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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">760216</article-id>
<article-id pub-id-type="doi">10.3389/feart.2021.760216</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>Color Reflectance of Coastal Sediments in the South Bohai Sea and its Implication to Orbital Forcing of East Asian Summer Monsoon</article-title>
<alt-title alt-title-type="left-running-head">Li et&#x20;al.</alt-title>
<alt-title alt-title-type="right-running-head">Orbital Monsoon Variability in Bohai</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Li</surname>
<given-names>Yibing</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Chen</surname>
<given-names>Yanping</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Jiang</surname>
<given-names>Xingyu</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Yi</surname>
<given-names>Liang</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/90070/overview"/>
</contrib>
</contrib-group>
<aff id="aff1">
<label>
<sup>1</sup>
</label>State Key Laboratory of Marine Geology, Tongji University, <addr-line>Shanghai</addr-line>, <country>China</country>
</aff>
<aff id="aff2">
<label>
<sup>2</sup>
</label>Second Institute of Oceanography, Ministry of Natural Resources, <addr-line>Hangzhou</addr-line>, <country>China</country>
</aff>
<aff id="aff3">
<label>
<sup>3</sup>
</label>Key Laboratory of Muddy Coastal Geo-Environment, Tianjin Centre, China Geological Survey, <addr-line>Tianjin</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/1414858/overview">Fangjian Xu</ext-link>, China University of Petroleum (Huadong), 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/846049/overview">Zhengguo Shi</ext-link>, Institute of Earth Environment (CAS), China</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1086717/overview">Haiwei Zhang</ext-link>, Xi&#x2019;an Jiaotong University, China</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Liang Yi, <email>yiliang@tongji.edu.cn</email>
</corresp>
<fn fn-type="other">
<p>This article was submitted to Marine Geoscience, a section of the journal Frontiers in Earth Science</p>
</fn>
</author-notes>
<pub-date pub-type="epub">
<day>12</day>
<month>10</month>
<year>2021</year>
</pub-date>
<pub-date pub-type="collection">
<year>2021</year>
</pub-date>
<volume>9</volume>
<elocation-id>760216</elocation-id>
<history>
<date date-type="received">
<day>17</day>
<month>08</month>
<year>2021</year>
</date>
<date date-type="accepted">
<day>28</day>
<month>09</month>
<year>2021</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2021 Li, Chen, Jiang and Yi.</copyright-statement>
<copyright-year>2021</copyright-year>
<copyright-holder>Li, Chen, Jiang and Yi</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&#x20;terms.</p>
</license>
</permissions>
<abstract>
<p>There are two distinct variabilities of the East Asian summer monsoon (EASM) on orbital timescales observed in different proxies, and the forcing mechanisms between them are hotly debated. One of the ways to reconcile the debate is to present a geological archive recording two cycles in dominance and somehow in equivalence. In this work, we retrieved an EASM record by studying color reflectance of coastal sediments in the south Bohai Sea, East Asia. The leading component of reflectance derivative spectra accounts for 58.9% variance in total and its loading spectrum can be well correlated to that of mineral assemblages of illite and goethite. For this monsoonal record, orbital variabilities in precession and eccentricity bands are highlighted. By comparing this monsoonal record to previously published proxies, it is speculated that the spectral difference in the sediments of the south Bohai Sea and between various proxies in the EASM domain may indicate an integrated forcing of solar insolation and ice-sheet evolution in the late Quaternary. Overall, the monsoonal record in the Bohai Sea offers an opportunity to fill the gap of the diverse periodicities between various proxies, which is critical to extending our understanding of the EASM on orbital timescales.</p>
</abstract>
<kwd-group>
<kwd>color reflectance</kwd>
<kwd>Bohai Sea</kwd>
<kwd>late Quaternary</kwd>
<kwd>East Asian summer monsoon</kwd>
<kwd>orbital variabilities</kwd>
</kwd-group>
<contract-sponsor id="cn001">Natural Science Foundation of Shanghai<named-content content-type="fundref-id">10.13039/100007219</named-content>
</contract-sponsor>
</article-meta>
</front>
<body>
<sec id="s1">
<title>Introduction</title>
<p>The Asian Monsoon plays a critical role in transporting large quantities of heat and moisture to the East Asia, the most populated region on the Earth (<xref ref-type="bibr" rid="B64">Zhang et&#x20;al., 2008</xref>; <xref ref-type="bibr" rid="B42">Tan et&#x20;al., 2021</xref>), and their evolution has been attracting a great amount of research attentions from geological records to numerical modeling (<xref ref-type="bibr" rid="B24">Jiang and Lang, 2010</xref>; <xref ref-type="bibr" rid="B37">Shi et&#x20;al., 2012</xref>; <xref ref-type="bibr" rid="B49">Wang et&#x20;al., 2014</xref>; <xref ref-type="bibr" rid="B67">An et&#x20;al., 2015</xref>; <xref ref-type="bibr" rid="B38">Shi et&#x20;al., 2019</xref>; <xref ref-type="bibr" rid="B11">Cheng et&#x20;al., 2021</xref>). These geological records include loess deposits (<xref ref-type="bibr" rid="B68">An et&#x20;al., 2001</xref>; <xref ref-type="bibr" rid="B18">Guo et&#x20;al., 2002</xref>; <xref ref-type="bibr" rid="B41">Sun et&#x20;al., 2019</xref>), speleothem records (<xref ref-type="bibr" rid="B52">Wang et&#x20;al., 2001</xref>; <xref ref-type="bibr" rid="B9">Cheng et&#x20;al., 2009</xref>; <xref ref-type="bibr" rid="B10">Cheng et&#x20;al., 2016</xref>), and marine and lacustrine sediments (<xref ref-type="bibr" rid="B44">Tian et&#x20;al., 2008</xref>; <xref ref-type="bibr" rid="B66">An et&#x20;al., 2011</xref>; <xref ref-type="bibr" rid="B12">Clemens et&#x20;al., 2018</xref>; <xref ref-type="bibr" rid="B58">Yi et&#x20;al., 2018</xref>; <xref ref-type="bibr" rid="B7">Chen et&#x20;al., 2020</xref>; <xref ref-type="bibr" rid="B54">Xu et&#x20;al., 2021</xref>). Because of the spectral difference between proxies, the variability and mechanism on orbital timescales are hotly debated, especially for the East Asian summer monsoon (EASM). The most commonly viewpoints can be summarized into two scenarios.</p>
<p>1) The monsoon is interpreted as an inter&#x2013;tropical convergence zone (ITCZ) substantially away from the equator (<xref ref-type="bibr" rid="B46">Wang, 1994</xref>; <xref ref-type="bibr" rid="B4">Chao and Chen, 2001</xref>), and the EASM variability is predominated by precessional cycles, i.e.,&#x20;19&#x2013;23&#xa0;kyr (<xref ref-type="bibr" rid="B51">Wang et&#x20;al., 2008</xref>; <xref ref-type="bibr" rid="B9">Cheng et&#x20;al., 2009</xref>; <xref ref-type="bibr" rid="B25">Jo et&#x20;al., 2014</xref>). In this scenario, the EASM is proposed to be directly controlled by solar insolation (<xref ref-type="bibr" rid="B26">Kutzbach, 1981</xref>; <xref ref-type="bibr" rid="B36">Ruddiman, 2006</xref>), mainly reported in Chinese cave deposits, such as the Hulu and Sanbao caves (<xref ref-type="fig" rid="F1">Figure&#x20;1</xref>). 2) The EASM variability is predominated by the eccentricity cycle, i.e.,&#x20;100&#xa0;kyr, which highlights the role of global ice volume in modulating the thermodynamic difference between the Asian continent and Pacific Ocean (<xref ref-type="bibr" rid="B1">An et&#x20;al., 1990</xref>). In this scenario, the EASM could be controlled by glacial&#x2013;interglacial alternations (<xref ref-type="bibr" rid="B15">Ding et&#x20;al., 1994</xref>; <xref ref-type="bibr" rid="B14">Ding et&#x20;al., 1995</xref>; <xref ref-type="bibr" rid="B48">Wang, 1999</xref>; <xref ref-type="bibr" rid="B18">Guo et&#x20;al., 2002</xref>; <xref ref-type="bibr" rid="B17">Guo et&#x20;al., 2004</xref>), such as profiles in the Chinese loess plateau and ODP 1148 site in the South China Sea (<xref ref-type="fig" rid="F1">Figure&#x20;1</xref>).</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Location, environmental system, and study site (Lz908) and reference sites mentioned in the text. KC, Kuroshio Current; YSWC, Yellow Sea warm current; EASM, East Asian summer monsoon. The base map data was generated using the open and free software DIVA-GIS 7.5 (<ext-link ext-link-type="uri" xlink:href="http://www.diva-gis.org/">http://www.diva-gis.org/</ext-link>).</p>
</caption>
<graphic xlink:href="feart-09-760216-g001.tif"/>
</fig>
<p>Besides of these two scenarios, the dominant obliquity band in the Chinese loess plateau and non&#x2013;precession component in the EASM variability in marine sediments at IODP U1429 site are also proposed (<xref ref-type="bibr" rid="B27">Li et&#x20;al., 2017</xref>; <xref ref-type="bibr" rid="B12">Clemens et&#x20;al., 2018</xref>), inferring a more complex response of the EASM to orbital forcing. To reconcile these hypotheses, <xref ref-type="bibr" rid="B8">Cheng et&#x20;al. (2021)</xref> suggested that different archives preferentially record a certain aspect of the EASM and spatial patterns of rainfall and wind across the precession cycle may be the major reason producing distinct regional divergences. However, testifying this new hypothesis is not easy, because the former requires a profile with a multiple dominance of eccentricity, obliquity, and precession cycles, or at least an equilibrium between them, while the later needs a full&#x2013;cover study in the monsoon domain.</p>
<p>The monsoonal record from the Bohai Sea (<xref ref-type="fig" rid="F1">Figure&#x20;1</xref>), East Asia may offer such an opportunity to fill the gap between the eccentricity&#x2013;and precession&#x2013;dominated monsoon variabilities (<xref ref-type="bibr" rid="B58">Yi et&#x20;al., 2018</xref>). In this study, an investigation was reported based on mineral properties of coastal sediments in core Lz908. A monsoon proxy of the late Quaternary was derived and three astronomical rhythms were observed. By comparing to other monsoon proxies across the East Asia, the different roles of monsoonal heat and moisture in pacing different records were discussed.</p>
</sec>
<sec sec-type="materials|methods" id="s2">
<title>Materials and Methods</title>
<sec id="s2-1">
<title>Core Lz908</title>
<p>The Bohai Sea is a semi&#x2013;enclosed interior continental shelf of the East China Sea (<xref ref-type="fig" rid="F1">Figure&#x20;1</xref>), with an average water depth of 18&#xa0;m, and it is connected to the Huanghai Sea by the narrow Bohai Strait. Core Lz908 is located onshore near the southern coast of the Bohai Sea (37&#xb0;09&#x2032;N, 118&#xb0;58&#x2032;E, elevation 6&#xa0;m). The core was drilled to a depth of 101.3&#xa0;m with an average recovery rate of 75% in the summer of 2007, by the First Institute of Oceanography, Ministry of Natural Resources of China. The drill site was submerged until the middle of the 20th century.</p>
<p>The upper 54.3&#xa0;m of the core contains marine and coastal sediments (<xref ref-type="fig" rid="F2">Figure&#x20;2</xref>), and has been chosen for paleoenvironmental studies (<xref ref-type="bibr" rid="B59">Yi et&#x20;al., 2012a</xref>; <xref ref-type="bibr" rid="B60">Yi et&#x20;al., 2012b</xref>). Integrated the radiocarbon and luminescence&#x2013;based age model, the geochronology of core Lz908 was established by synchronously tuning sediment grain&#x2013;size index to the July insolation at 65&#xb0;N (<xref ref-type="bibr" rid="B59">Yi et&#x20;al., 2012a</xref>), and the tuning bottom (260&#xa0;ka) has been well constrained by magnetostratigraphy (<xref ref-type="bibr" rid="B57">Yi et&#x20;al., 2015</xref>). Based on this age model (<xref ref-type="fig" rid="F2">Figure&#x20;2</xref>), the core was sampled in 10&#x2013;cm interval to investigate mineral properties of coastal sediments in the south Bohai&#x20;Sea.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>Profile with dating results and age model of core Lz908 (<xref ref-type="bibr" rid="B59">Yi et&#x20;al., 2012a</xref>), changes in sediment grain size (GS index), and color indices (L&#x2a;a&#x2a;b&#x2a;) in the CIELAB color space. L&#x2a;, lightness; a&#x2a;, redness (&#x2b;)/greenness (&#x2212;); b&#x2a;, yellowness (&#x2b;)/blueness (&#x2212;).</p>
</caption>
<graphic xlink:href="feart-09-760216-g002.tif"/>
</fig>
</sec>
<sec id="s2-2">
<title>Mineralogy by Diffuse Spectral Reflectance</title>
<p>The CIELAB color space, in which any sediment&#x2019;s color can be expressed by L&#x2a;a&#x2a;b&#x2a; values, can provide useful stratigraphic information (<xref ref-type="bibr" rid="B34">Ortiz, 2011</xref>; <xref ref-type="bibr" rid="B40">Sun et&#x20;al., 2011</xref>; <xref ref-type="bibr" rid="B56">Yi et&#x20;al., 2016</xref>). Measurements of diffuse spectral reflectance (DSR) were collected at 10&#x2013;cm resolution (373 samples in total) in the State Key Laboratory of Marine Geology, Tongji University of China. To reduce uncertainties of water losses, the samples of core Lz908 were dried, ground, and compacted before the measurement. The instrument is the Minolta CM&#x2013;700d spectrophotometer (400&#x2013;700&#xa0;nm wavelength range; 10&#xa0;nm resolution; 3&#xa0;mm spot size).</p>
<p>In order to reduce uncertainties of paleoenvironmental inference using original color data (L&#x2a;a&#x2a;b&#x2a;) in such a dynamic region (<xref ref-type="bibr" rid="B56">Yi et&#x20;al., 2016</xref>), we employ principle component analysis (PCA) to identify the contribution of different mineral assemblages to the downcore color variations. The PCA was calculated using the correlation matrix of the center&#x2013;weighted derivatives of the DSR data (<xref ref-type="bibr" rid="B35">Ortiz et&#x20;al., 2004</xref>; <xref ref-type="bibr" rid="B34">Ortiz, 2011</xref>) from core Lz908.</p>
</sec>
<sec id="s2-3">
<title>Mineralogy by X&#x2013;Ray Diffraction</title>
<p>As suggested in previous studies (<xref ref-type="bibr" rid="B34">Ortiz, 2011</xref>; <xref ref-type="bibr" rid="B40">Sun et&#x20;al., 2011</xref>; <xref ref-type="bibr" rid="B56">Yi et&#x20;al., 2016</xref>), the results of X&#x2013;Ray Diffraction (XRD) of the sediments can provide an independent check for the DSR&#x2013;based mineral identification. Thus, four representative samples from core Lz908 (15, 25, 35, and 45&#xa0;m in depth) were measured by the XRD, according to the methods described by <xref ref-type="bibr" rid="B29">Liu et&#x20;al. (2004)</xref> as follows.</p>
<p>The XRD clay mineral study was carried out on the &#x3c;2&#xa0;&#x3bc;m fraction, which was separated by conventional Stokes&#x2019; settling after the removal of carbonate and organic matter by acetic acid (15%) and hydrogen peroxide (10%), respectively. Clay minerals were then identified by using an X&#x2019;Pert PRO, PANalytical XRD instrument (40&#xa0;kV and 40&#xa0;mA) at the First Institute of Oceanography, Ministry of Natural Resources of China. Identification of clay minerals was made according to the position of the (001) series of basal reflections observed on the XRD diagrams (<xref ref-type="bibr" rid="B32">Moore and Reynolds, 1997</xref>).</p>
</sec>
</sec>
<sec sec-type="results" id="s3">
<title>Results</title>
<p>The blue&#x2013;yellow contrast (b&#x2a;) and the red&#x2013;green contrast (a&#x2a;) of the sediments of core Lz908 are closely correlated (r&#x20;&#x3d;&#x20;0.72, <italic>p</italic>&#x20;&#x3c; 0.01). The two indices vary between values of&#x20;&#x2212;0.24&#x2013;5.50 and 6.93&#x2013;34.02, respectively. Sediment brightness (L&#x2a;) oscillates between values of 51.37&#x2013;69.16, and its variability became larger below &#x223c;48.0&#xa0;m (<xref ref-type="fig" rid="F2">Figure&#x20;2</xref>). Changes in the color indices are somehow similar, and extracting the same pattern is a common way for paleoenvironmental inferences.</p>
<p>The PCA results show that the first leading DSR component (CF&#x2013;1) accounts for 58.9% of the variance in the correlation matrix of the reflectance derivative spectra. To identify the minerals or mineral assemblages associated with the CF&#x2013;1, we calculate the linear correlation between the CF&#x2013;1 and known minerals (<xref ref-type="fig" rid="F3">Figure&#x20;3A</xref>), which are available online from the USGS Digital Spectral Library. The CF&#x2013;1 can be correlated to a mixture of illite &#x2b; goethite (r &#x3d; 0.98, <italic>p</italic>&#x20;&#x3c; 0.01), similar to ones of core YDZ&#x2013;3 from the Huanghe River delta (<xref ref-type="bibr" rid="B56">Yi et&#x20;al., 2016</xref>), close to the study site. The first derivative spectrum for pure goethite has principal peaks at 535 and 435&#xa0;nm (<xref ref-type="bibr" rid="B13">Deaton and Balsam, 1991</xref>), also observed in <xref ref-type="fig" rid="F3">Figure&#x20;3A</xref> (590&#x2013;540 and 440&#xa0;nm). For the other two DSR components, which account for 28.6 and 5.5% variance in total, respectively, inherit the high&#x2013;frequency oscillation on suborbital and millennial timescales, and thus not discussed in this&#x20;study.</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>
<bold>(A)</bold> Varimax&#x2013;rotated factor loadings of core Lz908 and DSR first derivates of mineral standards (Illitite &#x2b; Goethite) plotted as a function of wavelength; <bold>(B)</bold> Four representative samples for XRD analysis with the identified minerals.</p>
</caption>
<graphic xlink:href="feart-09-760216-g003.tif"/>
</fig>
<p>As an independent check on the DSR analysis, additional results were obtained by XRD analysis from four representative sediment samples (<xref ref-type="fig" rid="F3">Figure&#x20;3B</xref>). The identified minerals are quartz (20.8&#x2013;29.0&#xa0;&#xc5;), mixed&#x2013;layer of illite&#x2013;quartz (26.5&#x2013;27.0&#xa0;&#xc5;), illite (8.8&#x2013;8.9&#xa0;&#xc5;, 17.6&#x2013;17.8&#xa0;&#xc5;), smectite (4.6&#x2013;4.9&#xa0;&#xc5;), chlorite (6.1&#x2013;6.3&#xa0;&#xc5;, 18.7&#x2013;18.9&#xa0;&#xc5;), and mixed&#x2013;layers of kaolinite&#x2013;chlorite (12.2&#x2013;12.5&#xa0;&#xc5;, 24.8&#x2013;25.3&#xa0;&#xc5;). The result of the XRD&#x2013;based clay mineral analysis supports the DSR results in this&#x20;study.</p>
<p>For the down&#x2013;core variation, the CF&#x2013;1 changed cyclically in the late Quaternary, and the most evident variation is the difference between glacial and interglacial intervals. For example, during the last and the penultimate glacial intervals, the illite &#x2b; goethite content was relatively high (<xref ref-type="fig" rid="F4">Figure&#x20;4A</xref>). The CF&#x2013;1 is also characterized in precession bands, and during each interval with high solar insolation, the illite &#x2b; goethite content was relatively low (<xref ref-type="fig" rid="F4">Figure&#x20;4B</xref>).</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>
<bold>(A)</bold> Changes in color (CF&#x2013;1) index of core Lz908 (thin line) with low&#x2013;frequent passed variabilities (bold line; FFT filter, &#x3c; 1/0.0125), <italic>versus</italic> Earth&#x2019;s orbital eccentricity (<xref ref-type="bibr" rid="B2">Berger and Loutre, 1991</xref>); <bold>(B)</bold> Changes in color index of core Lz908 (thin line) with precession&#x2013;band passed variabilities (bold line; FFT filter, 1/0.0255 &#x223c; 1/0.0235), <italic>versus</italic> changes in summer (July 21st) solar insolation at 65&#xb0;N (<xref ref-type="bibr" rid="B2">Berger and Loutre, 1991</xref>).</p>
</caption>
<graphic xlink:href="feart-09-760216-g004.tif"/>
</fig>
<p>Spectral analysis by the Blackman&#x2013;Tukey method (<xref ref-type="bibr" rid="B21">Howell et&#x20;al., 2006</xref>) confirms orbital variabilities (<xref ref-type="fig" rid="F5">Figure&#x20;5A</xref>). As shown, three astronomical rhythms are observed: the 100&#x2013;kyr periodicity is the major cycle in the CF&#x2013;1 record, the intensity of 41&#x2013;kyr periodicity is similar to the one of 23&#x2013;kyr periodicity, and the 19&#x2013;kyr cycle is much evident than other proxies of the EASM, such as marine and cave deposits (<xref ref-type="fig" rid="F5">Figures 5B,C</xref>). Moreover, the eccentricity band in the GS and the obliquity and precession bands in the CF&#x2013;1 are observed (<xref ref-type="fig" rid="F5">Figure&#x20;5</xref>), while for other proxies, either 100&#x2013;kyr or 23&#x2013;kyr dominated records, only one periodicity is highlighted (<xref ref-type="fig" rid="F5">Figure&#x20;5B</xref>), or evident (loess-based proxies) during interglacial intervals (e.g., <xref ref-type="bibr" rid="B31">Ma et&#x20;al., 2017</xref>; <xref ref-type="bibr" rid="B41">Sun et&#x20;al., 2019</xref>).</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>Spectral comparison following the Blackman&#x2013;Tukey method implemented with the ARAND software package (<xref ref-type="bibr" rid="B21">Howell et&#x20;al., 2006</xref>). MIS, deep&#x2013;sea sediment &#x3b4;<sup>18</sup>O records (<xref ref-type="bibr" rid="B28">Lisiecki and Raymo, 2005</xref>); MSLU, magnetic susceptibility record of the Luochuan profile (low frequency data) from the Chinese loess plateau (<xref ref-type="bibr" rid="B30">Lu and An, 1997</xref>); Color (CF&#x2013;1) and grain&#x2013;size (GS) indices of core Lz908; INS (solar insolation), July insolation at 65&#xb0;N (<xref ref-type="bibr" rid="B2">Berger and Loutre, 1991</xref>); CAVE, stalagmite &#x3b4;<sup>18</sup>O series (<xref ref-type="bibr" rid="B10">Cheng et&#x20;al., 2016</xref>).</p>
</caption>
<graphic xlink:href="feart-09-760216-g005.tif"/>
</fig>
<p>Further analyses of spectral curves by mathematical unmixing using a Gaussian equation provide a quantitative assessment for each astronomical rhythm (<xref ref-type="table" rid="T1">Table&#x20;1</xref>). The ratios of three astronomical rhythms are similar between the deep&#x2013;sea sediment &#x3b4;<sup>18</sup>O record (MIS) and the magnetic susceptibility record of the Yimaguan profile (frequency&#x2013;dependent data) from the Chinese loess plateau (MSHA), and between July insolation at 65&#xb0;N (INS) and the stalagmite &#x3b4;<sup>18</sup>O series (CAVE). However, for records derived from the Bohai Sea, the CF&#x2013;1 is highlighted in the eccentricity band (48%), followed by a close contribution of precession components (34%), and the GS is dominated in the precession band (66%), followed by an evident cycle of orbital eccentricity (23%).</p>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>Relative ratios of each orbital periodicity in various records.</p>
</caption>
<table>
<thead>
<tr>
<td align="left">Proxies</td>
<td align="center">Eccentricity (100&#xa0;kyr)</td>
<td align="center">Obliquity (41&#xa0;kyr)</td>
<td align="center">Precession (23 and 19&#xa0;kyr)</td>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">CF&#x2013;1 (Lz908)</td>
<td align="center">48%</td>
<td align="center">21</td>
<td align="center">21% &#x2b; 13%</td>
</tr>
<tr>
<td align="left">GS (Lz908)</td>
<td align="center">23%</td>
<td align="center">11</td>
<td align="center">58% &#x2b; 8%</td>
</tr>
<tr>
<td align="left">MIS</td>
<td align="center">59%</td>
<td align="center">27</td>
<td align="center">14%</td>
</tr>
<tr>
<td align="left">MSHA<xref ref-type="table-fn" rid="Tfn1">
<sup>a</sup>
</xref>
</td>
<td align="center">59%</td>
<td align="center">24</td>
<td align="center">17%</td>
</tr>
<tr>
<td align="left">INS</td>
<td align="center">&#x2014;</td>
<td align="center">19</td>
<td align="center">77% &#x2b; 5%</td>
</tr>
<tr>
<td align="left">CAVE</td>
<td align="center">5%</td>
<td align="center">11</td>
<td align="center">70% &#x2b; 14%</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn id="Tfn1">
<label>a</label>
<p>MSHA, magnetic susceptibility record of the Yimaguan profiles (frequency&#x2013;dependent data) from the Chinese loess plateau (<xref ref-type="bibr" rid="B20">Hao et&#x20;al., 2012</xref>). Other datasets are from <xref ref-type="fig" rid="F5">Figure&#x20;5</xref>.</p>
</fn>
</table-wrap-foot>
</table-wrap>
</sec>
<sec sec-type="discussion" id="s4">
<title>Discussion</title>
<sec id="s4-1">
<title>Monsoonal Proxies of Core Lz908</title>
<p>The sediment grain&#x2013;size record from the Bohai Sea, namely the GS record of core Lz908, can be used to indicate orbital changes of the EASM in the late Quaternary (<xref ref-type="bibr" rid="B59">Yi et&#x20;al., 2012a</xref>), because the sediment grain&#x2013;size variation is controlled by river discharge and resuspension process in the tidal zone (<xref ref-type="bibr" rid="B6">Chen et&#x20;al., 2013</xref>; <xref ref-type="bibr" rid="B39">Su et&#x20;al., 2016</xref>). Although the influence of regional sea&#x2013;level changes on the GS record of core Lz908 cannot be excluded (<xref ref-type="bibr" rid="B60">Yi et&#x20;al., 2012b</xref>), the EASM is the predominant factor controlling sedimentary dynamics in the south Bohai Sea, since &#x223c;80% of total variance of the GS record can be explained by solar insolation (<xref ref-type="bibr" rid="B58">Yi et&#x20;al., 2018</xref>).</p>
<p>For the CF&#x2013;1 record, mineral properties of coastal sediments in the south Bohai Sea are highlighted. Similar because these clay minerals were mainly from the Luzhong Mountains (<xref ref-type="fig" rid="F1">Figure&#x20;1</xref>), changes in the CF&#x2013;1 may be linked to weathering processes and river discharge, rather than regional sea&#x2013;level changes. For example, minerals illite and goethite in the Chinese loess plateau and the Huanghe River delta usually indicate a cold and dry climate in the past (e.g., <xref ref-type="bibr" rid="B23">Ji et&#x20;al., 2007</xref>; <xref ref-type="bibr" rid="B33">Niu et&#x20;al., 2015</xref>). In this study, the low&#x2013;frequency changes of the CF&#x2013;1 are in&#x2013;phase correlated with orbital eccentricity (<xref ref-type="fig" rid="F4">Figure&#x20;4</xref>), inferring that more illite and goethite were produced during glacial intervals in the Luzhong Mountains. Moreover, regional river inputs usually decrease to a much lower level in winters (<xref ref-type="bibr" rid="B56">Yi et&#x20;al., 2016</xref>), and most of detrital materials are transported to the south Bohai Sea in summers (<xref ref-type="bibr" rid="B59">Yi et&#x20;al., 2012a</xref>), <italic>via</italic> local rivers, such as the Mihe, Xiaoqinghe and Weihe Rivers. Since that the Asian monsoon is the major factor controlling clay minerals in the monsoon domain, such as in the Chinese loess plateau and the Huanghe River delta (e.g., <xref ref-type="bibr" rid="B40">Sun et&#x20;al., 2011</xref>; <xref ref-type="bibr" rid="B65">Zhao et&#x20;al., 2017</xref>; <xref ref-type="bibr" rid="B8">Chen et&#x20;al., 2021</xref>), the in&#x2013;phase relation between the CF&#x2013;1 and solar insolation is expected (<xref ref-type="fig" rid="F4">Figure&#x20;4</xref>). Thus, the CF&#x2013;1 can be linked to the EASM by mineralogical responses. When the EASM strengthens, a warmer and wetter climate would produce less minerals illite and goethite in the study area; but when the EASM weakens, the CF&#x2013;1 value increase, indicating more minerals illite and goethite in the sediments.</p>
<p>In summary, there are two monsoonal records derived from core Lz908, and the GS and the CF&#x2013;1 are linked to the EASM by sedimentary dynamics and mineral properties, respectively (<xref ref-type="fig" rid="F6">Figure&#x20;6</xref>). In specific, the GS record is correlated with the EASM in the late Quaternary by the processes of sedimentary dynamics and regional rainfall, dominated in precession bands (<xref ref-type="fig" rid="F5">Figure&#x20;5C</xref>). By regional weathering and river inputs, the CF&#x2013;1 record is linked to the EASM through both rainfall and temperature changes, highlighted in eccentricity and precession bands (<xref ref-type="fig" rid="F5">Figure&#x20;5A</xref>).</p>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>Comparisons between EASM proxies in the late Quaternary. <bold>(A)</bold> MIS record of deep&#x2013;sea sediment &#x3b4;<sup>18</sup>O (<xref ref-type="bibr" rid="B28">Lisiecki and Raymo, 2005</xref>); <bold>(B)</bold> MSLU, magnetic susceptibility record of the Luochuan profile (<xref ref-type="bibr" rid="B30">Lu and An, 1997</xref>); <bold>(C&#x2013;D)</bold> CF&#x2013;1 and GS records of core Lz908 (this study); <bold>(E)</bold> INS (solar insolation), July insolation at 65&#xb0;N (<xref ref-type="bibr" rid="B2">Berger and Loutre, 1991</xref>); <bold>(F)</bold> CAVE, stalagmite &#x3b4;<sup>18</sup>O series (<xref ref-type="bibr" rid="B10">Cheng et&#x20;al., 2016</xref>). The used datasets were from <xref ref-type="fig" rid="F5">Figure&#x20;5</xref>.</p>
</caption>
<graphic xlink:href="feart-09-760216-g006.tif"/>
</fig>
</sec>
<sec id="s4-2">
<title>An Integrated Forcing</title>
<p>Based on stalagmite records from Hulu, Dongge and Sanbao Caves of China, a clean and dominant precession cycle was observed (e.g., <xref ref-type="bibr" rid="B10">Cheng et&#x20;al., 2016</xref>). In these records, speleothem &#x3b4;<sup>18</sup>O changes can indicate &#x3b4;<sup>18</sup>O variation of local meteoric precipitation and thus characterize the EASM intensity (<xref ref-type="bibr" rid="B61">Yuan et&#x20;al., 2004</xref>; <xref ref-type="bibr" rid="B16">Dykoski et&#x20;al., 2005</xref>; <xref ref-type="bibr" rid="B10">Cheng et&#x20;al., 2016</xref>), which might be largely controlled by the large-scale monsoon circulation and concomitant latitudinal shifts of the monsoon rain belt (<xref ref-type="bibr" rid="B63">Zhang et&#x20;al., 2021</xref>). This relationship leads to the idea that the EASM can be directly driven by solar insolation (<xref ref-type="bibr" rid="B26">Kutzbach, 1981</xref>; <xref ref-type="bibr" rid="B63">Zhang et&#x20;al., 2021</xref>), explaining a high similarity in spectral characteristics between the EASM and solar insolation (<xref ref-type="bibr" rid="B24">Jiang and Lang, 2010</xref>; <xref ref-type="bibr" rid="B37">Shi et&#x20;al., 2012</xref>; <xref ref-type="bibr" rid="B38">Shi et&#x20;al., 2019</xref>). The linkage involves the shift of the ITCZ location (<xref ref-type="bibr" rid="B50">Wang et&#x20;al., 2005</xref>; <xref ref-type="bibr" rid="B9">Cheng et&#x20;al., 2009</xref>; <xref ref-type="bibr" rid="B25">Jo et&#x20;al., 2014</xref>), which modulates atmospheric circulations (<xref ref-type="bibr" rid="B3">Chao and Chen, 1999</xref>) and triggers the onset of Asian monsoon (<xref ref-type="bibr" rid="B5">Chao, 2000</xref>). Hence, although the physical significance of stalagmite &#x3b4;<sup>18</sup>O are still hotly debated (<xref ref-type="bibr" rid="B62">Zhang et&#x20;al., 2019</xref>), it is reasonable to speculate that monsoonal moisture is the major factor, since that tropical hydrological cycle varies mainly in precession bands (e.g., <xref ref-type="bibr" rid="B22">Huang et&#x20;al., 2020</xref>) and that summer rainfall can be well constrained by&#x20;stalagmite &#x3b4;<sup>18</sup>O in the Chinese loess plateau (e.g., <xref ref-type="bibr" rid="B43">Tan et&#x20;al., 2020</xref>).</p>
<p>Loess magnetic susceptibility as a proxy of the EASM is based on pedogenesis and mineral transformation (e.g., <xref ref-type="bibr" rid="B55">Yang et&#x20;al., 2015</xref>), <italic>via</italic> changing rainfall and temperature in the Chinese loess plateau between glacial and interglacial intervals. The monsoon circulation on glacial&#x2013;interglacial timescales was likely associated to the continental&#x2013;scale land&#x2013;sea thermal contrast (<xref ref-type="bibr" rid="B45">Wallace and Hobb, 1977</xref>; <xref ref-type="bibr" rid="B53">Webster et&#x20;al., 1998</xref>; <xref ref-type="bibr" rid="B47">Wang and Ding, 2008</xref>). Since not all of the rainfall could be used in pedogenesis and because of the loss of evaporation and surface runoff, changes in magnetic susceptibility may reflect effective precipitation (<xref ref-type="bibr" rid="B58">Yi et&#x20;al., 2018</xref>). Changes in global ice volume are proposed to modulate the thermodynamics of land&#x2013;sea contrast (<xref ref-type="bibr" rid="B1">An et&#x20;al., 1990</xref>), and it is reasonable to speculate that temperature changes were relatively important, considering that pedogenesis and chemical weathering in the Chinese loess plateau are likely not evident when winter temperature is below 0&#xb0;C (<xref ref-type="bibr" rid="B19">Hao and Guo, 2001</xref>). In addition, solar insolation could also modulate the sea-land thermal contrast and this influence was likely evident during interglacial intervals (e.g., <xref ref-type="bibr" rid="B31">Ma et&#x20;al., 2017</xref>).</p>
<p>For the GS record of core Lz908, regional rainfall is the dominant factor (<xref ref-type="bibr" rid="B59">Yi et&#x20;al., 2012a</xref>), while the influence of tropical cyclones (<xref ref-type="bibr" rid="B58">Yi et&#x20;al., 2018</xref>) and sea levels (<xref ref-type="bibr" rid="B60">Yi et&#x20;al., 2012b</xref>) can be excluded, and the former were likely paced by global temperature changes (e.g., <xref ref-type="bibr" rid="B69">Zhou et&#x20;al., 2019</xref>). Because of this, the GS record is dominated by precession cycles with a significant contribution in eccentricity and obliquity bands (<xref ref-type="table" rid="T1">Table&#x20;1</xref>). For the CF&#x2013;1, the intensified monsoon (rainfall) increases regional river discharge (<xref ref-type="bibr" rid="B8">Chen et&#x20;al., 2021</xref>), thus introducing precessional variabilities into the sediments. On the other hand, the intensified monsoon (temperature) may also strengthen regional pedogenesis in the Luzhong Mountains (<xref ref-type="fig" rid="F1">Figure&#x20;1</xref>), likely resulting in a transit of variabilities of eccentricity and obliquity into the sediments. Because of this, the CF&#x2013;1 record is dominated by eccentricity cycles with an equivalent component in precession bands (<xref ref-type="table" rid="T1">Table&#x20;1</xref>). Hence, monsoonal signals in the Bohai records may be not singly linked to temperature or rainfall changes like the loess&#x2013;and the speleothem&#x2013;based proxies, but demonstrate an integrated forcing of ice&#x2013;sheet evolution and solar insolation.</p>
<p>Overall, although the uncertainties in monsoonal proxies cannot be excluded in this study, the Bohai records likely fill the gap between the new hypothesis of <xref ref-type="bibr" rid="B11">Cheng et&#x20;al. (2021)</xref> and the diverse periodicities of monsoon proxies, supporting that different archives preferentially record a certain aspect of the EASM. Moreover, the difference between the two Bohai records responding to the EASM might highlight a distinct role of precession and eccentricity cycles, which are worth of further investigation in future.</p>
</sec>
</sec>
<sec sec-type="conclusion" id="s5">
<title>Conclusion</title>
<p>By analyzing DSR and XRD of the sediments in the Bohai Sea, mineral properties of core Lz908 in the late Quaternary were studied. Based on a principle component analysis, the leading component accounts for 58.9% variance in total and its loading spectrum can be well correlated to that of mineral assemblages of illite and goethite. A monsoonal record from the studied core was then derived, and orbital variabilities both in precession and eccentricity bands are evident. By comparing this mineral record to various monsoonal proxies, it is speculated that the precession variability in the EASM is mainly related to rainfall, while the eccentricity variability is likely associated with temperature changes. These findings demonstrate an integrated forcing of ice&#x2013;sheet evolution and solar insolation in the EASM in the late Quaternary. In summary, the Bohai records may fill the gap of the diverse periodicities between various monsoon proxies, supporting that different archives preferentially record a certain aspect of the&#x20;EASM.</p>
</sec>
</body>
<back>
<sec id="s6">
<title>Data Availability Statement</title>
<p>The raw data supporting the conclusion of this article will be made available by the authors, without undue reservation.</p>
</sec>
<sec id="s7">
<title>Author Contributions</title>
<p>Conceptualization, LY; formal analysis, YL, YC, and XJ; original draft preparation, YL; and review and editing, LY. All authors have read and agreed to the published version of the manuscript.</p>
</sec>
<sec id="s8">
<title>Funding</title>
<p>This research was funded by the Natural Science Foundation of Shanghai, grant number 19ZR1459800, the Global Changing and Air&#x2013;Sea Interaction, grant number GASI&#x2013;GEOGE&#x2013;04, and the National Natural Science Foundation of China, grant number 42177422.</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 Prof. YU Hongjun in the First Institute of Oceanography, Ministry of Natural Resources of China for providing samples for this&#x20;study.</p>
</ack>
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