed as classic tool to reconstruct the past depositional conditions in the bottom water (Brumsack, <xref ref-type="bibr" rid="B11">1980</xref>, <xref ref-type="bibr" rid="B12">2006</xref>; Calvert and Pedersen, <xref ref-type="bibr" rid="B13">1993</xref>; Dean et al., <xref ref-type="bibr" rid="B19">1999</xref>; Algeo and Tribovillard, <xref ref-type="bibr" rid="B6">2009</xref>). The redox elements such as Mo, V, Cr, Mn have different solubilities in marine water depending on the redox conditions and has been commonly used to trace anoxic conditions near the sediment-water interface (Agnihotri et al., <xref ref-type="bibr" rid="B2">2003</xref>; Rimmer, <xref ref-type="bibr" rid="B59">2004</xref>; Algeo and Lyons, <xref ref-type="bibr" rid="B4">2006</xref>; Tribovillard et al., <xref ref-type="bibr" rid="B72">2006</xref>; Banerji et al., <xref ref-type="bibr" rid="B8">2016</xref>). In oxic waters, Mn gets precipitated as Mn-oxides into the sediments, while V as vanadate oxyanions (<inline-formula><mml:math id="M1"><mml:msubsup><mml:mrow><mml:mtext>HVO</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> and H<sub>2</sub>VO<sup>4&#x02212;</sup>), Mo as molybdate (<inline-formula><mml:math id="M2"><mml:msubsup><mml:mrow><mml:mtext>MoO</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>) Cr as chromate anions (<inline-formula><mml:math id="M3"><mml:msubsup><mml:mrow><mml:mtext>CrO</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>) are present in dissolved form. Unlike Mn, all other redox sensitive elements are conservative in oxygenated waters with a constant concentration, but under anoxic conditions they are highly enriched in sediments especially where bottom water oxygen is zero (Calvert and Pedersen, <xref ref-type="bibr" rid="B13">1993</xref>, <xref ref-type="bibr" rid="B14">1996</xref>; Algeo and Lyons, <xref ref-type="bibr" rid="B4">2006</xref>; Tribovillard et al., <xref ref-type="bibr" rid="B72">2006</xref>; Pattan and Pearce, <xref ref-type="bibr" rid="B47">2009</xref>).</p>
<p>The Indian Ocean being situated in mid-way of global conveyor belt, between the Atlantic deep water formation and return of surface water from the Pacific, deep waters in the Indian Ocean are ventilated only from south (Piotrowski et al., <xref ref-type="bibr" rid="B50">2009</xref>). Presently, in the Northern Indian Ocean (NIO), intermediate depths comprises high salinity water masses such as Red Sea, Persian Gulf Waters and contribution from Pacific Ocean through Indonesian Archipelago at depths of 500 to 1,500 m (Kallel et al., <xref ref-type="bibr" rid="B33">1988</xref>). The Indian Ocean deep water is mainly North Atlantic Deep Water (NADW) between &#x0007E;2,000&#x02013;4,000 m relatively rich in dissolved oxygen compared to Antarctic Bottom Water (AABW) found below &#x0007E;4,000 m (Sarkar et al., <xref ref-type="bibr" rid="B61">1993</xref>). Various studies have shown that during last glacial period, the formation rate of the NADW was reduced, while the AABW remained unchanged or probably enhanced (Duplessy et al., <xref ref-type="bibr" rid="B23">1988</xref>; Ahmad et al., <xref ref-type="bibr" rid="B3">2008</xref>).</p>
<p>High resolution paleoclimatic records from late-Quaternary sediments has become increasingly useful tool for deciphering variability in sedimentary paleoproductivity and paleoredox conditions (Ivanochko and Pedersen, <xref ref-type="bibr" rid="B32">2004</xref>; Hendy and Pedersen, <xref ref-type="bibr" rid="B30">2005</xref>; Dean et al., <xref ref-type="bibr" rid="B20">2006</xref>; Cartapanis et al., <xref ref-type="bibr" rid="B16">2011</xref>). A study based on organic carbon (OC) and Mn concentrations from the Arabian Sea, suggested deposition of sediments under oxic conditions during deglacial period as a result of lower productivity and high Mn concentration (Shetye et al., <xref ref-type="bibr" rid="B65">2014</xref>). The prevalence of near anoxic bottom water conditions during glacial cycle has been demonstrated based on U and OC content in marine sediment from the SE Arabian Sea (Sarkar et al., <xref ref-type="bibr" rid="B61">1993</xref>). Study based on Mo and V concentrations near the SE Arabian Sea suggested prevalence of suboxic conditions during LGM (Pattan and Pearce, <xref ref-type="bibr" rid="B47">2009</xref>). During LGM, reduced proportion of NADW and increased proportion of AABW near the equatorial Indian Ocean has been inferred on the basis of Nd-isotopic composition of ferromagnese oxides and &#x003B4;<sup>13</sup>C of foraminifera implying a major trigger in the development of oxygen deficient bottom conditions (Piotrowski et al., <xref ref-type="bibr" rid="B50">2009</xref>). There have been substantial studies indicating the development and persistence of oxygen deficient conditions in the Northern Indian Ocean that are related to either productivity or change in bottom water conditions (Naqvi, <xref ref-type="bibr" rid="B42">1987</xref>; Pailler et al., <xref ref-type="bibr" rid="B46">2002</xref>; Rao et al., <xref ref-type="bibr" rid="B55">2010</xref>). However, there remains unaddressed issues on the simultaneous signatures of productivity and bottom water anoxia on redox sensitive elements. Thus, to address the role of productivity and thermohaline ventilation during glacial-interglacial periods, a sediment core (SK-304A/05) from the intermixing zone of two distinct basins of NIO near the equatorial region was geochemically investigated. This study attempts to substantiate the influence of both productivity and the bottom water ventilation during glacial-interglacial period near the equatorial region of NIO. The objectives of the present study is (i) to reconstruct the redox conditions during glacial-interglacial periods and (ii) to identify the variations in the bottom water oxygen conditions with its causative mechanism during the last 25 ka years BP.</p>
</sec>
<sec id="s2">
<title>Present day oceanographic setting</title>
<p>The Northern Indian Ocean is unique compared to the other oceans due to its topographical setting as it comprises two basins i.e., the Arabian Sea and the Bay of Bengal being separated by Indian subcontinent. The land-ocean thermal contrast leads to seasonal reversal of winds. During summer (June-September) the monsoonal winds are south-westerly (SW) and during winter (November-February) the monsoonal winds are north-easterly (NE) (Tomczak and Godfrey, <xref ref-type="bibr" rid="B71">2003</xref>). In response to wind, surface currents also reverses its direction in the equatorial Indian Ocean. During summer monsoon, a branch of Somali current (SC) at 4&#x000B0; turns offshore and supplies the summer monsoon current (SMC) flowing eastward. In addition to SC, the SMC also receives water from southward flowing West Indian Coastal Current (WICC) (Tiwari et al., <xref ref-type="bibr" rid="B70">2006</xref>). As SMC reaches Sri Lanka, it turns northward to Bay of Bengal by flowing around the cyclonic Sri Lanka Dome (SD) and feeding the northeastward flowing East Indian Coast Current (EICC) (Tiwari et al., <xref ref-type="bibr" rid="B70">2006</xref>). Thus, the SMC along with the WICC flows from west to east transporting highly saline water from the Arabian Sea to the Bay of Bengal. During winter monsoon, EICC reverses its direction and flows in southwest direction feeding low salinity water to the west flowing northeast monsoon current (NMC), which in turn contributes to northward flowing WICC (Schott and McCreary, <xref ref-type="bibr" rid="B63">2001</xref>). Thus, these currents play a crucial role in nutrient distribution and chlorophyll concentrations in the equatorial regions (Vidya et al., <xref ref-type="bibr" rid="B75">2013</xref>).</p>
<p>Geochemical investigations have shown that the equatorial Indian Ocean, off Sri Lanka is largely composed of calcareous and smectite clays (Nath, <xref ref-type="bibr" rid="B44">2001</xref>). The sediment trap study carried out for the measurement of biogenic fluxes in the Northern Indian Ocean found predominance of opal fluxes at western Arabian Sea and the Bay of Bengal. But the eastern Arabian Sea, the southern Bay of Bengal (SBBT), and the equatorial Indian Ocean (EIOT) traps are dominated by carbonate fluxes (Ramaswamy and Gaye, <xref ref-type="bibr" rid="B54">2006</xref>). Strong seasonality in the biogenic flux has been observed at SBBT while EIOT remained deprived of such seasonal variations (Vidya et al., <xref ref-type="bibr" rid="B75">2013</xref>).</p>
</sec>
<sec sec-type="methods" id="s3">
<title>Methodology</title>
<p>A &#x0007E;410 cm gravity core (SK-304A/05; water depth&#x02014;3,408 m) was raised off Srilanka (05&#x000B0;45.622&#x02032; N; 79&#x000B0;24.763&#x02032; E) in the equatorial Indian Ocean during the <italic>ORV</italic> Sagar Kanya cruise SK-304 in March 2013 (Figure <xref ref-type="fig" rid="F1">1</xref>). The core was sub-sampled at 1 cm interval with non-metallic knife to avoid metallic contamination and kept in a clean ziplock bags till further analysis. Subsamples were oven dried at 80&#x000B0;C and finely powdered with the help of agate mortar and pestle for its biogenic, geochemical and isotopic analysis.</p>
<fig id="F1" position="float">
<label>Figure 1</label>
<caption><p>Bathymetry map of Northern Indian Ocean with SK-304A/05 sediment core location retrieved during onboard ORV Sagarkanya. The sediment core lies at the mixing zone of the Arabian Sea and the Bay of Bengal near equatorial region.</p></caption>
<graphic xlink:href="feart-05-00084-g0001.tif"/>
</fig>
<p>The chronology for the upper 200 cm of the core was established based on nine AMS radiocarbon dates (<sup>14</sup>C) analyzed at NSF-AMS facility of Arizona University, USA on handpicked mixed planktonic foraminifera from different depths. The <sup>14</sup>C dates were calibrated by Calib 7.0.2 using Marine13 calibration curve (Stuiver et al., <xref ref-type="bibr" rid="B67">1998</xref>; Reimer et al., <xref ref-type="bibr" rid="B57">2009</xref>, <xref ref-type="bibr" rid="B58">2013</xref>) and were corrected with a reservoir age correction of &#x00394;R 60 &#x000B1; 52 years (Dutta et al., <xref ref-type="bibr" rid="B24">2001</xref>; Southon et al., <xref ref-type="bibr" rid="B66">2002</xref>).</p>
<p>In order to measure the trace elemental concentrations, &#x0007E;300 mg of the dried and crushed samples was subjected to closed digestion by treating it with acid mixture (HNO<sub>3</sub>, HCl, and HF) in microwave digestion system (<italic>Milestone, Start D</italic>). Trace elemental (Ti, Mo, V, Cr, Co, Mn) concentrations were measured by aspirating the digested solution in ICP-MS (<italic>Thermo-X series2</italic>). The accuracy and precision for the analysis were monitored by repeat measurements of reference sediment standards (marine sediment standards MAG-1 and NOVA) and was found to be better than &#x000B1;6 and &#x000B1;4% respectively. Calcium carbonate (CaCO<sub>3</sub>) was analyzed on Coulometer (<italic>UIC Coulometer, Model 5012</italic>) with a precision of &#x0007E;2%. Total organic carbon (OC) and total nitrogen (TN) was measured using NC Elemental Analyzer (<italic>Flash 2000</italic>) with a precision better than 0.2 and 2% respectively (Bhushan et al., <xref ref-type="bibr" rid="B10">2001</xref>).</p>
</sec>
<sec sec-type="results" id="s4">
<title>Results</title>
<sec>
<title>Chronology</title>
<p>Table <xref ref-type="table" rid="T1">1</xref> summarizes detailed AMS <sup>14</sup>C chronology results of the studied sediment core SK-304A/05 retrieved from the equatorial Indian Ocean. The reconstructed age-depth model for the sediment core based on the calibrated radiocarbon dates of foraminifers at various depths (upper 200 cm section) provides paleoclimatic records for the last 25 ka years BP (Figure <xref ref-type="fig" rid="F2">2</xref>). The sediment deposition rate at the core varies from &#x0007E;5.0 to 13.8 cm.ka<sup>&#x02212;1</sup>. The highest and the lowest sedimentation rates were observed between &#x0007E;8 to 11 ka years BP and &#x0007E;13.5 to 19.5 ka years BP respectively. An average sedimentation rate of &#x0007E;8 cm.ka<sup>&#x02212;1</sup> was observed for the studied sediment core (Figure <xref ref-type="fig" rid="F2">2</xref>). The late-Quaternary period has been broadly divided into Last Glacial Maxima (LGM: 22.5&#x02013;17.5 ka years BP), Deglacial Period (DP: 17.5&#x02013;11 ka years BP), and Holocene Period (HP: 11-Present) (Rao et al., <xref ref-type="bibr" rid="B55">2010</xref>).</p>
<table-wrap position="float" id="T1">
<label>Table 1</label>
<caption><p>Calibrated radiocarbon ages for the sediment core SK-304A/05.</p></caption>
<table frame="hsides" rules="groups">
<thead><tr>
<th valign="top" align="left"><bold>S.No</bold>.</th>
<th valign="top" align="left"><bold>Sample ID</bold></th>
<th valign="top" align="left"><bold>Laboratory ID</bold></th>
<th valign="top" align="center"><bold>Depth (cm)</bold></th>
<th valign="top" align="center"><bold>Radiocarbon age (year BP)</bold></th>
<th valign="top" align="center" colspan="2"><bold>Calibrated age 1&#x003C3; age range</bold></th>
</tr>
</thead>
<tbody>
<tr>
<td valign="top" align="left">1</td>
<td valign="top" align="left">PRL-AS-01</td>
<td valign="top" align="left">AA104059</td>
<td valign="top" align="center">4</td>
<td valign="top" align="center">2,793 &#x000B1; 32</td>
<td valign="top" align="center">2,338</td>
<td valign="top" align="center">2,528</td>
</tr>
<tr>
<td valign="top" align="left">2</td>
<td valign="top" align="left">PRL-AS-02</td>
<td valign="top" align="left">AA104060</td>
<td valign="top" align="center">11</td>
<td valign="top" align="center">3,209 &#x000B1; 32</td>
<td valign="top" align="center">2,844</td>
<td valign="top" align="center">3,013</td>
</tr>
<tr>
<td valign="top" align="left">3</td>
<td valign="top" align="left">PRL-AS-03</td>
<td valign="top" align="left">AA104061</td>
<td valign="top" align="center">21</td>
<td valign="top" align="center">4,173 &#x000B1; 33</td>
<td valign="top" align="center">4,071</td>
<td valign="top" align="center">4,257</td>
</tr>
<tr>
<td valign="top" align="left">4</td>
<td valign="top" align="left">PRL-AS-04</td>
<td valign="top" align="left">AA104062</td>
<td valign="top" align="center">40</td>
<td valign="top" align="center">5,787 &#x000B1; 35</td>
<td valign="top" align="center">6,050</td>
<td valign="top" align="center">6,217</td>
</tr>
<tr>
<td valign="top" align="left">5</td>
<td valign="top" align="left">PRL-AS-05</td>
<td valign="top" align="left">AA104063</td>
<td valign="top" align="center">60</td>
<td valign="top" align="center">8,014 &#x000B1; 38</td>
<td valign="top" align="center">8,347</td>
<td valign="top" align="center">8,476</td>
</tr>
<tr>
<td valign="top" align="left">6</td>
<td valign="top" align="left">PRL-AS-07</td>
<td valign="top" align="left">AA104065</td>
<td valign="top" align="center">101</td>
<td valign="top" align="center">10,372 &#x000B1; 44</td>
<td valign="top" align="center">1,1192</td>
<td valign="top" align="center">11,427</td>
</tr>
<tr>
<td valign="top" align="left">7</td>
<td valign="top" align="left">PRL-AS-08</td>
<td valign="top" align="left">AA104066</td>
<td valign="top" align="center">119</td>
<td valign="top" align="center">12,172 &#x000B1; 49</td>
<td valign="top" align="center">1,3459</td>
<td valign="top" align="center">13,648</td>
</tr>
<tr>
<td valign="top" align="left">8</td>
<td valign="top" align="left">PRL-AS-09</td>
<td valign="top" align="left">AA104067</td>
<td valign="top" align="center">149</td>
<td valign="top" align="center">16,642 &#x000B1; 63</td>
<td valign="top" align="center">1,9399</td>
<td valign="top" align="center">19,639</td>
</tr>
<tr>
<td valign="top" align="left">9</td>
<td valign="top" align="left">PRL-AS-10</td>
<td valign="top" align="left">AA104068</td>
<td valign="top" align="center">201</td>
<td valign="top" align="center">21,910 &#x000B1; 120</td>
<td valign="top" align="center">25,646</td>
<td valign="top" align="center">25,881</td>
</tr>
</tbody>
</table>
</table-wrap>
<fig id="F2" position="float">
<label>Figure 2</label>
<caption><p>Age-depth model of AMS dates of foraminifers at selected depth of the sediment core SK-304A/05. Linear interpolation of sedimentation rates is assumed based on the AMS dates.</p></caption>
<graphic xlink:href="feart-05-00084-g0002.tif"/>
</fig>
</sec>
<sec>
<title>Geochemical proxies</title>
<p>The downcore geochemical signatures were studied to reconstruct the paleoproductivity and paleoredox conditions prevailed during the last 25 ka years BP. Generally, Al and Ti are considered as extremely resistant to weathering and conservative elements as they remain unaffected due to changes in redox conditions (Nesbitt and Markovics, <xref ref-type="bibr" rid="B45">1997</xref>; Wei et al., <xref ref-type="bibr" rid="B76">2003</xref>) and has been extensively used to estimate the terrigenous material in the sedimentary environment (Murray and Leinen, <xref ref-type="bibr" rid="B38">1993</xref>, <xref ref-type="bibr" rid="B39">1996</xref>; Schroeder et al., <xref ref-type="bibr" rid="B64">1997</xref>; Klump et al., <xref ref-type="bibr" rid="B34">2000</xref>). Under certain circumstances, Al can form as a result of authigenic clay mineral formation (Timothy and Calvert, <xref ref-type="bibr" rid="B69">1998</xref>) or it may get scavenged as hydroxides coating over biogenic particles (Murray and Leinen, <xref ref-type="bibr" rid="B39">1996</xref>). Similar to Al, Si is also associated with biogenic opal and this limits its use as terrestrial tag. Thus, in the present study, the elements have been normalized by Ti instead of Al and Si. The Ti concentration in the studied sediment core varies between 1,923&#x02013;3,585 ppm (Figure <xref ref-type="fig" rid="F3">3</xref>). Sedimentary OC and CaCO<sub>3</sub> are important constituents of the biogenic fraction of the marine sediments, and thus can be used as a proxy for paleoproductivity. However, OC and CaCO<sub>3</sub> constitute only a fraction of total biological productivity in the surface oceanic water due to its biological degradation during its passage through the water column (Tribovillard et al., <xref ref-type="bibr" rid="B72">2006</xref>). The OC and CaCO<sub>3</sub> concentration ranges from 1.28&#x02013;5.14 to 25.30&#x02013;48.92 wt% respectively (Figures <xref ref-type="fig" rid="F4">4</xref>, <xref ref-type="fig" rid="F5">5</xref>). High OC concentration results in enhanced bacterial degradation causing oxygen deficient conditions (suboxic, anoxic, and euxinic) in the water column and at sediment-water interface. Under such oxygen deficient conditions at the sediment-water interface, the behavioral pattern of redox sensitive elements is generally used to comprehend the paleoredox conditions persisted at the time of sediment deposition. The elemental concentration of V, Mn, Cr, Mo, Ni, Co that has been used to access the paleoredox conditions ranges from 45&#x02013;110, 204&#x02013;380, 45&#x02013;91, 0.6&#x02013;2.8, 35&#x02013;90, and 7&#x02013;15 ppm respectively (Figures <xref ref-type="fig" rid="F3">3</xref>, <xref ref-type="fig" rid="F4">4</xref>).</p>
<fig id="F3" position="float">
<label>Figure 3</label>
<caption><p>Downcore variation of elemental concentration in the sediment core SK-304A/05 indicates low terrestrial flux during LGM with gradual increasing values during Deglacial and Holocene period. The dotted line in each plot indicates average crustal values for the respective elements.</p></caption>
<graphic xlink:href="feart-05-00084-g0003.tif"/>
</fig>
<fig id="F4" position="float">
<label>Figure 4</label>
<caption><p>Downcore variation of Mn, CaCO<sub>3</sub>, and Mn/Ti indicates that Mn forms authegenic carbonate in presence of CaCO<sub>3.</sub></p></caption>
<graphic xlink:href="feart-05-00084-g0004.tif"/>
</fig>
<fig id="F5" position="float">
<label>Figure 5</label>
<caption><p>Downcore variation of Ti normalized redox sensitive elements (Co, Ni, V, Mo), OC and OC flux. High values of OC and redox sensitive elements observed during LGM.</p></caption>
<graphic xlink:href="feart-05-00084-g0005.tif"/>
</fig>
</sec>
</sec>
<sec sec-type="discussion" id="s5">
<title>Discussion</title>
<p>The organic matter (Shetye et al., <xref ref-type="bibr" rid="B65">2014</xref>) and Fe- and Mn- oxyhydroxides (Tribovillard et al., <xref ref-type="bibr" rid="B72">2006</xref>) are the major sources for the transportation of the trace elements from water column to the sediments. In oxic and anoxic environments, the trace elements behave differently based on their oxidation states which is influenced by the redox conditions (Shetye et al., <xref ref-type="bibr" rid="B65">2014</xref>).</p>
<sec>
<title>Biogenic productivity during glacial interglacial periods</title>
<p>Consistently high values for the CaCO<sub>3</sub> (Figure <xref ref-type="fig" rid="F4">4</xref>) were observed during LGM with gradually declining trend during the early Holocene and subsequently marginal increase during the late Holocene. Such consistently high values suggest high calcareous productivity during LGM. Two conspicuous peaks of OC (Figure <xref ref-type="fig" rid="F5">5</xref>) during &#x0007E;21 ka years BP and at early Holocene (11&#x02013;8 ka years BP) has been observed. The early Holocene OC peak corroborates well with the abrupt increase in the sedimentation rate &#x0007E;13.5 cm.ka<sup>&#x02212;1</sup> primarily suggesting preservation of OC with efficient burial and not due to abrupt high overhead productivity. The OC peak at &#x0007E;21 ka years BP corresponding to LGM period, however, resulted due to high productivity and better OC preservation. High OC and CaCO<sub>3</sub> observed during LGM can be due to high productivity because of strong NE monsoonal winds that enhanced nutrient levels in the photic zone (Rostek et al., <xref ref-type="bibr" rid="B60">1997</xref>; Punyu et al., <xref ref-type="bibr" rid="B52">2014</xref>). With the commencement of deglacial period, weakening of NE monsoonal winds led to decrease in productivity during the Holocene period. Thus, high productivity could be one of the factors responsible for triggering reducing conditions at the sediment-water interface (Tribovillard et al., <xref ref-type="bibr" rid="B72">2006</xref>).</p>
</sec>
<sec>
<title>Redox proxy with detrital affect</title>
<p>Generally, Cr is present in the form of Cr (VI) as mobile chromate anion in oxygenated waters, while under anoxic conditions it gets reduced to Cr (III), which is very unstable and forms complex cations with humic and fulvic acids. It also gets adsorbed with Fe-Mn oxyhydroxides and transported to the sediments (Calvert and Pedersen, <xref ref-type="bibr" rid="B13">1993</xref>; Tribovillard et al., <xref ref-type="bibr" rid="B72">2006</xref>). Cr also gets transported to the sediments along with the detrital fraction due to its presence in chromite and ferromanganese minerals (Dill et al., <xref ref-type="bibr" rid="B21">1988</xref>; Francois, <xref ref-type="bibr" rid="B27">1988</xref>; Hild and Brumsack, <xref ref-type="bibr" rid="B31">1998</xref>). The average Cr concentration in the studied sediment core is &#x0007E;69 ppm, much higher than the average crustal value of 35 ppm (Taylor and McLennan, <xref ref-type="bibr" rid="B68">1995</xref>). Synchronous variation in vertical profiles of detrital proxies Ti and C/N along with Cr has been observed in this study (Figure <xref ref-type="fig" rid="F3">3</xref>). Consistent low values of Ti and Cr till 18 ka years BP with C/N &#x0003C;12 suggests reduced terrestrial contribution at the core location due to weakening of summer monsoon (Naidu and Malmgren, <xref ref-type="bibr" rid="B40">1996</xref>; Rashid et al., <xref ref-type="bibr" rid="B56">2007</xref>; Anand et al., <xref ref-type="bibr" rid="B7">2008</xref>). Gradual increase in Ti and Cr after 18 ka years BP till 8 ka years BP with C/N &#x02265;12 indicates enhanced land-driven clastic fraction to the region instigated by the summer monsoon intensification (Govil and Naidu, <xref ref-type="bibr" rid="B28">2011</xref>). The Cr concentrations in the studied sediment core is thus a function of changing detrital influx to the region rather than changing redox conditions in the water column and limits its application as redox proxy, but can be a potential proxy to decipher terrestrial influence.</p>
<p>Co has been used as potential tool to decipher paleoredox conditions at the sediment-water interface due to its complex formation with fluvic or humic acid under oxic seawaters (Achterberg et al., <xref ref-type="bibr" rid="B1">2003</xref>). In oxygen deficient waters it can get incorporated into the solid phase authigenic by sulfide formation as Fe sulfides (Algeo and Maynard, <xref ref-type="bibr" rid="B5">2004</xref>; Tribovillard et al., <xref ref-type="bibr" rid="B72">2006</xref>). Co is prone to be influenced by detrital clastic material. The average Co concentration throughout the sediment core is &#x0007E;11 ppm similar to the average crustal Co value of 10 ppm (Taylor and McLennan, <xref ref-type="bibr" rid="B68">1995</xref>). Near similar values of Co with crustal values suggests its detrital contribution, but marginal enrichment in Co/Ti during LGM could be indicative of being a reasonable proxy to decipher past redox conditions.</p>
</sec>
<sec>
<title>Redox proxy with low detrital affect</title>
<p>Under oxic conditions, vanadium occurs in the form of V(V) as vanadate species getting adsorbed onto Mn-Fe oxyhydroxide (Morford and Emerson, <xref ref-type="bibr" rid="B36">1999</xref>), whereas, Mo remains as unreactive dissolved molybdate species (<inline-formula><mml:math id="M4"><mml:msubsup><mml:mrow><mml:mtext>MoO</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>) (Emerson and Huested, <xref ref-type="bibr" rid="B25">1991</xref>; Calvert and Pedersen, <xref ref-type="bibr" rid="B13">1993</xref>; Tribovillard et al., <xref ref-type="bibr" rid="B72">2006</xref>; Pattan and Pearce, <xref ref-type="bibr" rid="B47">2009</xref>). Under oxygen deficient conditions, both V and Mo are removed from the water column and its enrichment in the sediment serves as potential tool to decipher reducing conditions at sediment-water interface (Calvert and Pedersen, <xref ref-type="bibr" rid="B13">1993</xref>; Tribovillard et al., <xref ref-type="bibr" rid="B72">2006</xref>; Pattan and Pearce, <xref ref-type="bibr" rid="B47">2009</xref>).</p>
<p>The average V and Mo concentrations in the present study, are &#x0007E;72 and &#x0007E;1.4 ppm respectively. The co-occurrence of high values for Mo, V, OC, Mo/Ti, and V/Ti observed during LGM suggests prevalence of anoxic conditions at the sediment-water interface. Synchronous decline in Mo, V, OC, Mo/Ti, and V/Ti during deglacial period indicates resumption of oxic conditions at the sediment-water interface (Figures <xref ref-type="fig" rid="F3">3</xref>, <xref ref-type="fig" rid="F5">5</xref>). Unlike V and V/Ti, a conspicuous enrichment in OC, Mo, and Mo/Ti has been observed during early Holocene between 11 and 8 ka years BP. This can be corroborated well with the high sedimentation rate of &#x0007E;13.5 cm.ka<sup>&#x02212;1</sup> during early Holocene. This underpins better preservation of organic matter as a function of high sedimentation rate, while enhanced Mo and Mo/Ti plausibly resulted due to the formation of Mo-S complexes (Tribovillard et al., <xref ref-type="bibr" rid="B73">2004</xref>).</p>
<p>In oxygenated waters, Mn is present as Mn (II) which is highly unstable and gets oxidized to insoluble Mn (IV) (Mn-oxyhydroxides) and is delivered to the sediments (Tribovillard et al., <xref ref-type="bibr" rid="B72">2006</xref>). Manganese thus plays a significant role in transferring trace metals by scavenging them from the water column to the ocean bottom. However, during anoxic conditions, at the sediment-water interface, the dissolution of oxides and hydroxides releases Mn (II) back to the waters (Rajendran et al., <xref ref-type="bibr" rid="B53">1992</xref>). Identical vertical distribution in V/Ti and Mn/Ti suggests adsorption of vanadate onto Fe- and Mn-oxyhydroxides (Calvert and Piper, <xref ref-type="bibr" rid="B15">1984</xref>). The co-occurrence of high values of Mo/Ti and V/Ti during LGM suggests anoxic conditions, which results in dissolution of oxides and hydroxides and releasing Mn (II) back to the waters (Rajendran et al., <xref ref-type="bibr" rid="B53">1992</xref>) leading to depletion of Mn concentration in the sediment. Contrarily, the simultaneous enrichment of V/Ti and Mo/Ti with Mn/Ti is observed along with the enhancement of CaCO<sub>3</sub> during LGM (Figure <xref ref-type="fig" rid="F4">4</xref>). Such conspicuous behavior of Mn can be attributed to trapping of Mn in authigenic Mn-carbonates during its export to the sediments (Pedersen and Price, <xref ref-type="bibr" rid="B49">1982</xref>; Morford et al., <xref ref-type="bibr" rid="B37">2001</xref>; Tribovillard et al., <xref ref-type="bibr" rid="B72">2006</xref>).</p>
<p>Similar to V/Ti and Mo/Ti, enhanced values of Ni/Ti during LGM indicate its role as a redox sensitive proxy. Generally, Ni acts as a micronutrient and occurs as soluble cation either as Ni<sup>2&#x0002B;</sup> in soluble nickel carbonate (NiCO<sub>3</sub>) or NiCl<sup>&#x0002B;</sup> in oxic environments (Calvert and Pedersen, <xref ref-type="bibr" rid="B13">1993</xref>; Whitfield, <xref ref-type="bibr" rid="B77">2001</xref>). The average Ni concentration (60 ppm) in the present study is higher than the average crustal abundance of 20 ppm (Taylor and McLennan, <xref ref-type="bibr" rid="B68">1995</xref>). Simultaneous enhancement in Ni/Ti and OC during LGM suggest scavenging of Ni by organic matter in the water column (Piper and Perkins, <xref ref-type="bibr" rid="B51">2004</xref>; Naimo et al., <xref ref-type="bibr" rid="B41">2005</xref>). During organic matter degradation under extreme reducing conditions (sulfate redution), Ni generally precipitates as NiS in sediments. Therefore, high Ni/Ti along with OC during LGM implies deposition of the sediments under anoxic conditions. During deglacial period (17.5&#x02013;10 ka years BP), synchronous decrease in Ni/Ti ratio and OC suggests oxic conditions in the sediment-water interface (Figure <xref ref-type="fig" rid="F5">5</xref>).</p>
<p>High OC and CaCO<sub>3</sub> values observed in the sediment core during LGM indicate enhanced productivity, whereas abrupt enhancement of OC during early Holocene (11&#x02013;8 ka years BP) can be attributed to better preservation with high sedimentation rate. Similarly, enhanced redox sensitive elements (Mo/Ti, V/Ti, Ni/Ti) along with high OC during LGM suggests anoxic conditions triggered by high bacterial degradation of organic matter at the sediment-water interface. Unlike CaCO<sub>3</sub> and redox sensitive elements, marginal enrichment in the OC is observed at &#x0007E;21 ka years BP which later declined, but CaCO<sub>3</sub> and redox sensitive elements showed consistently high values with declining pattern until 11 ka years BP. Moreover, the OC values are nearly similar at LGM and the early Holocene. Thus, during LGM, anoxic conditions persisted as indicated by redox sensitive elements, while no decipherable reducing conditions occurred during the early Holocene (11&#x02013;8 ka years BP). A similar observation in SE Arabian Sea suggests high productivity induced low oxygenated bottom water conditions during LGM (Rao et al., <xref ref-type="bibr" rid="B55">2010</xref>). In comparison to the present study, it has been reported that the sediments from the equatorial Arabian Sea (Pailler et al., <xref ref-type="bibr" rid="B46">2002</xref>) and SE Arabian Sea (Pattan and Pearce, <xref ref-type="bibr" rid="B47">2009</xref>) never witnessed complete anoxic bottom water conditions, instead a fluctuation between oxic and suboxic conditions has been observed during LGM. While, another study from the SE Arabian Sea suggests near-anoxic conditions probably resulting in enhanced OC preservation and removal of U from seawater during LGM (Sarkar et al., <xref ref-type="bibr" rid="B61">1993</xref>).</p>
<p>Therefore, it can be stated that anomalous high OC values and changing behavior of redox sensitive elements suggests that it is not only the high sedimentation rate or organic matter degradation which influenced the redox elements, but other processes too are responsible for instigating the oxygen deficient conditions at the sediment-water interface during LGM.</p>
</sec>
<sec>
<title>Evidence of anoxic bottom waters at LGM</title>
<p>The redox conditions at the sediment-water interface is mainly controlled by bottom water oxic conditions influenced by deep water circulation and increased oxygen demand for enhanced OC supply and its degradation (Pattan and Pearce, <xref ref-type="bibr" rid="B47">2009</xref>; Pattan et al., <xref ref-type="bibr" rid="B48">2013</xref>). Enhanced overhead productivity leads to greater organic matter export to the sediments. C/N ratios has been extensively used to decipher the provenance of organic matter, i.e., values of C/N &#x02264;12 and C/N &#x02265;12 suggests provenance of marine and terrestrial origin of OC respectively (Hedges and Parker, <xref ref-type="bibr" rid="B29">1976</xref>; Emerson and Hedges, <xref ref-type="bibr" rid="B26">1988</xref>; Meyers, <xref ref-type="bibr" rid="B35">1997</xref>; Bhushan et al., <xref ref-type="bibr" rid="B10">2001</xref>; Pattan et al., <xref ref-type="bibr" rid="B48">2013</xref>). The C/N ratio in the present study varies from 9 to 17 with an average of 12. The C/N ratio followed pattern similar to Ti with low values during LGM with gradual increasing trend during the early Holocene followed by marginal decrease till present (Figure <xref ref-type="fig" rid="F6">6</xref>). Low C/N (&#x0007E;10) and high OC (&#x0007E;5 wt%) during LGM suggests reduced contribution of terrestrial OC primarily derived from overhead productivity. Marine OC is more labile and prone to microbial activity leading to oxygen deficient conditions both in water column and sediment-water interface. In the present study, if the enhanced peak of OC is due to high overhead productivity, then similar pattern should have been displayed by the redox sensitive elements during &#x0007E;21 ka years BP. However, in the present scenario, the OC peak at &#x0007E;21 ka years BP clearly indicates better preservation of OC (Figure <xref ref-type="fig" rid="F6">6</xref>).</p>
<fig id="F6" position="float">
<label>Figure 6</label>
<caption><p>Comparative plot for detrital and redox proxies with OC suggesting preservation of OC during LGM and early Holocene Period.</p></caption>
<graphic xlink:href="feart-05-00084-g0006.tif"/>
</fig>
<p>Due to the geographical setup, the deep water in the Indian Ocean is ventilated solely from south (Piotrowski et al., <xref ref-type="bibr" rid="B50">2009</xref>). Previous studies on &#x003B4;<sup>13</sup>C and &#x003B4;<sup>18</sup>O isotopic composition of foraminifera suggested significant changes during the glacial-interglacial period in the chemical characteristics of surface and deep water masses (Duplessy, <xref ref-type="bibr" rid="B22">1982</xref>; Naqvi et al., <xref ref-type="bibr" rid="B43">1994</xref>; Schmiedl and Leuschner, <xref ref-type="bibr" rid="B62">2005</xref>; Ahmad et al., <xref ref-type="bibr" rid="B3">2008</xref>). NADW is the main source for deep water ventilation in the Northern Indian Ocean and marginal change in deep water circulation alters the bottom water oxygen conditions. Previous studies have suggested that during LGM, the export of deep water from north Atlantic was reduced, which further compensated increased formation of Southern Ocean deep water (Kallel et al., <xref ref-type="bibr" rid="B33">1988</xref>; Ahmad et al., <xref ref-type="bibr" rid="B3">2008</xref>) and allowed replacement of NADW with AABW penetrating further northward (Curry et al., <xref ref-type="bibr" rid="B18">1988</xref>; Curry and Oppo, <xref ref-type="bibr" rid="B17">2005</xref>).</p>
<p>The present study based on a sediment core raised from a water depth of 3,400 m demonstrates anoxic conditions during LGM in the equatorial Indian Ocean. Such anoxic conditions were established due to enhanced productivity with OC degradation and deep water circulation changes originating from weakly ventilated (poor in O<sub>2</sub> and rich CO<sub>2</sub>) Southern Ocean deep waters. This further augmented oxygen deficient conditions causing enhanced preservation of OC. High OC peak at &#x0007E;21 ka years BP can be attributed to post depositional preservation of organic matter at the sediment-water interface due to the bottom water anoxic conditions (Figure <xref ref-type="fig" rid="F6">6</xref>). The present observations of anoxic bottom water due to poor ventilation is further supported by Ahmad et al. (<xref ref-type="bibr" rid="B3">2008</xref>) and Piotrowski et al. (<xref ref-type="bibr" rid="B50">2009</xref>) from the equatorial Indian Ocean. They suggested weak deep-water ventilation in Northern Indian Ocean as a result of reduced proportion of NADW (poor in CO<sub>2</sub> and rich in O<sub>2</sub>) and increased proportion of AABW (rich in CO<sub>2</sub> and poor in O<sub>2</sub>) during LGM. During early Holocene (11&#x02013;8 ka years BP), enhanced OC with C/N &#x0003E;12 (&#x0007E;16) suggests terrestrial origin of organic carbon (Figure <xref ref-type="fig" rid="F6">6</xref>). The OC preservation during the Holocene period without any significant variation in redox sensitive elements is mainly due to high sedimentation rate with deposition under well ventilated bottom water conditions.</p>
</sec>
</sec>
<sec sec-type="conclusions" id="s6">
<title>Conclusions</title>
<p>The behavior of redox sensitive elements has been extensively used to decipher paleo redox conditions at the sediment-water interface. On the basis of investigation of redox sensitive elements and OC content in a sediment core from the equatorial Indian Ocean, the present study demonstrates prevalence of anoxic conditions during LGM. The anoxic condition in the water column at the sediment-water interface during &#x0007E;21 ka years BP is due to the degradation of organic matter exported from enhanced overhead productivity further instigated by poorly ventilated bottom water. This results in post depositional preservation of OC. The early Holocene period (11&#x02013;8 ka years BP) with increased OC has been attributed to high sedimentation rate supported by high overhead OC flux without any significant variation in the redox sensitive elements. The present study provides a valuable signature of poor bottom water ventilation at the equatorial Indian Ocean during LGM and its role in better OC preservation with concurrent occurrence of high surface productivity.</p>
</sec>
<sec id="s7">
<title>Author contributions</title>
<p>All the authors have significantly contributed to bring the manuscript in final form. RB collected the samples. KC conducted the experiments and measurements. RB and KC compiled the data, interpreted, and prepared the manuscript. AJ provided radiocarbon AMS dates and chronology estimation of the sediment core.</p>
<sec>
<title>Conflict of interest statement</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
</sec>
</body>
<back>
<ack><p>We are thankful for the support of Ministry of Earth Sciences, Govt. of India under GEOTRACES Project (MOES/36/OOIS. Siber07). We thank cruise participants for their help and support during sediment core collection. We also thank Captain and Crew members of Sagar Kanya and NCAOR for providing logistic support during the cruise. We thank Director, PRL for support.</p>
</ack>
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