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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">870298</article-id>
<article-id pub-id-type="doi">10.3389/feart.2022.870298</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>The Early Miocene Provenance Shift of ODP Site 1177 and Implications for the Tectonic Evolution of the Shikoku Basin, Philippine Sea Plate</article-title>
<alt-title alt-title-type="left-running-head">Liu et al.</alt-title>
<alt-title alt-title-type="right-running-head">Provenance Shift of ODP Site 1177</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Liu</surname>
<given-names>Wei</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1666559/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Feng</surname>
<given-names>Wanyi</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Gai</surname>
<given-names>Congcong</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1671860/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Zhou</surname>
<given-names>Yang</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Zhong</surname>
<given-names>Yi</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1734936/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Cao</surname>
<given-names>Wei</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1663046/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Li</surname>
<given-names>Yuanjie</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Zhao</surname>
<given-names>Xixi</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Liu</surname>
<given-names>Qingsong</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/116639/overview"/>
</contrib>
</contrib-group>
<aff id="aff1">
<sup>1</sup>
<institution>School of Environment</institution>, <institution>Harbin Institute of Technology</institution>, <addr-line>Harbin</addr-line>, <country>China</country>
</aff>
<aff id="aff2">
<sup>2</sup>
<institution>Center for Marine Magnetism (CM<sup>2</sup>)</institution>, <institution>Department of Ocean Science and Engineering</institution>, <institution>Southern University of Science and Technology</institution>, <addr-line>Shenzhen</addr-line>, <country>China</country>
</aff>
<aff id="aff3">
<sup>3</sup>
<institution>Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou)</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/491492/overview">Monika Korte</ext-link>, GFZ German Research Centre for Geosciences, Germany</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/1263984/overview">Yongjian Yao</ext-link>, Guangzhou Marine Geological Survey, China</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1328239/overview">David Buchs</ext-link>, Cardiff University, United Kingdom</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Qingsong Liu, <email>qsliu@sustech.edu.cn</email>
</corresp>
<fn fn-type="other">
<p>This article was submitted to Geomagnetism and Paleomagnetism, a section of the journal Frontiers in Earth Science</p>
</fn>
</author-notes>
<pub-date pub-type="epub">
<day>24</day>
<month>05</month>
<year>2022</year>
</pub-date>
<pub-date pub-type="collection">
<year>2022</year>
</pub-date>
<volume>10</volume>
<elocation-id>870298</elocation-id>
<history>
<date date-type="received">
<day>06</day>
<month>02</month>
<year>2022</year>
</date>
<date date-type="accepted">
<day>04</day>
<month>05</month>
<year>2022</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2022 Liu, Feng, Gai, Zhou, Zhong, Cao, Li, Zhao and Liu.</copyright-statement>
<copyright-year>2022</copyright-year>
<copyright-holder>Liu, Feng, Gai, Zhou, Zhong, Cao, Li, Zhao and Liu</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>The Ocean Drilling Program Site 1177 recovered the oldest (&#x223c;23&#xa0;Ma) sedimentary records in the Shikoku Basin, northeastern part of the Philippine Sea Plate. Changes in sediment provenances bear important implications for the tectonic evolution of the Philippine Sea Plate, but existing data are still controversial for the early Miocene. By integrating Sr-Nd isotopes, rock-magnetic parameters, diffuse reflectance spectroscopy, and the previous data on the detrital zircons and clay minerals from Site 1177, we found that a significant provenance shift occurred at &#x223c;16.5&#xa0;Ma. The sediments of Site 1177 before &#x223c;16.5&#xa0;Ma were mainly sourced from the Pearl River and Izu-Bonin Arc, but changed to the Yangtze River and Izu-Bonin Arc sources after that. This provenance shift was strongly linked with the northward motion and clockwise rotation of the Shikoku Basin in the Miocene, which marked the final time of separation between the Shikoku Basin and the South China Sea.</p>
</abstract>
<kwd-group>
<kwd>ODP site 1177</kwd>
<kwd>provenance shift</kwd>
<kwd>philippine sea plate</kwd>
<kwd>tectonic</kwd>
<kwd>rock-magnetism</kwd>
</kwd-group>
</article-meta>
</front>
<body>
<sec id="s1">
<title>Introduction</title>
<p>The Philippine Sea Plate is uniquely located among the Eurasian, Pacific, and Indo-Australian plates, and is of great importance to fundamental plate tectonic theory and global tectonic evolution (<xref ref-type="bibr" rid="B12">Hall, 2002</xref>; <xref ref-type="bibr" rid="B39">Reagan et al., 2010</xref>; <xref ref-type="bibr" rid="B53">Wu et al., 2016</xref>; <xref ref-type="bibr" rid="B34">Maunder et al., 2020</xref>; <xref ref-type="bibr" rid="B47">Sibuet et al., 2021</xref>). The Philippine Sea Plate is not only a natural laboratory for the study of plate tectonics on aspects of initial subduction, arc rifting, and back-arc spreading (<xref ref-type="bibr" rid="B39">Reagan et al., 2010</xref>; <xref ref-type="bibr" rid="B1">Arculus et al., 2015</xref>; <xref ref-type="bibr" rid="B34">Maunder et al., 2020</xref>; <xref ref-type="bibr" rid="B3">Chen et al., 2021</xref>; <xref ref-type="bibr" rid="B26">Li et al., 2021</xref>) but is also significant for the tectonic reconstruction of the West Pacific and East Asia (<xref ref-type="bibr" rid="B12">Hall, 2002</xref>; <xref ref-type="bibr" rid="B59">Zahirovic et al., 2014</xref>; <xref ref-type="bibr" rid="B24">Lallemand, 2016</xref>; <xref ref-type="bibr" rid="B53">Wu et al., 2016</xref>; <xref ref-type="bibr" rid="B33">Ma et al., 2019</xref>; <xref ref-type="bibr" rid="B38">Quea&#xf1;o et al., 2020</xref>; <xref ref-type="bibr" rid="B29">Liu et al., 2021</xref>; <xref ref-type="bibr" rid="B47">Sibuet et al., 2021</xref>).</p>
<p>From west to east, the Philippine Sea Plate can be divided into the West Philippine Basin, Kyushu-Palau Ridge, Shikoku Basin, Parece Vela Basin, East Mariana Ridge, Mariana Trough (or Mariana Back-Arc Basin), and Izu-Bonin-Mariana Arc (<xref ref-type="fig" rid="F1">Figure 1</xref>). The seafloor spreading of the West Philippine Basin was thought to have started from 51&#xa0;Ma (<xref ref-type="bibr" rid="B19">Ishizuka et al., 2013</xref>), 55&#xa0;Ma (<xref ref-type="bibr" rid="B6">Deschamps and Lallemand, 2002</xref>), or 58&#xa0;Ma (<xref ref-type="bibr" rid="B15">Hilde and Lee, 1984</xref>) to 36&#x2013;34&#xa0;Ma (<xref ref-type="bibr" rid="B42">Sasaki et al., 2014</xref>) or 33&#x2013;30&#xa0;Ma (<xref ref-type="bibr" rid="B6">Deschamps and Lallemand, 2002</xref>). The Kyushu-Palau Ridge was a remnant arc, which was ever connected to Izu-Bonin-Mariana Arc before the back-arc spreading of the Shikoku Basin and Parece Vela Basin at 30&#x2013;15&#xa0;Ma (<xref ref-type="bibr" rid="B36">Okino et al., 1999</xref>; <xref ref-type="bibr" rid="B44">Sdrolias et al., 2004</xref>). The Mariana Trough was a back -arc basin, which has been spreading since &#x223c;7&#xa0;Ma (<xref ref-type="bibr" rid="B18">Hussong and Uyeda, 1982</xref>; <xref ref-type="bibr" rid="B56">Yamazaki et al., 2003</xref>).</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Schematic map showing the studying area. Sites mentioned in this study are indicated by the purple circles. SCS &#x3d; South China Sea, WPB &#x3d; West Philippine Basin, KPR &#x3d; Kyushu-Palau Ridge, SB &#x3d; Shikoku Basin, PVB &#x3d; Parece Vela Basin, EMR &#x3d; East Mariana Ridge, MT &#x3d; Mariana Trough, IBMA &#x3d; Izu-Bonin-Mariana Arc, ECS &#x3d; East China Sea.</p>
</caption>
<graphic xlink:href="feart-10-870298-g001.tif"/>
</fig>
<p>The Ocean Drilling Program (ODP) Site 1177 recovered cores from the early Miocene to Pliocene sedimentary succession, which was the oldest sedimentary record in the Shikoku Basin. Thus, the study of Site 1177 provenance can shed light on the Miocene tectonic evolution of the Shikoku Basin, even the Philippine Sea Plate. Previous studies have constructed the tectonic evolutionary models of the Philippine Sea Plate based on evidences from paleomagnetism (<xref ref-type="bibr" rid="B32">Louden, 1977</xref>; <xref ref-type="bibr" rid="B22">Kinoshita, 1980</xref>; <xref ref-type="bibr" rid="B21">Keating, 1981</xref>; <xref ref-type="bibr" rid="B20">Keating and Herrero, 1981</xref>; <xref ref-type="bibr" rid="B2">Bleil, 1982</xref>; <xref ref-type="bibr" rid="B13">Haston and Fuller, 1991</xref>; <xref ref-type="bibr" rid="B14">Haston et al., 1992</xref>; <xref ref-type="bibr" rid="B23">Koyama et al., 1992</xref>; <xref ref-type="bibr" rid="B10">Hall et al., 1995</xref>; <xref ref-type="bibr" rid="B37">Queano et al., 2007</xref>; <xref ref-type="bibr" rid="B57">Yamazaki et al., 2010</xref>, <xref ref-type="bibr" rid="B55">2021</xref>; <xref ref-type="bibr" rid="B40">Richter and Ali, 2015</xref>; <xref ref-type="bibr" rid="B29">Liu et al., 2021</xref>), submarine magnetic anomaly (<xref ref-type="bibr" rid="B36">Okino et al., 1999</xref>; <xref ref-type="bibr" rid="B44">Sdrolias et al., 2004</xref>), seismic tomography (<xref ref-type="bibr" rid="B59">Zahirovic et al., 2014</xref>; <xref ref-type="bibr" rid="B53">Wu et al., 2016</xref>; <xref ref-type="bibr" rid="B33">Ma et al., 2019</xref>; <xref ref-type="bibr" rid="B47">Sibuet et al., 2021</xref>) and sedimentary provenance (<xref ref-type="bibr" rid="B4">Clift et al., 2013</xref>; <xref ref-type="bibr" rid="B41">Saitoh et al., 2015</xref>), etc. Researchers agreed on the first-order evolution that the Philippine Sea Plate moved &#x223c;20&#xb0;northward from the equator to the present position and simultaneously rotated &#x223c;90&#xb0;clockwise since the Eocene (<xref ref-type="bibr" rid="B12">Hall, 2002</xref>; <xref ref-type="bibr" rid="B57">Yamazaki et al., 2010</xref>; <xref ref-type="bibr" rid="B59">Zahirovic et al., 2014</xref>; <xref ref-type="bibr" rid="B53">Wu et al., 2016</xref>; <xref ref-type="bibr" rid="B33">Ma et al., 2019</xref>; <xref ref-type="bibr" rid="B29">Liu et al., 2021</xref>). However, the details of the evolution of the Philippine Sea Plate are still needed to be clarified, especially for the Shikoku Basin.</p>
<p>The evolution of provenance can be used to constrain plate tectonics by examining different spatio-temporal relationships of the source to sink (<xref ref-type="bibr" rid="B4">Clift et al., 2013</xref>; <xref ref-type="bibr" rid="B41">Saitoh et al., 2015</xref>). Some work on early Miocene provenance analyses has been performed for sediments from Site 1177; however, there are still controversies. For example, based on the lithological similarity between Site 1177 and Site 296, <xref ref-type="bibr" rid="B46">Shipboard Scientific Party (2001)</xref> thought that the sedimentary materials of Site 1177 most likely originated from the Kyushu-Palau Ridge, and they also did not rule out the small possibility of sources from Japan. However, the results from <xref ref-type="bibr" rid="B46">Shipboard Scientific Party (2001)</xref> are preliminary, and the interpretations were tentative. In a post-cruise study, <xref ref-type="bibr" rid="B50">Underwood and Fergusson (2005)</xref> identified large amounts of smectite from Site 1177 mudstones in the early Miocene. Given that the Izu-Bonin Arc is mainly composed of basalt, which contributes greatly to the formation of smectite (<xref ref-type="bibr" rid="B7">Fagel et al., 2001</xref>), <xref ref-type="bibr" rid="B50">Underwood and Fergusson (2005)</xref> speculated that the early Miocene provenance might derive from the Izu-Bonin Arc. Recently, <xref ref-type="bibr" rid="B29">Liu et al. (2021)</xref> suggested that the silt turbidites from Site 1177 were sourced from the Pearl River on the basis of similar zircon age spectra between Site 1177 and Site X28 (<xref ref-type="fig" rid="F2">Figure 2C</xref>).</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>
<bold>(A)</bold> The stratigraphic column of ODP Site 1177. A, B, C, and D in Unit III represented four sand packets. mbsf &#x3d; meters below seafloor. <bold>(B)</bold> A larger version of Panel 2A between 675 and 831&#xa0;m. The red arrows indicate locations of 11 mudstone samples that Sr-Nd isotope experiments were conducted in this study. <bold>(C)</bold> The zircon age spectrum of turbidites from Site 1177. The blue arrows indicate locations of turbidites that zircon U-Pb dating experiments were performed in the previous study. The silt turbidites were sourced from the Pearl River at &#x223c;18.6&#xa0;Ma (<xref ref-type="bibr" rid="B29">Liu et al., 2021</xref>), and the Yangtze River zircons were found in the sand turbidites at &#x223c;15.4&#xa0;Ma (<xref ref-type="bibr" rid="B4">Clift et al., 2013</xref>).</p>
</caption>
<graphic xlink:href="feart-10-870298-g002.tif"/>
</fig>
<p>These differences in provenance interpretation arose from at least two aspects. On the one hand, the research materials are different. Mudstones (<xref ref-type="bibr" rid="B50">Underwood and Fergusson, 2005</xref>) and turbidites (<xref ref-type="bibr" rid="B29">Liu et al., 2021</xref>) in the sedimentary sequence experienced different sedimentary processes and, therefore, may have originated from different sources. On the other hand, the above-mentioned studies are generally based on a certain method but lack comprehensive analysis. Therefore, it is necessary to integrate multiple methods to re-evaluate provenance evolution.</p>
<p>The Nd isotope is resistant to the processes of weathering, denudation, transportation, and deposition, which could preserve reliable provenance information (<xref ref-type="bibr" rid="B9">Goldstein and Jacobsen, 1988</xref>; <xref ref-type="bibr" rid="B52">Wei et al., 2012</xref>). Generally, the plots of Sr-Nd isotopes are sensitive in tracking the different provenances (<xref ref-type="bibr" rid="B5">Clift et al., 2014</xref>). The magnetic minerals in the sediments can also be used to distinguish provenance according to the variations in the type, concentration, and grain size of magnetic minerals (<xref ref-type="bibr" rid="B27">Liu et al., 2012</xref>). Specifically, the <italic>L</italic>-ratio, proposed by <xref ref-type="bibr" rid="B28">Liu Q. et al. (2007)</xref>, is very sensitive to provenance changes. The larger the <italic>L</italic>-ratio, the &#x2018;harder&#x2019; (higher-coercivity) the magnetic minerals (<xref ref-type="bibr" rid="B28">Liu Q. et al., 2007</xref>). Diffuse reflectance spectroscopy (DRS) can be used to identify the properties and concentrations of goethite (Gt) and hematite (Hm) (<xref ref-type="bibr" rid="B43">Scheinost, 1998</xref>; <xref ref-type="bibr" rid="B16">Hu et al., 2016</xref>).</p>
<p>In this study, we integrated new Sr-Nd isotope, rock-magnetic parameter, and DRS data from mudstones from &#x223c;22&#xa0;Ma to &#x223c;14&#xa0;Ma, as well as published provenance data of detrital zircons and clay minerals, to conduct a comprehensive provenance analysis of Site 1177, which could reconcile the previous provenance disputes. Moreover, if the turbidites were derived from the Pearl River and Yangtze River at &#x223c;18.6&#xa0;Ma and &#x223c;15.4&#xa0;Ma, respectively, this would imply a provenance shift between 18.6&#xa0;Ma and 15.4&#xa0;Ma. When did the provenance shift occur? Was the provenance shift attributed to tectonic events in the Philippine Sea Plate? A comprehensive provenance study can answer the above questions and deepen the understanding of the provenance and tectonic evolution of the Shikoku Basin.</p>
</sec>
<sec sec-type="materials|methods" id="s2">
<title>Materials and Methods</title>
<sec id="s2-1">
<title>Materials</title>
<p>To study the deformation and related fluid flow processes of the accretionary prism in the Nankai Trough, Sites 1173&#x2013;1178 during ODP Leg 190 were drilled. Among these sites, Site 1177 (31&#xb0; 39&#x2032;N, 134&#xb0; 0&#x2032;E, 4,844&#xa0;m water depth) yields the oldest sedimentary rocks in the northern Sikoku Basin. It consists of a sedimentary record between 300&#xa0;m below seafloor (mbsf) and 831.08&#xa0;mbsf, and a basalt basement with a thickness of 1&#xa0;m (<xref ref-type="fig" rid="F2">Figure 2A</xref>). The sediments from Site 1177 are muds, silts, sands, and volcanic ashes, which gradually consolidated downward into sedimentary rocks. Site 1177 is divided into five units based on lithologic assemblages (<xref ref-type="bibr" rid="B46">Shipboard Scientific Party, 2001</xref>). Unit I is interpretated as upper Shikoku Basin hemipelagic facies, while Units II and III are described as lower Shikoku Basin hemipelagic facies and turbidite facies, respectively. Unit IV represents volcaniclastic-rich facies and Unit V is the basalt basement. In Units III and IV, the zircon age spectrum of turbidites was determined (<xref ref-type="bibr" rid="B4">Clift et al., 2013</xref>; <xref ref-type="bibr" rid="B29">Liu et al., 2021</xref>) (<xref ref-type="fig" rid="F2">Figure 2C</xref>). The results indicated that the Pearl River zircons were found in the silt turbidites at &#x223c; 18.6&#xa0;Ma and the Yangtze River zircons were found in the sand turbidites at &#x223c;15.4&#xa0;Ma. In this investigation, we aimed to analyze the provenance evolution of mudstones in Units III and IV from 821&#xa0;mbsf (&#x223c;22&#xa0;Ma) to 687&#xa0;mbsf (&#x223c;14&#xa0;Ma) (<xref ref-type="fig" rid="F2">Figure 2B</xref>). The age of each sample was determined by linear interpolation based on the magnetostratigraphic and biostratigraphic ages (<xref ref-type="bibr" rid="B46">Shipboard Scientific Party, 2001</xref>).</p>
</sec>
<sec id="s2-2">
<title>Methods</title>
<p>Together, 11 mudstone samples were selected to conduct Sr-Nd isotope analysis. The detailed analytical procedures were the same as those described by <xref ref-type="bibr" rid="B52">Wei et al. (2012)</xref>. In the pre-treatment, we firstly removed the biogenic carbonate with 2&#xa0;N HAc, and then the samples were centrifuged, dried and crushed into powders. Next the powders were heated to remove the organic materials at 700&#xb0;C, digested by an HNO<sub>3</sub>&#x2b;HF acid mixture, and dissolved in a 2&#xa0;N HCl solution. Finally, a MicroMass Isoprobe multi-collector&#x2013;inductively coupled plasma&#x2013;mass spectrometer (MC&#x2013;ICP&#x2013;MS) were used to determine the Sr-Nd isotope data.</p>
<p>The mass-specific magnetic susceptibility (<italic>&#x3c7;</italic>), anhysteretic remanent magnetization (ARM), isothermal remanent magnetization (IRM) and DRS of 38 mudstone samples were measured. The susceptibility was measured at dual frequencies of 976&#xa0;Hz (<italic>&#x3c7;</italic>
<sub>lf</sub>) and 15616&#xa0;Hz (<italic>&#x3c7;</italic>
<sub>hf</sub>). The frequency-dependent susceptibility is defined as <italic>&#x3c7;</italic>
<sub>fd</sub> &#x3d; <italic>&#x3c7;</italic>
<sub>lf</sub> &#x2212;<italic>&#x3c7;</italic>
<sub>hf</sub>. The ARM was induced in a peak alternating field of 100&#xa0;mT with a 50&#xa0;&#x3bc;T direct current field, which was normalized to ARM susceptibility (<italic>&#x3c7;</italic>
<sub>ARM</sub>). The IRM was firstly acquired by an ASC IM10-30 Impulse Magnetizer in a 1000&#xa0;mT direct current field, which was regarded as saturation IRM (SIRM). Then reverse fields of &#x2212;100&#xa0;mT and &#x2212;300&#xa0;mT were used for demagnetization, which corresponded to IRM&#x2212;<sub>100mT</sub> and IRM&#x2212;<sub>300mT</sub>, respectively. The (SIRM &#x2b; IRM&#x2212;<sub>300mT</sub>)/(SIRM &#x2b; IRM&#x2212;<sub>100 mT</sub>) was calculated to determine the <italic>L</italic>-ratio (<xref ref-type="bibr" rid="B28">Liu Q. et al., 2007</xref>).</p>
<p>DRS measurements were conducted by a Cary 5000 spectrophotometer with the same methods as used by <xref ref-type="bibr" rid="B16">Hu et al. (2016)</xref>. The second derivatives of the Kubelka-Munk functions were used to determine the band positions of Hm and Gt, which are &#x223c;535&#xa0;nm (P<sub>535&#xa0;nm</sub>) and &#x223c;425&#xa0;nm (P<sub>425&#xa0;nm</sub>), respectively. Because of Al substitution, the position of P<sub>535&#xa0;nm</sub> and P<sub>425&#xa0;nm</sub> might vary (<xref ref-type="bibr" rid="B16">Hu et al., 2016</xref>). We choose the locations nearest to 535 and 425&#xa0;nm to define P<sub>535&#xa0;nm</sub> and P<sub>425&#xa0;nm,</sub> respectively. The amplitudes of the hematite (I<sub>535&#xa0;nm</sub>) and goethite (I<sub>425&#xa0;nm</sub>) were used for the relative concentrations of hematite and goethite, respectively (<xref ref-type="bibr" rid="B43">Scheinost, 1998</xref>). The concentration ratio of Hm/Gt is obtained by: Hm/Gt &#x3d; I<sub>535&#xa0;nm</sub>/I<sub>425&#xa0;nm</sub>.</p>
</sec>
</sec>
<sec sec-type="results" id="s3">
<title>Results</title>
<p>The isotope, rock-magnetic parameter, and DRS results are shown in <xref ref-type="fig" rid="F3">Figures 3</xref>, <xref ref-type="fig" rid="F4">4</xref>. The &#x3b5;Nd values range from &#x2212;8.9 to &#x2212;3.4 (<xref ref-type="fig" rid="F3">Figure 3A</xref>). Before &#x223c;16.5&#xa0;Ma, the &#x3b5;Nd values are changeable and more positive, with an average &#x3b5;Nd value of &#x2212;6.3. After &#x223c;16.5&#xa0;Ma, the &#x3b5;Nd values are more stable and negative, with an average &#x3b5;Nd value of &#x2212;8.5. The plot of <sup>87</sup>Sr/<sup>86</sup>Sr and &#x3b5;Nd is shown in <xref ref-type="fig" rid="F4">Figure 4</xref>. The data distribution can be divided into two clusters. The pre-16.5&#xa0;Ma data are located in the middle part of the plot, while the post-16.5&#xa0;Ma data are clustered in a region that near the Yangtze River (<xref ref-type="fig" rid="F4">Figure 4</xref>).</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>The temporal variations of isotopic and rock-magnetic parameters between &#x223c;14&#xa0;Ma and &#x223c;22&#xa0;Ma: <bold>(A)</bold> &#x3b5;Nd, <bold>(B)</bold> <italic>L</italic>-ratio, <bold>(C)</bold> P<sub>425&#xa0;nm</sub>, <bold>(D)</bold> P<sub>535&#xa0;nm</sub>, <bold>(E)</bold> Hm/Gt of Site 1177, <bold>(F)</bold> Hm/Gt of Site 1148 (<xref ref-type="bibr" rid="B5">Clift et al., 2014</xref>), <bold>(G)</bold> <italic>&#x3c7;</italic>
<sub>lf</sub>, <bold>(H)</bold> <italic>&#x3c7;</italic>
<sub>hf</sub>, <bold>(I)</bold> <italic>&#x3c7;</italic>
<sub>fd</sub>, <bold>(J)</bold> <italic>&#x3c7;</italic>
<sub>ARM</sub>, <bold>(K)</bold> SIRM, <bold>(L)</bold> <italic>&#x3c7;</italic>
<sub>ARM</sub>/SIRM, <bold>(M)</bold> smectite, and <bold>(N)</bold> illite (<xref ref-type="bibr" rid="B48">Steurer and Underwood, 2003</xref>; <xref ref-type="bibr" rid="B50">Underwood and Fergusson, 2005</xref>). The northward motion of <bold>(O)</bold> the western PSP (<xref ref-type="bibr" rid="B37">Queano et al., 2007</xref>), <bold>(P)</bold> the southern PSP (<xref ref-type="bibr" rid="B10">Hall et al., 1995</xref>), <bold>(Q)</bold> the northeastern PSP (DSDP and ODP sites in the SB and IBA: sites 442, 782, 784, 786, 787, 792, 793, and 1177) (<xref ref-type="bibr" rid="B22">Kinoshita, 1980</xref>; <xref ref-type="bibr" rid="B13">Haston and Fuller, 1991</xref>; <xref ref-type="bibr" rid="B14">Haston et al., 1992</xref>; <xref ref-type="bibr" rid="B29">Liu et al., 2021</xref>), and <bold>(R)</bold> the clockwise rotation of the PSP (<xref ref-type="bibr" rid="B13">Haston and Fuller, 1991</xref>; <xref ref-type="bibr" rid="B37">Queano et al., 2007</xref>). The blue thick lines mark the sudden changes in geochemical, rock-magnetic, and spectral parameters, and tectonic movement of the PSP. The red lines in <bold>(O</bold>&#x2013;<bold>R)</bold> are used to visualize the tectonic movement trends. PSP &#x3d; Philippine Sea Plate, SB &#x3d; Shikoku Basin, IBA &#x3d; Izu-Bonin Arc.</p>
</caption>
<graphic xlink:href="feart-10-870298-g003.tif"/>
</fig>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>The plot of <sup>87</sup>Sr/<sup>86</sup>Sr and &#x3b5;Nd for sediments from ODP Site 1177. Data for sediments from the Pearl River (<xref ref-type="bibr" rid="B30">Liu Z. et al., 2007</xref>), the Yangtze River (<xref ref-type="bibr" rid="B58">Yang et al., 2007</xref>; <xref ref-type="bibr" rid="B35">Meng et al., 2008</xref>), and the IBA (<xref ref-type="bibr" rid="B49">Tollstrup et al., 2010</xref>) are also shown for comparison.</p>
</caption>
<graphic xlink:href="feart-10-870298-g004.tif"/>
</fig>
<p>In terms of the rock-magnetic parameters and DRS results, the <italic>L</italic>-ratio (<xref ref-type="fig" rid="F3">Figure 3B</xref>) and P<sub>425&#xa0;nm</sub> (<xref ref-type="fig" rid="F3">Figure 3C</xref>) could be divided into two parts. The <italic>L</italic>-ratios were overall greater than 0.13 before &#x223c;16.5&#xa0;Ma and lesser than 0.13 since &#x223c;16.5&#xa0;Ma, which indicates that the coercivity distribution of magnetic minerals changed at &#x223c;16.5&#xa0;Ma. P<sub>425&#xa0;nm</sub> and P<sub>535 nm</sub> are the characteristic band position of Gt and Hm, respectively. Variations in P<sub>425&#xa0;nm</sub> (P<sub>535&#xa0;nm</sub>) values can be caused by different degrees of Al substitution (<xref ref-type="bibr" rid="B16">Hu et al., 2016</xref>). P<sub>425&#xa0;nm</sub> was relatively stable and was approximately 413&#xa0;nm before &#x223c;16.5&#xa0;Ma, and P<sub>425&#xa0;nm</sub> was variable and was larger than 413&#xa0;nm after &#x223c;16.5&#xa0;Ma. The temporal variations of P<sub>425&#xa0;nm</sub> indicate the different properties of Gt around &#x223c;16.5&#xa0;Ma. The P<sub>535&#xa0;nm</sub> values were generally centered at 545&#xa0;nm, except for a few points, and did not show an obvious first order shift trend before and after &#x223c;16.5&#xa0;Ma (<xref ref-type="fig" rid="F3">Figure 3D</xref>). The Hm/Gt ratios varied between 0 and 0.5 (<xref ref-type="fig" rid="F3">Figure 3E</xref>). To compare with Site 1177, the trend of Hm/Gt ratios on Site 1148 (<xref ref-type="bibr" rid="B5">Clift et al., 2014</xref>) was shown (<xref ref-type="fig" rid="F3">Figure 3F</xref>). Obviously, Sites 1148 and 1177 have different trends in Hm/Gt ratios.</p>
<p>The <italic>&#x3c7;</italic>
<sub>lf</sub>, <italic>&#x3c7;</italic>
<sub>hf</sub>, <italic>&#x3c7;</italic>
<sub>fd</sub>, <italic>&#x3c7;</italic>
<sub>ARM</sub>, SIRM, and <italic>&#x3c7;</italic>
<sub>ARM</sub>/SIRM variations are shown in <xref ref-type="fig" rid="F3">Figures 3G&#x2013;3L</xref>. Although these rock-magnetic parameters are somewhat scattered, and could not be divided into two parts as clearly as <italic>L</italic>-ratio and P<sub>425 nm</sub>, there is still a rough transition point at &#x223c;16.5&#xa0;Ma. The mean values of these magnetic parameters are also different before and after &#x223c;16.5&#xa0;Ma. For example, before &#x223c;16.5&#xa0;Ma, the mean values for <italic>&#x3c7;</italic>
<sub>lf</sub>, <italic>&#x3c7;</italic>
<sub>hf,</sub> <italic>&#x3c7;</italic>
<sub>fd,</sub> <italic>&#x3c7;</italic>
<sub>ARM,</sub> SIRM, and <italic>&#x3c7;</italic>
<sub>ARM</sub>/SIRM are 9.02 &#xd7; 10<sup>-8</sup>&#xa0;m<sup>3</sup>/kg, 8.96 &#xd7; 10<sup>-8</sup>&#xa0;m<sup>3</sup>/kg, 6.90 &#xd7; 10<sup>-10</sup>&#xa0;m<sup>3</sup>/kg, 2.81 &#xd7; 10<sup>-8</sup>&#xa0;m<sup>3</sup>/kg, 1.74 &#xd7; 10<sup>-4</sup>&#xa0;Am<sup>2</sup>/kg, and 2.56 &#xd7; 10<sup>-4</sup>&#xa0;A/m, respectively. After &#x223c;16.5&#xa0;Ma, the mean values become <italic>&#x3c7;</italic>
<sub>lf</sub> (1.05 &#xd7; 10<sup>-7</sup>&#xa0;m<sup>3</sup>/kg), <italic>&#x3c7;</italic>
<sub>hf</sub> (1.03 &#xd7; 10<sup>-7</sup>&#xa0;m<sup>3</sup>/kg), <italic>&#x3c7;</italic>
<sub>fd</sub> (1.65 &#xd7; 10<sup>-9</sup>&#xa0;m<sup>3</sup>/kg), <italic>&#x3c7;</italic>
<sub>ARM</sub> (1.12 &#xd7; 10<sup>-8</sup>&#xa0;m<sup>3</sup>/kg), SIRM (3.48 &#xd7; 10<sup>-4</sup>&#xa0;Am<sup>2</sup>/kg), and <italic>&#x3c7;</italic>
<sub>ARM</sub>/SIRM (4.91 &#xd7; 10<sup>-5</sup>&#xa0;A/m). These differences imply different properties of magnetic minerals around &#x223c;16.5&#xa0;Ma.</p>
</sec>
<sec sec-type="discussion" id="s4">
<title>Discussions</title>
<p>Overall, rock-magnetic, spectral, and geochemical parameters for sediments from the Site 1177 all shift at &#x223c;16.5&#xa0;Ma in different degrees (<xref ref-type="fig" rid="F3">Figure 3</xref>). Although different methods have inherent complexities in interpreting the sediment provenances, the combined method is the best approach to mutually attest to the potential changes in provenances.</p>
<p>First, the mineralogy, concentration, and grain size of magnetic minerals are tightly related to primary tectonic and/or environmental evolution (<xref ref-type="bibr" rid="B27">Liu et al., 2012</xref>). Variations in the magnetic parameters of sediments from Site 1177 indicate that the overall concentration of magnetic particles is larger (<xref ref-type="fig" rid="F3">Figures 3G&#x2013;I</xref>) and low-coercivity magnetic particles are coarser since &#x223c;16.5&#xa0;Ma (<xref ref-type="fig" rid="F3">Figures 3B,</xref>L), which suggests that there should be a crucial geological and/or environmental change at &#x223c;16.5&#xa0;Ma.</p>
<p>The Philippine Sea is dominated by the sub-tropical East Asian monsoonal climate (<xref ref-type="bibr" rid="B54">Xu et al., 2012</xref>). Annual precipitation mostly occurs during the summer monsoon season (May&#x2013;October) while dry winds prevail during the winter monsoon season (November&#x2013;April) (<xref ref-type="bibr" rid="B31">Liu et al., 2009</xref>). Hm/Gt has been successfully employed as an indicator of subtropical East Asian monsoonal precipitation, the higher Hm/Gt, the less precipitation and weaker summer monsoon (e.g., <xref ref-type="bibr" rid="B60">Zhang et al., 2007</xref>; <xref ref-type="bibr" rid="B8">Gai et al., 2020</xref>). However, variations in the Hm/Gt record from Site 1177 share little similarity with that from the South China Sea Site 1148 (<xref ref-type="fig" rid="F3">Figures 3E,F</xref>), which also locates in the subtropical East Asian monsoonal region (<xref ref-type="bibr" rid="B5">Clift et al., 2014</xref>). Differences between these two sites suggest that paleoclimate evolution cannot be used solely to explain the Hm/Gt record at Site 1177. Alternatively, geological processes such as sediment provenance and transportation changes should be taken into consideration. The mean <italic>L</italic>-ratio value is lower for sediment from the Site 1177 since &#x223c;16.5&#xa0;Ma (<xref ref-type="fig" rid="F3">Figure 3B</xref>), which indicates that coercivity of hard magnetic minerals (i.e., hematite and goethite) are changed systematically. Meanwhile, the characteristic DRS band position of goethite changed from approximately 413&#xa0;nm to larger and variable wavelengths (<xref ref-type="fig" rid="F3">Figure 3C</xref>), which indicates that the degree of Al substitution in goethite is increased and further explains the <italic>L</italic>-ratio value changes at &#x223c;16.5&#xa0;Ma. That is, different degrees of Al substitution in goethite leads to changes in coercivity and affect the <italic>L</italic>-ratio values. Considering that the degree of Al substitution in antiferromagnetic minerals is correlated with the weathering condition in the material provenance (<xref ref-type="bibr" rid="B16">Hu et al., 2016</xref>), and the overall weathering condition is relatively stable (<xref ref-type="bibr" rid="B5">Clift et al., 2014</xref>), it is suggested that the shift of magnetic properties of sediments from the Site 1177 can be attributed to a provenance change.</p>
<p>Second, Sr and Nd isotopes are useful in tracing source changes (<xref ref-type="bibr" rid="B52">Wei et al., 2012</xref>; <xref ref-type="bibr" rid="B5">Clift et al., 2014</xref>). Clay mineral analyses suggested that the Izu-Bonin Arc was an important source for Site 1177 (<xref ref-type="bibr" rid="B50">Underwood and Fergusson, 2005</xref>). However, features of Sr-Nd isotopes from Site 1177 differ from that in the Izu-Bonin Arc, which indicates that the Izu-Bonin Arc cannot be the only provenance that feeds the Philippine Sea Plate and materials from other regions are needed to produce the Sr-Nd isotopic pattern in Site 1177. <xref ref-type="bibr" rid="B29">Liu et al. (2021)</xref> and <xref ref-type="bibr" rid="B4">Clift et al. (2013)</xref> suggested that the Pearl River and Yangtze River could provide materials to Site 1177. Therefore, we suggested that the early to middle Miocene provenances of Site 1177 were a mixture of the Izu-Bonin Arc, Pearl River, and Yangtze River. The pre-16.5&#xa0;Ma and post-16.5&#xa0;Ma Sr-Nd isotopes exhibit different patterns (<xref ref-type="fig" rid="F4">Figure 4</xref>), which is consistent with variations in magnetic proxies at &#x223c; 16.5&#xa0;Ma (<xref ref-type="fig" rid="F3">Figures 3B&#x2013;L</xref>). The clay mineralogical data (<xref ref-type="fig" rid="F3">Figures 3M,N</xref>) from <xref ref-type="bibr" rid="B50">Underwood and Fergusson (2005)</xref> also show detectable changes at &#x223c;16.5&#xa0;Ma.</p>
<p>Third, zircons from the Pearl River and the Yangtze River were detected in Site 1177 turbidites deposited at &#x223c;18.6&#xa0;Ma and &#x223c;15.4&#xa0;Ma, respectively (<xref ref-type="bibr" rid="B4">Clift et al., 2013</xref>; <xref ref-type="bibr" rid="B29">Liu et al., 2021</xref>). The turbidites at &#x223c;18.6&#xa0;Ma and &#x223c;15.4&#xa0;Ma not only have different zircon age spectra, but they also have different lithologies, thicknesses of strata, stratigraphic units, and paleolatitudes. This implies that there was a provenance shift between &#x223c;18.6&#xa0;Ma and &#x223c;15.4&#xa0;Ma.</p>
<p>Given that the Izu-Bonin Arc has always been providing materials in the Miocene (<xref ref-type="bibr" rid="B50">Underwood and Fergusson, 2005</xref>), the shift of provenance could be attributed to the change of sources from Pearl River to Yangtze River. In fact, the Izu-Bonin Arc was oriented northwest and was at a relatively low latitude at &#x223c;20&#xa0;Ma (<xref ref-type="bibr" rid="B29">Liu et al., 2021</xref>), which would prevent the transport of materials from the Yangtze River. Therefore, we suggest that mudstone materials in Site 1177 are sourced more from the Izu-Bonin Arc and the Pearl River before &#x223c;16.5&#xa0;Ma, and from the Izu-Bonin Arc and the Yantze River after that.</p>
<p>The provenance evolutionary results are consistent with the paleomagnetic tectonic model that the Philippine Sea Plate experienced northward movement and clockwise rotation since the Eocene (<xref ref-type="bibr" rid="B12">Hall, 2002</xref>; <xref ref-type="bibr" rid="B37">Queano et al., 2007</xref>; <xref ref-type="bibr" rid="B29">Liu et al., 2021</xref>). It is obvious that the acceleration of the northward movement and clockwise rotation of the Philippine Sea Plate also occurred at approximately &#x223c;16.5&#xa0;Ma (<xref ref-type="fig" rid="F3">Figures 3O&#x2013;R</xref>). Therefore, we suggest that the tectonic evolution plays a key role in the source shift at &#x223c;16.5&#xa0;Ma for the studied site. <xref ref-type="bibr" rid="B29">Liu et al. (2021)</xref> proposed a model that the South China Sea was geographically connected to the Shikoku Basin at &#x223c;20&#xa0;Ma (<xref ref-type="fig" rid="F5">Figure 5A</xref>). Because of the collision between the Australian Plate and the Southeast Asia at &#x223c;20&#xa0;Ma (<xref ref-type="bibr" rid="B44">Sdrolias et al., 2004</xref>) or &#x223c;23&#xa0;Ma (<xref ref-type="bibr" rid="B11">Hall, 2011</xref>), the Shikoku Basin began to separate from the South China Sea. At &#x223c;15&#xa0;Ma, the Shikoku Basin had completely separated from the South China Sea (<xref ref-type="fig" rid="F5">Figure 5C</xref>). However, the initial time when the Shikoku Basin had completely separated from the South China Sea is unknown. Our new rock-magnetic, spectral, and geochemical analyses suggest that the provenance shift occurred significantly at &#x223c; 16.5&#xa0;Ma, which implies that the Shikoku Basin had thoroughly separated from the South China Sea at &#x223c;16.5&#xa0;Ma (<xref ref-type="fig" rid="F5">Figure 5B</xref>). Considering that the spreading of the South China Sea ceased at 16&#x2013;15&#xa0;Ma (<xref ref-type="bibr" rid="B25">Li et al., 2014</xref>), which is close to the full-separation time between the South China Sea and the Shikoku Basin at &#x223c;16.5&#xa0;Ma, it is possible that these two tectonic events are attributed to an identical dynamic mechanism. The paleolatitude of the South China Block was relatively stable during the opening of the South China Sea (<xref ref-type="bibr" rid="B17">Huang et al., 2008</xref>), the stop spreading of the South China Sea should be related to the plate located south of the South China Sea. The Australia plate, located to the south of the South China Sea and the Philippine Sea Plate, has been moving northward since the Cenozoic (<xref ref-type="bibr" rid="B12">Hall, 2002</xref>; <xref ref-type="bibr" rid="B45">Seton et al., 2012</xref>), which can not only explain the separation between the Shikoku Basin and the South China Sea but also account for the stop spreading of the South China Sea. With the Australian Plate moving northward, there is no room for the South China Sea to spread at 16&#x2013;15&#xa0;Ma, whereas the Shikoku Basin, with its subduction zone to the north, could move northward and clockwise rotate to sperate from the South China Sea. <xref ref-type="bibr" rid="B50">Underwood and Fergusson (2005)</xref>, and <xref ref-type="bibr" rid="B51">Underwood and Pickering (2018)</xref> proposed that the Shikoku Basin was close to Japan and received sediments from Japan, the East China Sea, and the Izu-Bonin Arc since the middle Miocene. By combining our new results, we further suggest that the Shikoku Basin could have experienced considerable northward motion and clockwise rotation between the early Miocene and middle Miocene.</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>The tectonic and provenance evolution of the Shikoku Basin at &#x223c;20&#xa0;Ma (<xref ref-type="bibr" rid="B29">Liu et al., 2021</xref>), &#x223c;16.5&#xa0;Ma (this study), and &#x223c;15&#xa0;Ma (<xref ref-type="bibr" rid="B29">Liu et al., 2021</xref>). <bold>(A)</bold> The Shikoku Basin connected with the South China Sea, and Site 1177 received materials from the Pearl River and Izu-Bonin Arc at &#x223c;20&#xa0;Ma. <bold>(B)</bold> The initial complete separation between the Shikoku Basin and the South China Sea was at &#x223c;16.5&#xa0;Ma, and Site 1177 began to receive materials from the Yangtze River and Izu-Bonin Arc. <bold>(C)</bold> The Shikoku Basin moved further northward at &#x223c;15&#xa0;Ma, and the provenance of Site 1177 was the same with that at &#x223c; 16.5&#xa0;Ma. The red arrows indicate the provenance directions. The dashed lines in <bold>(A)</bold> denote the recovered subducted slabs of the South China Sea (<xref ref-type="bibr" rid="B61">Zhao et al., 2019</xref>) and Shikoku Basin (<xref ref-type="bibr" rid="B53">Wu et al., 2016</xref>). To emphasize the relationships between the South China Sea and the Shikoku Basin, some ridges in the West Philippine Basin were not shown.</p>
</caption>
<graphic xlink:href="feart-10-870298-g005.tif"/>
</fig>
</sec>
<sec sec-type="conclusion" id="s5">
<title>Conclusion</title>
<p>The provenances of sedimentary rocks from Site 1177 were comprehensively studied based on the temporal variations of geochemical, rock-magnetic, and spectral parameters from &#x223c;22&#xa0;Ma to &#x223c;14&#xa0;Ma. The results show that the provenance shifted at &#x223c;16.5&#xa0;Ma. Before 16.5&#xa0;Ma, mudstone materials mainly came from the Pearl River and Izu-Bonin Arc. After &#x223c;16.5&#xa0;Ma, the materials originated from the Yangtze River and Izu-Bonin Arc. The provenance evolution is consistent with the Philippine Sea Plate tectonic model that the Shikoku Basin experienced northward motion and clockwise rotation in the Miocene, and the provenance shift constrains the time when the Shikoku Basin has been completely separated from the South China Sea at &#x223c;16.5&#xa0;Ma.</p>
</sec>
</body>
<back>
<sec id="s6">
<title>Data Availability Statement</title>
<p>The original contributions presented in the study are included in the article/Supplementary Material, further inquiries can be directed to the corresponding author.</p>
</sec>
<sec id="s7">
<title>Author Contributions</title>
<p>QL designed the study and revised the manuscript. WL conducted the experiments, analyzed the data, and wrote the initial manuscript. CG helped to analyze the data and revised the manuscript. WF, YAZ, YIZ, WC, and YL helped to analyze the data. XZ revised the manuscript.</p>
</sec>
<sec id="s8">
<title>Funding</title>
<p>This study was supported by the National Natural Science Foundation of China (92158208, 41874076, 41874078, 42002052, 41704068), the China Postdoctoral Science Foundation (2021M701557), the opening foundation (SSKP202101) of the Shanghai Sheshan National Geophysical Observatory, Shanghai, China, and the Shenzhen Science and Technology Program (KQTD20170810111725321).</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>Samples in this research were provided by the Ocean Drilling Program (ODP). We thank Prof. Minghui Zhao and Prof. Jian Lin provided good suggestions.</p>
</ack>
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