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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="publisher-id">882201</article-id>
<article-id pub-id-type="doi">10.3389/feart.2022.882201</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>Sedimentary Rock Magnetic Response to Holocene Environmental Instability in the Pearl River Delta</article-title>
<alt-title alt-title-type="left-running-head">Wu et al.</alt-title>
<alt-title alt-title-type="right-running-head">Magnetic Variations in Holocene PRD</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Wu</surname>
<given-names>Yi</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1691774/overview"/>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Fu</surname>
<given-names>Shuqing</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Xiong</surname>
<given-names>Haixian</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Zong</surname>
<given-names>Yongqiang</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Ouyang</surname>
<given-names>Tingping</given-names>
</name>
<xref ref-type="aff" rid="aff7">
<sup>7</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Peng</surname>
<given-names>Shasha</given-names>
</name>
<xref ref-type="aff" rid="aff8">
<sup>8</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Cai</surname>
<given-names>Jianxin</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Han</surname>
<given-names>Yulin</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Zhu</surname>
<given-names>Zhaoyu</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
<xref ref-type="aff" rid="aff8">
<sup>8</sup>
</xref>
</contrib>
</contrib-group>
<aff id="aff1">
<sup>1</sup>
<institution>Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou)</institution>, <addr-line>Guangzhou</addr-line>, <country>China</country>
</aff>
<aff id="aff2">
<sup>2</sup>
<institution>Key Lab of Guangdong for Utilization of Remote Sensing and Geographical Information System</institution>, <institution>Guangdong Open Laboratory of Geospatial Information Technology and Application</institution>, <institution>Guangzhou Institute of Geography</institution>, <institution>Guangdong Academy of Sciences</institution>, <addr-line>Guangzhou</addr-line>, <country>China</country>
</aff>
<aff id="aff3">
<sup>3</sup>
<institution>Key Laboratory of Ocean and Marginal Sea Geology</institution>, <institution>South China Sea Institute of Oceanology</institution>, <institution>Innovation Academy of South China Sea Ecology and Environmental Engineering</institution>, <institution>Chinese Academy of Sciences</institution>, <addr-line>Guangzhou</addr-line>, <country>China</country>
</aff>
<aff id="aff4">
<sup>4</sup>
<institution>State Key Laboratory of Loess and Quaternary Geology</institution>, <institution>Institute of Earth Environment</institution>, <institution>Chinese Academy of Sciences</institution>, <addr-line>Xi&#x2019;an</addr-line>, <country>China</country>
</aff>
<aff id="aff5">
<sup>5</sup>
<institution>School of Marine Sciences</institution>, <institution>Sun Yat-sen University</institution>, <addr-line>Zhuhai</addr-line>, <country>China</country>
</aff>
<aff id="aff6">
<sup>6</sup>
<institution>Department of Earth Sciences</institution>, <institution>The University of Hong Kong</institution>, <addr-line>Hong Kong</addr-line>, <country>Hong Kong SAR, China</country>
</aff>
<aff id="aff7">
<sup>7</sup>
<institution>School of Geography</institution>, <institution>South China Normal University</institution>, <addr-line>Guangzhou</addr-line>, <country>China</country>
</aff>
<aff id="aff8">
<sup>8</sup>
<institution>State Key Laboratory of Isotope Geochemistry</institution>, <institution>CAS Center for Excellence in Deep Earth Science</institution>, <institution>Guangzhou Institute of Geochemistry</institution>, <institution>Chinese Academy of Sciences</institution>, <addr-line>Guangzhou</addr-line>, <country>China</country>
</aff>
<author-notes>
<fn fn-type="edited-by">
<p>
<bold>Edited by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1225839/overview">Xiting Liu</ext-link>, Ocean University of China, China</p>
</fn>
<fn fn-type="edited-by">
<p>
<bold>Reviewed by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/290046/overview">Weiguo Zhang</ext-link>, East China Normal University, China</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/923733/overview">Deming Kong</ext-link>, Guangdong Ocean University, China</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Yi Wu, <email>wuy@scsio.ac.cn</email>; Shuqing Fu, <email>fsq519@163.com</email>
</corresp>
<fn fn-type="other">
<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>20</day>
<month>06</month>
<year>2022</year>
</pub-date>
<pub-date pub-type="collection">
<year>2022</year>
</pub-date>
<volume>10</volume>
<elocation-id>882201</elocation-id>
<history>
<date date-type="received">
<day>23</day>
<month>02</month>
<year>2022</year>
</date>
<date date-type="accepted">
<day>10</day>
<month>05</month>
<year>2022</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2022 Wu, Fu, Xiong, Zong, Ouyang, Peng, Cai, Han and Zhu.</copyright-statement>
<copyright-year>2022</copyright-year>
<copyright-holder>Wu, Fu, Xiong, Zong, Ouyang, Peng, Cai, Han and Zhu</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) and the copyright owner(s) 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>Located on the northern coast of the South China Sea, the densely populated Pearl River Delta has experienced the combined effects of sea-level change, monsoon-driven discharge, and especially human activity, since the late Holocene. However, how these factors have regulated the regional environmental and sedimentary evolution remains unclear. To better understand these processes, we conducted a high-resolution rock magnetic investigation of the Holocene sediments of core DS01, drilled in the vicinity of the West River channel in the head area of the Pearl River deltaic plain. The magnetic grain-size proxy of the ARM/&#x3ba;<sub>lf</sub> ratio (the ratio of anhysteretic remanent magnetization to low-field magnetic susceptibility) indicates a long-term fining trend of the magnetite grain size, which may be a response to an increase in the weathering intensity in the Asian monsoon region during the Holocene. An interval with an enhanced concentration of magnetic minerals (mainly magnetite and hematite) occurred during 7.7&#x2013;4.8&#xa0;kyr&#xa0;BP (calendar years before 1950), coinciding with a period of delta progradation. During the marine transgression in the early Holocene, two similar intervals of magnetic enrichment may reflect regional hydrodynamic shifts associated with cooling events at &#x223c;9.5&#x2013;9.3&#xa0;kyr&#xa0;BP and 8.2&#xa0;kyr&#xa0;BP. The subsequent 4.2&#xa0;kyr&#xa0;BP cooling event possibly induced a cold and dry environment in the sediment source area. From &#x223c;800&#xa0;yr&#xa0;BP onward, there was a major increase in the sedimentary magnetic mineral content, likely in response to intensified agricultural and industrial activities.</p>
</abstract>
<kwd-group>
<kwd>environmental evolution</kwd>
<kwd>magnetic minerals</kwd>
<kwd>sea-level changes</kwd>
<kwd>cold events</kwd>
<kwd>human activity</kwd>
<kwd>Pearl River Delta</kwd>
</kwd-group>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>The formation of the sedimentary sequences of the Pearl River (Zhu Jiang) Delta in southern China likely began in the late Quaternary (e.g., <xref ref-type="bibr" rid="B16">Huang et al., 1982</xref>; <xref ref-type="bibr" rid="B50">Zhao, 1990</xref>). Developed on the northern coast of the South China Sea, in an area undergoing long-term tectonic subsidence, the regional sedimentary sequences of the deltaic plain have documented the complex history of marine transgression and regression (e.g., <xref ref-type="bibr" rid="B58">Zong et al., 2009</xref>; <xref ref-type="bibr" rid="B39">Wei and Wu, 2011</xref>; <xref ref-type="bibr" rid="B57">Zong et al., 2012</xref>; <xref ref-type="bibr" rid="B56">Zong et al., 2016</xref>; <xref ref-type="bibr" rid="B38">Wei X. et al., 2020</xref>). The modern Pearl River Delta is a densely populated and industrialized area, which is strongly influenced by the Asian summer monsoon (<xref ref-type="bibr" rid="B2">An, 2000</xref>; <xref ref-type="bibr" rid="B1">An et al., 2000</xref>). Determining the environmental and sedimentary evolution of the Pearl River Delta is a complex task, especially during the Holocene, when human activities became an increasingly important influence. Stalagmite records from China have provided detailed information on the paleoclimatic evolution of the Asian monsoon over the last 640&#xa0;kyr (<xref ref-type="bibr" rid="B7">Cheng et al., 2016</xref>). For the latest 10&#xa0;kyr, from the early Holocene onward, precisely dated proxy environmental records are available, such as the stalagmite records from southern China (<xref ref-type="bibr" rid="B47">Yuan et al., 2004</xref>; <xref ref-type="bibr" rid="B11">Dykoski et al., 2005</xref>; <xref ref-type="bibr" rid="B36">Wang et al., 2005</xref>). The &#x3b4;<sup>18</sup>O record from Dongge Cave suggests a weakening trend of Asian monsoon intensity for most of the Holocene, which was punctuated by pronounced short-term monsoon events that can be correlated regionally or globally (<xref ref-type="bibr" rid="B36">Wang et al., 2005</xref>).</p>
<p>An integrated analysis of a transect of sediment cores recovered from along both sides of the current channel of the West River (Xi Jiang), a tributary extending west&#x2013;east to the Pearl River catchment, has provided a Holocene record of the deltaic evolution of the head area of the Pearl River deltaic plain (<xref ref-type="fig" rid="F1">Figure 1</xref>) (<xref ref-type="bibr" rid="B43">Xiong et al., 2018</xref>; <xref ref-type="bibr" rid="B13">Fu et al., 2020</xref>). Within the area, lithostratigraphic units deposited above bedrock can be subdivided into three major groups: fluvial deposits, estuarine-deltaic deposits, and delta plain deposits, with decreasing depth. These sedimentary facies correspond to different sedimentary environments in the head area of the Pearl River Delta, and they provide an opportunity to obtain a relatively complete regional paleoenvironmental record throughout the Holocene.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Location map <bold>(A,B)</bold> and stratigraphic information <bold>(C)</bold> for sediment core DS01 (red circle) in the head area (dotted rectangle) of the Pearl River deltaic plain. Black circles mark the locations of sites discussed in the text: Dongge Cave (<xref ref-type="bibr" rid="B36">Wang et al., 2005</xref>), Dahu Swamp (<xref ref-type="bibr" rid="B54">Zhou et al., 2004</xref>), Huguangyan Maar Lake in south China (<xref ref-type="bibr" rid="B35">Wang et al., 2016</xref>), core HKUV11 (8.4&#xa0;m water depth, <xref ref-type="bibr" rid="B41">Wu et al., 2017</xref>), core MD05-2905 (1,647&#xa0;m water depth, <xref ref-type="bibr" rid="B53">Zhou et al., 2012</xref>) in the northern South China Sea, core NZ2 (4.6&#xa0;m water depth) in Lingdingyang Bay (Pearl River estuary, <xref ref-type="bibr" rid="B42">Wu et al., 2021</xref>), and core PD and core SX97 from the banks of the Pearl River estuary (<xref ref-type="bibr" rid="B45">Yang et al., 2008</xref>; <xref ref-type="bibr" rid="B27">Peng et al., 2014</xref>). The 10 radiocarbon dates for core DS01 shown in <bold>(C)</bold> are from <xref ref-type="bibr" rid="B13">Fu et al. (2020)</xref>. Details of the methods used to produce the age data are given in <xref ref-type="bibr" rid="B43">Xiong et al. (2018)</xref>. The maps were produced using Tencent Map App.</p>
</caption>
<graphic xlink:href="feart-10-882201-g001.tif"/>
</fig>
<p>In this study, we investigated a Holocene sedimentary sequence from the Pearl River Delta using rock magnetic measurements, which have been widely used for paleoenvironmental reconstruction (<xref ref-type="bibr" rid="B32">Thompson and Oldfield, 1986</xref>; <xref ref-type="bibr" rid="B12">Evans and Heller, 2003</xref>; <xref ref-type="bibr" rid="B21">Liu et al., 2012</xref>). Originating from the adjacent terrigenous areas of the Pearl River drainage, the detrital magnetic minerals in the sediments can potentially be used to decipher the paleoenvironmental history of the drainage area. Rock magnetic results have been reported for various drilling sites in the Pearl River estuary (e.g., <xref ref-type="bibr" rid="B45">Yang et al., 2008</xref>; <xref ref-type="bibr" rid="B27">Peng et al., 2014</xref>; <xref ref-type="bibr" rid="B42">Wu et al., 2021</xref>) (<xref ref-type="fig" rid="F1">Figures 1A,B</xref>). These studies have provided abundant information about the interplay of sea-level changes and sedimentary evolution in the coastal area since at least the late Pleistocene. In the present study, we measured multiple rock magnetic parameters, at high stratigraphic resolution, from a sediment core from the delta, with the aim of reconstructing millennial- to centennial-scale records of the Holocene sedimentary evolution of the head area of the Pearl River Delta. We compare the records with previous reconstructions of past regional climatic and environmental changes and attempt to understand how changes in climate, sea-level, and human impacts influenced the Holocene evolution of this coastal area.</p>
</sec>
<sec id="s2">
<title>2 Materials and Methods</title>
<p>We used sediment core DS01 (<xref ref-type="fig" rid="F1">Figure 1B</xref>; 23&#xb0;13.47&#x2032;N, 112&#xb0;44.43&#x2032;E; 25.61&#xa0;m in length), obtained from the north side of the West River. The altitude of the coring site was &#x223c;4.4&#xa0;m above the sea level. The base of the core consists of compact, reddish weathered bedrock. Above, the sediments can be divided into three lithological units, as illustrated in <xref ref-type="fig" rid="F1">Figure 1C</xref>. An age of 18,181&#x2013;17,865&#xa0;cal.&#xa0;yr Before Present (BP) was obtained for a sand layer (within Unit I) that unconformably covered the base rock. The three units are described as follows: Unit I: (25.61&#x2013;23.6&#xa0;m), sand and clayey silt with occasional plant residues. Unit II (23.6&#x2013;5.6&#xa0;m), mainly dark silt with occasional plant residues; soft. This unit comprises the main part of the core. Unit III: (5.6&#x2013;0&#xa0;m), mainly gray silt with occasional plant fragments; loose structure. <xref ref-type="bibr" rid="B13">Fu et al. (2020)</xref> identified four subunits that should comprise a complete Unit III within the vicinity of the head area of the Pearl River Delta (<xref ref-type="fig" rid="F1">Figure 1</xref>). However, in core DS01, two of these subunits are missing (sub-units IIIa and IIIb). Thus, we infer the existence of another sedimentary discontinuity between Unit II and Unit III.</p>
<p>Although not continuously represented in core DS01, the sedimentary succession in the study area was found to record a progressive transition from an estuarine to a deltaic environment, associated with the upper part of Unit II (<xref ref-type="fig" rid="F1">Figure 1C</xref>). In this study, samples were collected every 2&#xa0;cm by pressing plastic cubes (2 &#xd7; 2 &#xd7; 2&#xa0;cm<sup>3</sup>) into the center of the archive half of core DS01. The surface sediments (upper &#x223c;110&#xa0;cm) were not sampled to avoid sediments affected by recent agricultural and industrial activities. Another set of samples was collected at 10&#x2013;20&#xa0;cm intervals for analyses of grain size, organic carbon isotopes, and diatoms. These results were previously published (<xref ref-type="bibr" rid="B43">Xiong et al., 2018</xref>; <xref ref-type="bibr" rid="B13">Fu et al., 2020</xref>) and will be partially aiding the following discussions in our study.</p>
<p>Low-frequency (976&#xa0;Hz) and high-frequency (15,616&#xa0;Hz) volume magnetic susceptibilities (&#x3ba;<sub>lf</sub> and &#x3ba;<sub>hf</sub>, respectively) were measured on a total of 570 discrete cubic specimens (equivalent to a sampling resolution of 4.3&#xa0;cm), using an AGICO Kappabridge MFK1-FA magnetic susceptibility meter. The volume frequency-dependent susceptibility (&#x3ba;<sub>fd</sub>) was calculated as &#x3ba;<sub>fd</sub> &#x3d; &#x3ba;<sub>lf</sub>&#x2013;&#x3ba;<sub>hf</sub>. &#x3ba;<sub>lf</sub> generally reflects the concentration of paramagnetic and ferromagnetic components, and &#x3ba;<sub>fd</sub> is sensitive to the presence of superparamagnetic grains (<xref ref-type="bibr" rid="B32">Thompson and Oldfield, 1986</xref>; <xref ref-type="bibr" rid="B12">Evans and Heller, 2003</xref>; <xref ref-type="bibr" rid="B21">Liu et al., 2012</xref>).</p>
<p>Anhysteretic remanent magnetization (ARM) was imparted in a peak alternating field (AF) of 100&#xa0;mT with a direct current biasing field of 0.05&#xa0;mT superimposed, using a 2G AF demagnetizer. ARM was measured using a 2G three-axis cryogenic superconducting rock magnetometer (755R) installed in a shielded room with residual fields of &#x3c;300&#xa0;nT, in the Paleomagnetism Laboratory of the South China Sea Institute of Oceanology, Chinese Academy of Sciences. ARM is sensitive to stable single-domain ferrimagnetic grains (e.g., &#x223c;40&#xa0;nm for magnetite). We calculated the ARM/&#x3ba;<sub>lf</sub> ratio as a proxy for detecting relative changes in the grain size of magnetite (<xref ref-type="bibr" rid="B3">Banerjee et al., 1981</xref>; <xref ref-type="bibr" rid="B17">King et al., 1982</xref>).</p>
<p>Saturation isothermal remanent magnetization (SIRM) was imparted in a field of 1T using an ASC Impulse Magnetizer (IM-10-30) and measured using an AGICO JR-6A rock magnetometer. Back fields of 100&#xa0;mT (IRM<sub>-100&#xa0;mT</sub>) and 300&#xa0;mT (IRM<sub>-300&#xa0;mT</sub>) were then imparted and measured sequentially. Back IRMs were imparted to every third sample (<italic>n</italic> &#x3d; 190). The SIRM and backfield IRMs are used to calculate hard IRM (HIRM) and <italic>S</italic>-ratio (<xref ref-type="bibr" rid="B32">Thompson and Oldfield, 1986</xref>; <xref ref-type="bibr" rid="B12">Evans and Heller, 2003</xref>) as follows:<disp-formula id="equ1">
<mml:math id="m1">
<mml:mrow>
<mml:mtext>HIRM</mml:mtext>
<mml:mo>&#x3d;</mml:mo>
<mml:mtext>0</mml:mtext>
<mml:mtext>.</mml:mtext>
<mml:mn>5</mml:mn>
<mml:mtext>&#xd7;</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mtext>SIRM</mml:mtext>
<mml:mo>&#x2b;</mml:mo>
<mml:mtext>IRM</mml:mtext>
</mml:mrow>
<mml:mrow>
<mml:mo>-</mml:mo>
<mml:mn>300</mml:mn>
<mml:mtext>mT</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mtext>,</mml:mtext>
</mml:mrow>
</mml:math>
</disp-formula>
<disp-formula id="equ2">
<mml:math id="m2">
<mml:mrow>
<mml:mtext>S</mml:mtext>
<mml:mo>-</mml:mo>
<mml:mtext>ratio</mml:mtext>
<mml:mo>&#x3d;</mml:mo>
<mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mo>-</mml:mo>
<mml:mtext>IRM</mml:mtext>
</mml:mrow>
<mml:mrow>
<mml:mo>-</mml:mo>
<mml:mn>300</mml:mn>
<mml:mtext>mT</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>/</mml:mo>
<mml:mrow>
<mml:mtext>SIRM</mml:mtext>
</mml:mrow>
</mml:mrow>
<mml:mtext>.</mml:mtext>
</mml:mrow>
</mml:math>
</disp-formula>SIRM mainly reflects the combined concentrations of ferrimagnetic (e.g., magnetite) and imperfect antiferromagnetic particles (e.g., hematite and goethite), predominantly the former, unless the magnetic mineral assemblages are dominated by imperfect antiferromagnetic material. HIRM and <italic>S</italic>-ratio are widely used as proxies for the absolute and relative concentrations of imperfect antiferromagnetic particles, respectively. The ARM/SIRM ratio was calculated as an additional magnetic grain-size proxy, since it is unaffected by paramagnetic and superparamagnetic minerals.</p>
<p>In addition to the aforementioned routine magnetic measurements, selected samples were used for the following more detailed magnetic measurements. High-temperature magnetic susceptibility measurements (&#x3ba;<sub>lf</sub>-T) were made on freeze-dried powder samples in an argon environment, using the Kappabridge MFK1-FA combined with a CS-4 high-temperature furnace. IRM acquisition curves were measured in magnetic fields ranging from 1&#xa0;mT to 1.5&#xa0;T (in 90 logarithmically distributed steps), followed by backfield demagnetization in a range of magnetic fields up to 100&#xa0;mT. Hysteresis loops were obtained by cycling the magnetic field between &#xb1;1.0&#xa0;T, with a step size of 5&#xa0;mT. These measurements were made using a Lakeshore 8600 vibrating sample magnetometer (software version 1.3) at the Environmental Magnetism Laboratory of South China Normal University.</p>
</sec>
<sec id="s3">
<title>3 Results</title>
<sec id="s3-1">
<title>3.1 Magnetic Mineralogy</title>
<p>The thermomagnetic curves (&#x3ba;<sub>lf</sub>-T) of the five representative samples are largely consistent, showing a slight decrease in &#x3ba;<sub>lf</sub> from room temperature to &#x223c;300&#xb0;C during heating (see the lower panel in <xref ref-type="fig" rid="F2">Figure 2</xref>). This may be caused by the gradual unblocking of paramagnetic (or superparamagnetic) minerals, such as siderite and pyrite (<xref ref-type="bibr" rid="B10">Dunlop and &#xd6;zdemir, 2001</xref>; <xref ref-type="bibr" rid="B29">Roberts, 2015</xref>). Above &#x223c;300&#xb0;C, &#x3ba;<sub>lf</sub> begins to increase and a &#x201c;hump&#x201d; is evident between 400 and 550&#xb0;C. The cooling limb of the curve is not reversible because stoichiometric ferrimagnetic minerals have been produced during heating, possibly from the thermally induced alteration of paramagnetic iron-bearing silicates and/or clays (e.g., <xref ref-type="bibr" rid="B8">Deng et al., 2001</xref>; <xref ref-type="bibr" rid="B20">Liu et al., 2020</xref>). All the curves show a sharp decrease near 580&#xb0;C, the Curie temperature of magnetite, indicating that magnetite is likely the major magnetic carrier of the samples. The decreasing trend continues beyond 600&#xb0;C, revealing the presence of a magnetic phase with a Curie temperature greater than that of magnetite. A weak convex pattern appears at &#x223c;120&#xb0;C during each of the cooling runs, likely arising from the presence of a minor amount of goethite.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>Temperature-dependent magnetic susceptibility (&#x3ba;<sub>lf</sub>-T) curves for representative samples from core DS01. Arrows indicate heating (red) and cooling (blue) runs.</p>
</caption>
<graphic xlink:href="feart-10-882201-g002.tif"/>
</fig>
<p>
<xref ref-type="fig" rid="F3">Figure 3A</xref> shows that the IRMs at 300&#xa0;mT contribute &#x223c;73&#x2013;88% to the SIRM values, with <italic>S</italic>-ratios ranging from 11.5 to 95.3%, with a &#x223c;61% median for the whole core (<italic>n</italic> &#x3d; 192). The representative samples have a wide range of coercivities of remanence (&#x223c;35&#x2013;105&#xa0;mT) (<xref ref-type="fig" rid="F3">Figure 3B</xref>). We conclude that the dominant remanence carriers are low-coercivity ferrimagnetic minerals, but with high-coercivity phases being abundant.</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>IRM acquisition curves and backfield IRM curves <bold>(A</bold>,<bold>B)</bold> and hysteresis loops <bold>(C</bold>&#x2013;<bold>G)</bold> for representative samples from core DS01. Ms, saturation magnetization; Mrs, saturation remanence; Bc, coercivity; Bcr, coercivity of remanence. Hysteresis loop data of the samples shown in <bold>(C</bold>&#x2013;<bold>F)</bold> were processed using the HystLab program (<xref ref-type="bibr" rid="B26">Paterson et al., 2018</xref>).</p>
</caption>
<graphic xlink:href="feart-10-882201-g003.tif"/>
</fig>
<p>The hysteresis loops of the selected samples are slightly wasp-waisted (<xref ref-type="fig" rid="F3">Figures 3C&#x2013;G</xref>), which may result from the coexistence of two different magnetic components with contrasting coercivities (<xref ref-type="bibr" rid="B28">Roberts et al., 1995</xref>; <xref ref-type="bibr" rid="B31">Tauxe et al., 1996</xref>). Furthermore, the loops are almost closed when approaching 600&#xa0;mT, which also demonstrates the coexistence of both low- and high-coercivity magnetic components in the sediments.</p>
</sec>
<sec id="s3-2">
<title>3.2 Down-Core Variations in Magnetic Properties</title>
<p>Down-core plots of multiple magnetic parameters are presented in <xref ref-type="sec" rid="s11">Supplementary Figure S1</xref>. Using the pre-existing age data for the core (<xref ref-type="fig" rid="F1">Figure 1C</xref>), we built an age model based on linear interpolation or extrapolation (<xref ref-type="fig" rid="F4">Figure 4</xref>). However, this was not possible for Unit I (25.6&#x2013;23.6&#xa0;m) because the evaluated ages for the upper part would be much younger than those of the base of Unit II, assuming a constant sedimentation rate (&#x223c;16.5&#xa0;cm/kyr) estimated from the pre-existing age data. We infer that Unit I was rapidly deposited in a high-energy freshwater environment. Two age data are available for Unit III, and they indicate a high sedimentation rate (&#x223c;5&#xa0;m/kyr) within the interval of 1308&#x2013;420&#xa0;yr&#xa0;BP, resulting in a clear age discrepancy between Unit III and Unit II. This sedimentary hiatus may have been caused by river channel migration or later human activities (<xref ref-type="bibr" rid="B13">Fu et al., 2020</xref>). Six age data are available for Unit II, and therefore the chronology for this lithologic unit is of a relatively high resolution.</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>Comparison of magnetic records for core DS01 with selected independent paleoenvironmental records. <bold>(A</bold>&#x2013;<bold>C)</bold> ARM, ARM/&#x3ba;<sub>lf</sub>, and HIRM (this study); <bold>(D</bold>&#x2013;<bold>F)</bold> sand content, clay content, and carbon isotope ratios (&#x3b4;<sup>13</sup>C) from core DS01 (<xref ref-type="bibr" rid="B13">Fu et al., 2020</xref>); <bold>(G)</bold> elevations of ice-volume equivalent sea-level (<xref ref-type="bibr" rid="B19">Lambeck et al., 2014</xref>); <bold>(H)</bold> elevations from the mean sea level during 6&#x2013;10&#xa0;kyr&#xa0;BP, after correction for regional tectonic subsidence and sedimentary compaction [redrawn from <xref ref-type="bibr" rid="B43">Xiong et al. (2018)</xref>]; <bold>(I</bold>,<bold>J)</bold> sea surface temperature reconstructions from core HKUV11 (<xref ref-type="bibr" rid="B41">Wu et al., 2017</xref>) and core MD05-2905 (<xref ref-type="bibr" rid="B53">Zhou et al., 2012</xref>), respectively; <bold>(K)</bold> total organic matter (TOM) record from Huguangyan Maar Lake (<xref ref-type="bibr" rid="B35">Wang et al., 2016</xref>); and <bold>(L)</bold> the speleothem oxygen isotope record (&#x3b4;<sup>18</sup>O from Dongge Cave, an indicator of Asian summer monsoon intensity, ASM) (&#x223c;0&#x2013;9&#xa0;kyr&#xa0;BP, cyan curve (<xref ref-type="bibr" rid="B36">Wang et al., 2005</xref>); 0&#x2013;10&#xa0;kyr&#xa0;BP, gray curve (<xref ref-type="bibr" rid="B11">Dykoski et al., 2005</xref>). In <bold>(H)</bold>, red circles represent corrected elevations (without range) from drilling cores from the Pearl River Delta head area and estuarine area, while the (upper and lower) gray curves represent the 99% probability envelope of the reconstructed sea-level changes across the Pearl River Delta.</p>
</caption>
<graphic xlink:href="feart-10-882201-g004.tif"/>
</fig>
<p>Within Unit II, four horizons are highlighted due to the relatively high values of most of the magnetic parameters (<xref ref-type="sec" rid="s11">Supplementary Figure S1</xref>, <xref ref-type="table" rid="T1">Table 1</xref> and <xref ref-type="fig" rid="F4">Figure 4</xref>). Interval (a) (&#x223c;22.0&#x2013;23.6&#xa0;m, &#x223c;9.3&#x2013;9.5&#xa0;kyr&#xa0;BP) is a plateau-like zone of the magnetic parameters, at the base of Unit II, corresponding to the period when an estuarine environment began to dominate in the study area. In interval (b), around the middle of Unit II, a minor peak is evident in almost all the magnetic parameter profiles. However, intervals (a) and (b) do not have comparably high HIRM values, which indicates the dominant contribution of ferrimagnetic minerals (magnetite) in these intervals. Except for intervals (a) and (b), Unit II shows increasing but slightly different values of the magnetic parameters, including &#x3ba;<sub>lf</sub>, ARM, SIRM, HIRM, <italic>S</italic>-ratio, and ARM/&#x3ba;<sub>lf</sub> (<xref ref-type="sec" rid="s11">Supplementary Figures S1C,E&#x2013;J</xref>). Therefore, these trends did not develop simultaneously. Within interval (c), &#x3ba;<sub>lf</sub>, ARM, SIRM, HIRM, and <italic>S</italic>-ratio fluctuate within an interval of overall higher values. Interval (d), at the top of Unit II, is characterized by rapid changes in most of the magnetic parameters, with HIRM showing a significant peak, indicating a peak in the concentration of hard magnetic components (mainly hematite). In contrast, there are only minor peaks in &#x3ba;<sub>lf</sub>, ARM, and SIRM.</p>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>Ranges of variation of the magnetic parameters for core DS01 and intervals (a&#x2013;d).</p>
</caption>
<table>
<thead valign="top">
<tr>
<th rowspan="2" align="left"/>
<th colspan="2" align="center">Core DS01</th>
<th colspan="2" align="center">Interval a</th>
<th colspan="2" align="center">Interval b</th>
<th colspan="2" align="center">Interval c</th>
<th colspan="2" align="center">Interval d</th>
</tr>
<tr>
<th align="center">Mean</th>
<th align="center">Max/min</th>
<th align="center">Mean</th>
<th align="center">Max/min</th>
<th align="center">Mean</th>
<th align="center">Max/min</th>
<th align="center">Mean</th>
<th align="center">Max/min</th>
<th align="center">Mean</th>
<th align="center">Max/min</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">&#x3ba;<sub>lf</sub> (10<sup>&#x2212;6</sup>, SI)</td>
<td align="char" char=".">175.7</td>
<td align="char" char="(">452.2 (25.5)</td>
<td align="char" char=".">171.3</td>
<td align="char" char="(">290.0 (91.4)</td>
<td align="char" char=".">320.0</td>
<td align="char" char="(">379.3 (219.7)</td>
<td align="char" char=".">265.8</td>
<td align="char" char="(">452.2 (58.5)</td>
<td align="char" char=".">96.3</td>
<td align="char" char="(">126.6 (62.6)</td>
</tr>
<tr>
<td align="left">&#x3ba;<sub>fd</sub> (10<sup>&#x2212;6</sup>, SI)</td>
<td align="char" char=".">2.9</td>
<td align="char" char="(">28.6 (0.0)</td>
<td align="char" char=".">6.9</td>
<td align="char" char="(">19.1 (0.0)</td>
<td align="char" char=".">5.7</td>
<td align="char" char="(">12.1 (2.0)</td>
<td align="char" char=".">3.5</td>
<td align="char" char="(">8.1 (0.9)</td>
<td align="char" char=".">2.1</td>
<td align="char" char="(">8.1 (1.0)</td>
</tr>
<tr>
<td align="left">ARM (10<sup>&#x2212;2</sup>&#xa0;A/m)</td>
<td align="char" char=".">1.5</td>
<td align="char" char="(">13.4 (0.2)</td>
<td align="char" char=".">7.8</td>
<td align="char" char="(">13.4 (0.6)</td>
<td align="char" char=".">3.3</td>
<td align="char" char="(">5.3 (1.1)</td>
<td align="char" char=".">1.8</td>
<td align="char" char="(">3.0 (0.5)</td>
<td align="char" char=".">0.7</td>
<td align="char" char="(">3.0 (0.5)</td>
</tr>
<tr>
<td align="left">SIRM (A/m)</td>
<td align="char" char=".">1.1</td>
<td align="char" char="(">3.9 (0.0)</td>
<td align="char" char=".">1.1</td>
<td align="char" char="(">1.6 (0.6)</td>
<td align="char" char=".">1.9</td>
<td align="char" char="(">2.7 (0.7)</td>
<td align="char" char=".">2.3</td>
<td align="char" char="(">3.9 (0.5)</td>
<td align="char" char=".">0.7</td>
<td align="char" char="(">0.8 (0.5)</td>
</tr>
<tr>
<td align="left">HIRM (A/m)</td>
<td align="char" char=".">0.2</td>
<td align="char" char="(">0.4 (0.0)</td>
<td align="char" char=".">0.2</td>
<td align="char" char="(">0.2 (0.1)</td>
<td align="char" char=".">0.2</td>
<td align="char" char="(">0.3 (0.2)</td>
<td align="char" char=".">0.2</td>
<td align="char" char="(">0.4 (0.1)</td>
<td align="char" char=".">0.2</td>
<td align="char" char="(">0.2 (0.2)</td>
</tr>
<tr>
<td align="left">
<italic>S</italic>-ratio (%)</td>
<td align="char" char=".">59.8</td>
<td align="char" char="(">95.3 (11.5)</td>
<td align="char" char=".">68.0</td>
<td align="char" char="(">81.1 (16.8)</td>
<td align="char" char=".">71.2</td>
<td align="char" char="(">84.9 (47.3)</td>
<td align="char" char=".">77.7</td>
<td align="char" char="(">84.2 (50.3)</td>
<td align="char" char=".">42.6</td>
<td align="char" char="(">50.7 (36.3)</td>
</tr>
<tr>
<td align="left">ARM/&#x3ba;<sub>lf</sub> (A/m)</td>
<td align="char" char=".">91.4</td>
<td align="char" char="(">1042.4 (10.0)</td>
<td align="char" char=".">480.5</td>
<td align="char" char="(">1042.4 (53.8)</td>
<td align="char" char=".">98.5</td>
<td align="char" char="(">155.4 (48.1)</td>
<td align="char" char=".">68.5</td>
<td align="char" char="(">92.8 (46.8)</td>
<td align="char" char=".">71.0</td>
<td align="char" char="(">108.9 (52.9)</td>
</tr>
<tr>
<td align="left">ARM/SIRM (10<sup>&#x2212;2</sup>)</td>
<td align="char" char=".">1.6</td>
<td align="char" char="(">10.1 (0.7)</td>
<td align="char" char=".">6.2</td>
<td align="char" char="(">10.1 (0.9)</td>
<td align="char" char=".">1.3</td>
<td align="char" char="(">1.9 (0.9)</td>
<td align="char" char=".">0.8</td>
<td align="char" char="(">1.2 (0.7)</td>
<td align="char" char=".">1.0</td>
<td align="char" char="(">1.1 (1.0)</td>
</tr>
</tbody>
</table>
</table-wrap>
<p>There is a general upward-increasing trend in ARM/&#x3ba;<sub>lf</sub>, as shown in <xref ref-type="sec" rid="s11">Supplementary Figure S1I</xref>, suggesting the progressive fining of the magnetic grains (mainly magnetite). The ARM/SIRM ratio shows relatively uniform values throughout most of the core, with no comparable fluctuations in the interval of 11.3&#x2013;6.8&#xa0;m [interval (c)], but with an increase thereafter (<xref ref-type="sec" rid="s11">Supplementary Figure S1J</xref>).</p>
<p>Cross-plots showing the relationships between the magnetic parameters are shown in <xref ref-type="sec" rid="s11">Supplementary Figure S2</xref>. For &#x3ba;<sub>lf</sub>, &#x3ba;<sub>fd</sub>, ARM, and SIRM (<xref ref-type="sec" rid="s11">Supplementary Figures S2A&#x2013;C,F</xref>, respectively) linear relationships are evident for most of the data, indicating a general consistency of the sedimentary magnetic assemblages; deviations in these linear relationships generally correspond to high-amplitude fluctuations of the respective parameters within the profiles. &#x3ba;<sub>fd</sub> was not expected to be closely related with both ARM and SIRM (<xref ref-type="sec" rid="s11">Supplementary Figures S2D,E</xref>) as they are indicative of distinctive magnetic-domain states; however, the data points in both plots are generally clustered, as the magnetic minerals are seemingly concentrated within sedimentary intervals with a higher clay content (<xref ref-type="fig" rid="F4">Figure 4</xref>).</p>
</sec>
<sec id="s3-3">
<title>3.3 Hard Isothermal Remanent Magnetization and <italic>S</italic>-Ratio</title>
<p>The rock magnetic results show that magnetite and hematite are the dominant magnetic minerals in core DS01 and that the parameters related to magnetic mineral concentration (&#x3ba;<sub>lf</sub>, ARM, SIRM, HIRM, and <italic>S</italic>-ratio) show very similar stratigraphic patterns. The depositional context of the core location varied substantially since &#x223c;18&#xa0;kyr&#xa0;BP, and the material sources of the core sediments may have undergone substantial changes. This inference may undermine the use of HIRM and <italic>S</italic>-ratio, as they may be significantly affected by changes in magnetic mineral coercivity. Therefore, we used the <italic>L</italic>-ratio of <xref ref-type="bibr" rid="B22">Liu et al. (2007)</xref> to evaluate if these parameters were influenced by Al-substituted hematite or goethite, or both, since this would result in a wide range of coercivities which would invalidate their use. The <italic>L</italic>-ratio is calculated as follows:<disp-formula id="equ3">
<mml:math id="m3">
<mml:mrow>
<mml:mi>L</mml:mi>
<mml:mo>-</mml:mo>
<mml:mtext>ratio</mml:mtext>
<mml:mo>&#x3d;</mml:mo>
<mml:mrow>
<mml:mrow>
<mml:mtext>HIRM</mml:mtext>
</mml:mrow>
<mml:mo>/</mml:mo>
<mml:mrow>
<mml:mrow>
<mml:mo>[</mml:mo>
<mml:mrow>
<mml:mtext>0</mml:mtext>
<mml:mtext>.</mml:mtext>
<mml:mn>5</mml:mn>
<mml:mtext>&#xd7;</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mtext>SIRM</mml:mtext>
<mml:mo>&#x2b;</mml:mo>
<mml:mtext>IRM</mml:mtext>
</mml:mrow>
<mml:mrow>
<mml:mo>-</mml:mo>
<mml:mn>100</mml:mn>
<mml:mtext>mT</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>]</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:mrow>
<mml:mtext>.</mml:mtext>
</mml:mrow>
</mml:math>
</disp-formula>Reference to <xref ref-type="fig" rid="F5">Figure 5A</xref> shows a nearly constant distribution for most of the data points. The outliers are related to the specific sediment layers in <xref ref-type="fig" rid="F5">Figure 5B</xref> and <xref ref-type="fig" rid="F4">Figure 4</xref> and coincide with the transitional interval from Unit II to Unit III (<xref ref-type="sec" rid="s11">Supplementary Figure S1</xref>), during which the depositional environment was very unstable. The horizontally shaded intervals in <xref ref-type="fig" rid="F5">Figure 5B</xref> are characterized by magnetic minerals with substantially different coercivities, which may reflect different sources; hence, the use of HIRM and <italic>S</italic>-ratio may be inappropriate in these intervals. However, in the other intervals, both parameters can be used to quantify the absolute and relative concentrations of high-coercivity magnetic minerals (<xref ref-type="bibr" rid="B22">Liu et al., 2007</xref>; <xref ref-type="bibr" rid="B30">Roberts et al., 2020</xref>).</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>Relationship between <italic>L</italic>-ratio and HIRM, and down-core variations of <italic>S</italic>-ratio, HIRM, and <italic>L</italic>-ratio. Red dotted lines (in <bold>B</bold>) indicate three depths with low values in the <italic>L</italic>-ratio profile, referring to symbols plotted within the red-dotted ellipse (in <bold>A</bold>).</p>
</caption>
<graphic xlink:href="feart-10-882201-g005.tif"/>
</fig>
</sec>
</sec>
<sec id="s4">
<title>4 Discussion</title>
<p>The magnetic properties of sedimentary archives are often correlated with geological processes that control the provenance, transportation, deposition, and post-depositional modification (e.g., diagenesis) of sediments. The thermomagnetic analyses suggest a relatively uniform sedimentary magnetic mineral composition (<xref ref-type="fig" rid="F2">Figure 2</xref>), likely suggesting a consistent sediment source. This inference is supported by the generally consistent coercivities of the magnetic minerals indicated by the <italic>L</italic>-ratio (<xref ref-type="fig" rid="F5">Figure 5</xref>), as well as by the similar hysteresis loops of the representative samples (<xref ref-type="fig" rid="F3">Figures 3C&#x2013;G</xref>). However, there are significant fluctuations in magnetic mineral concentration and in magnetic grain size, as shown by the stratigraphic variations of &#x3ba;<sub>lf</sub>, ARM, SIRM, HIRM, and <italic>S</italic>-ratio and by the magnetic grain-size indicators, ARM/&#x3ba;<sub>lf</sub> and ARM/SIRM. We now focus on these fluctuations, especially on the intervals of enhanced magnetic concentration and their potential paleoenvironmental implications.</p>
<sec id="s4-1">
<title>4.1 Episodes of Magnetic Mineral Enrichment</title>
<p>Intervals (a&#x2013;d) in Unit II are dated to &#x223c;9.5&#x2013;9.3&#xa0;kyr&#xa0;BP, 8.5&#x2013;8.4&#xa0;kyr&#xa0;BP, 7.7&#x2013;4.8&#xa0;kyr&#xa0;BP, and 4.4&#x2013;4.2&#xa0;kyr&#xa0;BP, respectively, while the uppermost part of the core may provide a record of the last &#x223c;800&#xa0;yr (<xref ref-type="fig" rid="F4">Figure 4</xref>, <xref ref-type="table" rid="T1">Table 1</xref>). Intervals (a), (b), and (d) in core DS01 correspond to three short Bond-like cooling events (<xref ref-type="bibr" rid="B5">Bond et al., 1997</xref>; <xref ref-type="bibr" rid="B4">Bond et al., 2001</xref>) that are recorded in the stalagmite record from Dongge Cave, in southern China, in which more enriched &#x3b4;<sup>18</sup>O values represent intervals of a weakened monsoon (<xref ref-type="fig" rid="F4">Figure 4L</xref>). These rapid events may be dynamically linked to climate changes in the North Atlantic and Greenland (<xref ref-type="bibr" rid="B11">Dykoski et al., 2005</xref>; <xref ref-type="bibr" rid="B36">Wang et al., 2005</xref>). The linkage may be related to the strengthening of the Siberia High, which significantly affects the East Asian monsoon climate (<xref ref-type="bibr" rid="B6">Chen et al., 1991</xref>; <xref ref-type="bibr" rid="B9">Ding et al., 1995</xref>; <xref ref-type="bibr" rid="B23">Liu and Ding, 1998</xref>).</p>
<p>Intervals (a), (b), and (c) in core DS01 correspond to enhanced concentrations of both hard and soft magnetic components (<xref ref-type="fig" rid="F4">Figure 4</xref>, <xref ref-type="table" rid="T1">Table 1</xref>, and <xref ref-type="sec" rid="s11">Supplementary Figure S1</xref>). These intervals are related to quite different regional environments in terms of the degree of marine influence, representing the transition from an estuarine to a deltaic environment in the head area of the Pearl River Delta (<xref ref-type="fig" rid="F1">Figure 1</xref>). In contrast, interval (d), at the top of Unit II, is characterized by a higher concentration of imperfect antiferromagnetic minerals. Combined with the evaluation of the HIRM and <italic>S</italic>-ratio records (below), we infer that interval (d) represents a cold climatic event, similar to interval (b); however, the two intervals may be the product of different fluvial processes and depositional environments. The uppermost part of the core may predominantly reflect anthropogenic influences, rather than natural processes.</p>
<sec id="s4-1-1">
<title>4.1.1 Possible Brief Climatic Events at 9.5&#x2013;9.3, 8.5&#x2013;8.4, and 4.4&#x2013;4.2 Thousand Years Before Present</title>
<p>During the early Holocene, the entire Pearl River Delta likely experienced a rapid sea-level rise (<xref ref-type="fig" rid="F4">Figure 4H</xref>). <xref ref-type="bibr" rid="B43">Xiong et al. (2018)</xref> found that the rates of sea-level rise around the southeast coast of China doubled from 10.5 to 9.5&#xa0;kyr&#xa0;BP, increasing from 16 to 33&#xa0;mm/yr. Global sea-level changes, reconstructed from fluctuations in global ice volume, show a near-uniform rise during &#x223c;11.4&#x2013;8.4&#xa0;kyr&#xa0;BP (<xref ref-type="fig" rid="F4">Figure 4G</xref>, <xref ref-type="bibr" rid="B19">Lambeck et al., 2014</xref>). Core DS01 contains a prominent peak in the concentration of magnetic minerals after 9.5&#xa0;kyr&#xa0;BP. At this time, the head area of the Pearl River Delta may have become an intertidal environment, corresponding to the lower part of Unit II (<xref ref-type="fig" rid="F1">Figures 1B,C</xref>). Therefore, the site location of core DS01 would have been strongly influenced by the marine transgression at &#x223c;9.5&#xa0;kyr&#xa0;BP. Subsequently, rapid sediment accumulation occurred at the core site, including fine-grained sediments. Interval (a) is well-defined in most of the magnetic profiles (<xref ref-type="sec" rid="s11">Supplementary Figure S1</xref>) and has a comparable level of magnetic enhancement to interval (b). In both zones, there is a pronounced increase in the clay content and a corresponding low sand content (<xref ref-type="fig" rid="F4">Figures 4D,E</xref>). Evidently, these fine-grained sediments had higher concentrations of magnetic minerals than the coarse fraction. Thus, the magnetic properties and bulk sediment grain size suggest that these two intervals represent an abrupt shift in hydrodynamic forces that may have been associated with changes in precipitation and runoff in the river catchment during a period of weakened summer monsoon intensity.</p>
<p>Within the limits of the age model, intervals (b) (8.5&#x2013;8.4&#xa0;kyr&#xa0;BP) and (d) (4.4&#x2013;4.2&#xa0;kyr&#xa0;BP) are potentially correlative with the Holocene cooling events on the centennial scale, at &#x223c;8.2 and 4.2&#xa0;kyr&#xa0;BP, respectively. The magnetic parameters (<xref ref-type="sec" rid="s11">Supplementary Figure S1</xref>), bulk sediment grain size, and carbon isotope ratios (<xref ref-type="fig" rid="F4">Figure 4</xref>) collectively display coherent variations corresponding to intervals (a) and (b). By contrast, interval (d) is characterized by an increase in HIRM, hence showing an increase in the hematite content. This may reflect a cold, dry climate and oxidizing conditions in the source area. In a deltaic environment with a limited marine influence, the core site was likely subjected to weak hydrodynamic sorting during this interval (<xref ref-type="fig" rid="F4">Figures 4D,F</xref>). Adjacent sediment core HKUV11 likely recorded a rapid cooling event at &#x223c;4.2&#xa0;kyr&#xa0;BP (<xref ref-type="fig" rid="F4">Figure 4I</xref>; <xref ref-type="bibr" rid="B41">Wu et al., 2017</xref>), while core MD05-2905 from the northern South China Sea recorded an abrupt temperature decrease at &#x223c;8.2&#xa0;kyr&#xa0;BP (<xref ref-type="fig" rid="F4">Figure 4J</xref>; <xref ref-type="bibr" rid="B53">Zhou et al., 2012</xref>). However, there is no corresponding cooling signal in the global sea-level record (<xref ref-type="fig" rid="F4">Figure 4G</xref>, <xref ref-type="bibr" rid="B19">Lambeck et al., 2014</xref>). In southernmost mainland China, the total organic matter content of the sediments of Huguangyan Maar Lake recorded cooling events at 8.2&#xa0;kyr&#xa0;BP and 9.2&#xa0;kyr&#xa0;BP (<xref ref-type="fig" rid="F4">Figure 4K</xref>). Several other short-term cold/dry events are also evident in proxy environmental records from Holocene lake sediments from the region, including the 4.2&#xa0;kyr&#xa0;BP cold event (<xref ref-type="bibr" rid="B35">Wang et al., 2016</xref>).</p>
</sec>
<sec id="s4-1-2">
<title>4.1.2 Environmental Changes During 7.7&#x2013;4.8 Thousand Years Before Present</title>
<p>The diatom-derived salinity record (<xref ref-type="sec" rid="s11">Supplementary Figure S1K</xref>) indicates that during the interval of 7.7&#x2013;4.8&#xa0;kyr&#xa0;BP, following the early&#x2013;middle Holocene marine transgression, the study site experienced delta progradation and the accumulation of terrestrial sediments (or a marine regression) (<xref ref-type="bibr" rid="B57">Zong et al., 2012</xref>; <xref ref-type="bibr" rid="B56">Zong et al., 2016</xref>; <xref ref-type="bibr" rid="B43">Xiong et al., 2018</xref>; <xref ref-type="bibr" rid="B13">Fu et al., 2020</xref>). Reconstructions of the Holocene sea-level history in the Pearl River Delta show that the sea level was approximately stable during the last 7&#xa0;kyr (<xref ref-type="bibr" rid="B57">Zong et al., 2012</xref>; <xref ref-type="bibr" rid="B43">Xiong et al., 2018</xref>). The diatom profile suggests that the head area of the Pearl River Delta experienced a reduced marine influence during this interval (<xref ref-type="sec" rid="s11">Supplementary Figure S1K</xref>), which may be associated with the initiation of widespread sedimentation in the Pearl River deltaic basin (<xref ref-type="fig" rid="F4">Figure 4</xref>). Sediments that were sourced from tropical and subtropical areas and had undergone intensive weathering were deposited in the basin area, leading to the overall sedimentary magnetic enhancement throughout this interval.</p>
</sec>
<sec id="s4-1-3">
<title>4.1.3 Environmental Changes Since &#x223c;800&#xa0;Years Before Present</title>
<p>Recent agricultural and industrial activities, such as cultivation, deforestation, and mining, may have accelerated the production of magnetic minerals in Earth surface sediments. Organic carbon isotope records (&#x3b4;<sup>13</sup>C) from at least two drilling cores (including core DS01) from the head area of the Pearl River Delta reveal a general enrichment trend in the uppermost sedimentary unit (<xref ref-type="bibr" rid="B13">Fu et al., 2020</xref>). Numerous previous studies have provided evidence of agricultural activity in the Pearl River Delta since at least 2.5&#x2013;2.2&#xa0;kyr&#xa0;BP (e.g., <xref ref-type="bibr" rid="B59">Zong et al., 2010</xref>; <xref ref-type="bibr" rid="B44">Yang et al., 2012</xref>; <xref ref-type="bibr" rid="B14">Hu et al., 2013</xref>). Although the uppermost part of the core was not sampled for magnetic measurements, there is a pronounced increase in the contents of hematite and fine-grained magnetite since &#x223c;800&#xa0;yr BP (<xref ref-type="fig" rid="F4">Figures 4A,C</xref>), which is approximately coeval with the mid-Southern Song Dynasty. This interval corresponds to the peak period of Medieval warmth, represented in terrestrial climatic reconstructions (<xref ref-type="bibr" rid="B24">Mann et al., 2008</xref>). These changes in the magnetic profiles of core DS01 may be the result of intensified human activities in the Pearl River catchment, rather than to the phase of deltaic development over the area. Based on speleothem records, <xref ref-type="bibr" rid="B49">Zhang et al. (2008)</xref> hypothesized a close linkage between changes in monsoonal climate and Chinese cultural phases. A rapid increase in human disturbance from &#x223c;900&#xa0;yr BP is evident in the As record from a sediment core from the south of Hainan Island (<xref ref-type="bibr" rid="B33">Wan et al., 2015</xref>). The provision of high-resolution chronologies for the late Quaternary sediments of the study area remains challenging (e.g., <xref ref-type="bibr" rid="B46">Yim, 1999</xref>); moreover, there may be uncertainties in correlating records of monsoon intensity and rainfall, as argued by <xref ref-type="bibr" rid="B48">Zhang et al. (2010)</xref>. Further research is needed to precisely determine the contribution of human activities to the properties of the recent sediments of the study area.</p>
</sec>
</sec>
<sec id="s4-2">
<title>4.2 Regional Environmental Changes in the Context of the Evolution of the East Asian Summer Monsoon</title>
<sec id="s4-2-1">
<title>4.2.1 Holocene Climatic Optimum</title>
<p>The period before interval (c) (&#x223c;7.7&#x2013;4.8&#xa0;kyr&#xa0;BP) corresponds to the early Holocene marine transgression and is regarded as the climatic optimum in East Asia. Early studies proposed quite different timings for the Holocene optimum (defined as the peak in monsoonal precipitation or effective moisture) across the domain of the East Asian summer monsoon: at &#x223c;3&#xa0;kyr&#xa0;BP in southern China and at &#x223c;9&#xa0;kyr&#xa0;BP in northern China (see <xref ref-type="bibr" rid="B1">An et al., 2000</xref> and references therein). <xref ref-type="bibr" rid="B55">Zhou et al. (2022)</xref> proposed a gradual northward expansion of the Holocene optimum in the East Asian monsoon region (from 24.25&#xb0;N to 48.74&#xb0;N), based on pollen-based precipitation reconstructions. A depleted early Holocene stalagmite &#x3b4;<sup>18</sup>O signal is evident at Dongge Cave (<xref ref-type="fig" rid="F4">Figure 4L</xref>), which likely indicates a wetter Asian summer monsoon climate, as the &#x3b4;<sup>18</sup>O record of Dongge Cave is anticorrelated with the Asian summer monsoon intensity (<xref ref-type="bibr" rid="B36">Wang et al., 2005</xref>). Records of pollen (<xref ref-type="bibr" rid="B54">Zhou et al., 2004</xref>) and bulk organic carbon isotope ratios (<xref ref-type="bibr" rid="B52">Zhong et al., 2010</xref>) from Dahu Swamp, to the north of the East River in the Pearl River drainage (<xref ref-type="fig" rid="F1">Figure 1</xref>), suggest a pronounced warm and wet period during the early Holocene (&#x223c;10&#x2013;6&#xa0;kyr&#xa0;BP), which may be related to a strengthened East Asian summer monsoon. <xref ref-type="bibr" rid="B40">Wei Z. et al. (2020)</xref> conducted sedimentary magnetic analyses at Dahu Swamp and proposed a rainfall maximum during the mid-Holocene (&#x223c;8&#x2013;4&#xa0;kyr&#xa0;BP). Although the magnetic record differs from other paleoenvironmental reconstructions from Dahu Swamp, the magnetic record is in phase with an equivalent record from Daping Swamp (26&#xb0;10.18&#x2032;N, 110&#xb0;08&#x2032;E), to the north-west of Dahu Swamp (<xref ref-type="bibr" rid="B51">Zhong et al., 2018</xref>). Both locations may be sensitive to local hydrological changes as they are in hydrologically closed lake basins (<xref ref-type="bibr" rid="B51">Zhong et al., 2018</xref>; <xref ref-type="bibr" rid="B40">Wei Z. et al., 2020</xref>). Huguangyan Maar Lake (<xref ref-type="fig" rid="F1">Figure 1</xref>) may record the earliest timing of the Holocene optimum, as indicated by an elevated total organic matter content during 11.5&#x2013;6.5&#xa0;kyr&#xa0;BP (<xref ref-type="bibr" rid="B35">Wang et al., 2016</xref>). A pollen record from the lake sediments indicated that during the early Holocene (11.6&#x2013;7.8&#xa0;kyr&#xa0;BP), the area was dominantly occupied by trees and shrubs, with tropical trees recording maximum percentages during &#x223c;9.5&#x2013;8.0&#xa0;kyr&#xa0;BP (<xref ref-type="bibr" rid="B34">Wang et al., 2007</xref>). Thus, there may be minor offsets in the timing of the climatic optimum between the reconstructions from Huguangyan Maar Lake and Dahu Swamp. However, it is possible to conclude that, at least in southeastern China, the Holocene climatic optimum was not significantly time-transgressive and that the Holocene optimum undoubtedly occurred during the early Holocene. In the vicinity of the site of core DS01, a rapid marine transgression occurred during this period, which was associated with relatively low and uniform magnetic mineral concentrations, except the interval (a) (<xref ref-type="fig" rid="F4">Figure 4</xref>).</p>
</sec>
<sec id="s4-2-2">
<title>4.2.2 Long-Term Trend of Environmental Evolution</title>
<p>Both magnetic grain-size parameters in core DS01 (<xref ref-type="sec" rid="s11">Supplementary Figures S1I,J</xref>) show no clear response to either marine transgression or regression, when compared, for example, with the salinity profile (<xref ref-type="sec" rid="s11">Supplementary Figure S1K</xref>). This is quite different from the records from core SX97 (<xref ref-type="bibr" rid="B27">Peng et al., 2014</xref>) or core PD (<xref ref-type="bibr" rid="B45">Yang et al., 2008</xref>), which recorded frequent oscillations during the late Quaternary or Holocene. The ARM/&#x3ba;<sub>lf</sub> ratio in core DS01 indicates the long-term fining of the magnetic grain size, except for the lower part of the core (below &#x223c;22&#xa0;m). Neither of the neighboring cores shows comparable trends in their magnetic records (<xref ref-type="bibr" rid="B45">Yang et al., 2008</xref>; <xref ref-type="bibr" rid="B27">Peng et al., 2014</xref>; <xref ref-type="bibr" rid="B42">Wu et al., 2021</xref>). Seaward of the Pearl River estuary, the magnetic grains within the surface sediments become increasingly fine, which likely resulted from the dissolution of superparamagnetic grains (<xref ref-type="bibr" rid="B25">Ouyang et al., 2017</xref>). An increasing distance from the source areas could also result in a fining of the magnetic grain size, as finer grains are likely to be transported longer distances than coarser grains (<xref ref-type="bibr" rid="B15">Huang et al., 2021</xref>). However, this is not applicable here, as indicated by the <italic>L</italic>-ratio (<xref ref-type="fig" rid="F5">Figure 5</xref>). It is unlikely that sea-level changes were responsible for the long-term fining trend of magnetic grains evident in core DS01, although there is a close relationship between sea-level changes and sedimentary magnetic grain-size variations in the South China Sea (see <xref ref-type="bibr" rid="B18">Kissel et al., 2020</xref> and references therein). Neither is there clear evidence for the effect of sea-level change on East Asian monsoon intensity (e.g., <xref ref-type="bibr" rid="B37">Wang et al., 2001</xref>). We tentatively attribute the magnetic grain-size trend to a slightly increasing weathering intensity in the material source areas. Within the East Asian monsoon domain, the monsoonal climate (as a source of heat and moisture) would be expected to be a major factor controlling erosion and weathering processes in the Pearl River catchment. In comparison, there was a long-term trend of decreasing monsoon precipitation in southern China since the early Holocene (<xref ref-type="fig" rid="F4">Figure 4L</xref>; <xref ref-type="bibr" rid="B11">Dykoski et al., 2005</xref>; <xref ref-type="bibr" rid="B36">Wang et al., 2005</xref>), which does not necessarily conflict with increased weathering during the same period because of the complex regional hydrothermal conditions. Additionally, sediment pore water may have affected the magnetic measurements. Since water is generally diamagnetic and the sedimentary water content generally decreases down-core, ARM/&#x3ba;<sub>lf</sub> could be biased accordingly. However, this influence is likely to be minor, as the pore-water content was relatively low.</p>
</sec>
</sec>
</sec>
<sec id="s5">
<title>5 Summary</title>
<p>We have obtained a high-resolution rock magnetic record for drilling core DS01 to reconstruct the Holocene environmental evolution of the Pearl River Delta. The results indicate a relatively uniform magnetic mineral assemblage. A sedimentary hiatus occurred during &#x223c;3.9&#x2013;1.3&#xa0;kyr&#xa0;BP. Enhanced magnetic mineral concentrations have occurred at the top of the core since &#x223c;800&#xa0;yr&#xa0;BP, which we attribute to the intensified anthropogenic impact. The ARM/&#x3ba;<sub>lf</sub> ratio indicates a long-term trend of decreasing magnetite grain size during the Holocene, which may be a response to intensified weathering in the East Asian monsoon region. However, we cannot exclude the influence of residual pore water on this trend. A prominent interval of increased magnetic mineral concentration occurred during &#x223c;7.7&#x2013;4.8&#xa0;kyr&#xa0;BP, associated with delta progradation (or marine regression) in the study area. Three abrupt shifts in magnetic properties occurred at &#x223c;9.5&#x2013;9.3, &#x223c;8.5&#x2013;8.4, and &#x223c;4.4&#x2013;4.2&#xa0;kyr&#xa0;BP, which are potentially correlated with Bond-like events. The two older events are coeval with the initiation of the Holocene optimum in southeastern China, while the youngest event occurred in the context of deltaic development and minimal direct marine influence. It should be noted that possible uncertainties in the age model of core DS01 hinder the definitive correlation of these events with records from elsewhere, and further investigations of the Holocene sedimentary sequences in the Pearl River Delta and adjacent regions of East Asian monsoon influence are needed.</p>
</sec>
</body>
<back>
<sec id="s6">
<title>Data Availability Statement</title>
<p>New data from this study are available from the Mendeley Data (<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.17632/wcdhtstwtc.1">http://dx.doi.org/10.17632/wcdhtstwtc.1</ext-link>).</p>
</sec>
<sec id="s7">
<title>Author Contributions</title>
<p>YW and SF conceived the study and collected sub-samples for measurements; HX conducted the core drilling; YZ initiated the study on the Pearl River Delta; YW, YH, and JC conducted environmental magnetic analyses; TO and SP performed the rock magnetic analyses; and YW wrote the manuscript with input from SF, HX, ZZ, and TO. All co-authors contributed to discussion and approved the submitted version.</p>
</sec>
<sec id="s8">
<title>Funding</title>
<p>This work was supported financially by grants from the Key Special Project for Introduced Talents Team of Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou) (No. GML2019ZD0204), the Guangdong Basic and Applied Basic Research Foundation (Nos. 2019A1515011488 and 2017A030311020), the Guangdong Academy of Sciences (Nos. 2016GDASRC-0209 and 2020GDASYL-20200401001), and the Open Foundation of State Key Laboratory of Loess and Quaternary Geology at the Institute of Earth Environment, CAS (No. SKLLQG1838).</p>
</sec>
<sec sec-type="COI-statement" id="s9">
<title>Conflict of Interest</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 sec-type="disclaimer" id="s10">
<title>Publisher&#x2019;s Note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors, and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p>
</sec>
<ack>
<p>We thank Qunshu Tang for helpful discussions during the preparation of the manuscript, Yuemin Lin and Mingkun Li for assistance with rock magnetic analyses performed at South China Normal University, and Jan Bloemendal for language polishing. We thank the Associate Editor (Xiting Liu) and the reviewers for constructive comments that helped to improve the article.</p>
</ack>
<sec id="s11">
<title>Supplementary Material</title>
<p>The Supplementary Material for this article can be found online at: <ext-link ext-link-type="uri" xlink:href="https://www.frontiersin.org/articles/10.3389/feart.2022.882201/full#supplementary-material">https://www.frontiersin.org/articles/10.3389/feart.2022.882201/full&#x23;supplementary-material</ext-link>
</p>
<supplementary-material xlink:href="DataSheet1.docx" id="SM1" mimetype="application/docx" xmlns:xlink="http://www.w3.org/1999/xlink"/>
</sec>
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