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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="research-article">
  <front>
    <journal-meta><journal-id journal-id-type="publisher">CP</journal-id><journal-title-group>
    <journal-title>Climate of the Past</journal-title>
    <abbrev-journal-title abbrev-type="publisher">CP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Clim. Past</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1814-9332</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/cp-21-1853-2025</article-id><title-group><article-title>Quantitative reconstruction of deglacial bottom-water nitrate in marginal Pacific seas using the pore density of denitrifying benthic foraminifera</article-title><alt-title>Quantitative reconstruction of deglacial bottom-water nitrate</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Govindankutty Menon</surname><given-names>Anjaly</given-names></name>
          <email>anjalygmenon9@gmail.com</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Bieler</surname><given-names>Aaron L.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Firrincieli</surname><given-names>Hanna</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Alcorn</surname><given-names>Rachel</given-names></name>
          
        <ext-link>https://orcid.org/0009-0007-9350-998X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff6">
          <name><surname>Lahajnar</surname><given-names>Niko</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Davis</surname><given-names>Catherine V.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4279-5369</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Schiebel</surname><given-names>Ralf</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Nürnberg</surname><given-names>Dirk</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff6">
          <name><surname>Schmiedl</surname><given-names>Gerhard</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Glock</surname><given-names>Nicolaas</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Department of Earth System Sciences, Institute for Geology, Universität Hamburg, Bundesstrasse 55, 20146 Hamburg, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Climate Geochemistry Department, Max Planck Institute for Chemistry, Hahn-Meitner-Weg 1, 55128 Mainz, Germany</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Department of Earth and Planetary Sciences, ETH Zürich, Sonneggstrasse 5, 8092 Zürich, Switzerland</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Department of Marine, Earth, and Atmospheric Sciences, North Carolina State University, 2800 Faucette Dr, Raleigh, NC, 27607, USA</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>GEOMAR Helmholtz Centre for Ocean Research Kiel, Wischhofstr. 1-3, Geb. 8c, Raum 106, 24148 Kiel, Germany</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Center for Earth System Research and Sustainability, Institute for Geology, Universität Hamburg, Bundesstrasse 55, 20146 Hamburg, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Anjaly Govindankutty Menon (anjalygmenon9@gmail.com)</corresp></author-notes><pub-date><day>27</day><month>October</month><year>2025</year></pub-date>
      
      <volume>21</volume>
      <issue>10</issue>
      <fpage>1853</fpage><lpage>1869</lpage>
      <history>
        <date date-type="received"><day>12</day><month>March</month><year>2025</year></date>
           <date date-type="rev-request"><day>25</day><month>March</month><year>2025</year></date>
           <date date-type="rev-recd"><day>5</day><month>September</month><year>2025</year></date>
           <date date-type="accepted"><day>15</day><month>September</month><year>2025</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2025 Anjaly Govindankutty Menon et al.</copyright-statement>
        <copyright-year>2025</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://cp.copernicus.org/articles/21/1853/2025/cp-21-1853-2025.html">This article is available from https://cp.copernicus.org/articles/21/1853/2025/cp-21-1853-2025.html</self-uri><self-uri xlink:href="https://cp.copernicus.org/articles/21/1853/2025/cp-21-1853-2025.pdf">The full text article is available as a PDF file from https://cp.copernicus.org/articles/21/1853/2025/cp-21-1853-2025.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e203">Quantifying past ocean nitrate concentrations is crucial for understanding the global nitrogen cycle. Here, we reconstruct deglacial bottom-water nitrate concentrations ([NO<inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub>) in the oxygen-deficient zones of the Sea of Okhotsk, the Gulf of California, the Mexican Margin, and the Gulf of Guayaquil. Using the pore density of denitrifying benthic foraminifera as a nitrate proxy, differences in [NO<inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> are observed at the study sites spanning the Last Glacial Maximum to the Holocene. Changes in water-column denitrification, water-mass ventilation, primary productivity, and sea surface temperatures may account for nitrate differences at the study sites. The [NO<inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> in the Sea of Okhotsk, the Gulf of California, and the Gulf of Guayaquil are influenced by the intermediate water masses while, the [NO<inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> at the Mexican Margin is likely influenced by deglacial changes in the Pacific Deep Water. The comparison of past and present [NO<inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] shows that the modern Gulf of Guayaquil and the Gulf of California currently have stronger oxygen-deficient zones with higher denitrification than during the Last Glacial Maximum. In contrast, the modern Mexican Margin and the Sea of Okhotsk may have higher oxygen than during the Last Glacial Maximum, indicated by low modern denitrification.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Deutsche Forschungsgemeinschaft</funding-source>
<award-id>Heisenberg grant GL 999/3-1 and grant GL 999/4-1</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d2e312">The marine nitrogen cycle is a complex web of microbially mediated processes controlling the inventory and distribution of bioavailable nitrogen in marine environments (Casciotti, 2016). Biological nitrogen fixation by nitrogen-fixing diazotrophs (e.g., cyanobacteria) in the surface layer is the main source of bioavailable nitrogen in the ocean, and denitrification and anammox, are the main fixed nitrogen loss processes (Lam and Kuypers, 2011), both of which occur under low-oxygen conditions. The primary form of bioavailable nitrogen in the ocean is nitrate (NO<inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>), (Casciotti, 2016), which is a limiting nutrient throughout the tropical and subtropical oceans (Moore et al., 2013).</p>
      <p id="d2e327">Oxygen-deficient zones (ODZs) are regions of very low dissolved oxygen (O<sub>2</sub>) where the O<sub>2</sub> concentration is less than 22 <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup>, usually within depths of 100–1200 m (Levin, 2003; 2018). Oxygen plays a key role in the marine nitrogen cycle (Keeling et al., 2010) because some microbial processes require oxygen while others are inhibited by it (Voss et al., 2013). For example, denitrification (reduction of nitrate to dinitrogen gas) in the ocean occurs in suboxic (oxygen <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M16" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup>) conditions (Codispoti et al., 2001; Levin, 2018). On a global scale, <inline-formula><mml:math id="M18" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 %–50 % of fixed nitrogen loss in the world's oceans occurs in ODZs (Gruber, 2008), either through denitrification or anammox (Devol et al., 2006; Lam and Kuypers, 2011; Evans et al., 2023). Due to the complex interactions and feedbacks within the biogeochemical nitrogen cycle, the amount of benthic denitrification also influences other important processes, such as global nitrogen fixation and net primary production (Somes et al., 2017; Li et al., 2024). Oxygen Deficient Zones cover only 1 % of the world's seafloor (Codispoti et al., 2001), however, 10 % of the global benthic denitrification occurs in these regions (Bohlen et al., 2012). Observations and climate model simulations have predicted that ODZs will continue to expand until at least the year 2100 (Stramma et al., 2008, 2010; Schmidtko et al., 2017; Oschlies, 2021). However, the long-term evolution of ODZs remains uncertain (Yamamoto et al., 2015; Takano et al., 2018; Fu et al., 2018; Frölicher et al., 2020). There is growing evidence that ODZs may contract during transient and equilibrium climate warmings over timescales of millennia and beyond (Auderset et al., 2022; Moretti et al., 2024). Considering the role of ODZs in modulating the marine nitrogen cycle, it is of key scientific interest to understand how nitrogen cycling works in these ecosystems and the potential factors that influence the nitrogen cycle.</p>
      <p id="d2e406">In this study, we use the pore density (number of pores per unit area) of <italic>Bolivina spissa </italic>and <italic>Bolivina subadvena </italic>as a NO<inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> proxy (Fig. 1a) to reconstruct bottom-water nitrate [NO<inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> in intermediate water depths of the Sea of Okhotsk, the Gulf of California, the Gulf of Guayaquil, and in the Pacific Deep Water (PDW) depths of the Mexican Margin (Figs. 2 and 3). The [NO<inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> calibration using the pore density of <italic>B. spissa </italic>and <italic>B. subadvena </italic>(see Fig. 1b) developed in Govindankutty Menon et al. (2023) is applied in the current study. Combining a proxy for [NO<inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> (pore density of denitrifying foraminifera) and a proxy for N-cycle processes in the water column (<inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub>) facilitates a more comprehensive understanding of past N-cycling in different zones of the water column. Here, we try to understand 1) whether there are differences in reconstructed [NO<inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> between today, deglacial, and glacial periods in the four studied sites, and 2) whether the reconstructed [NO<inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> records are in agreement with insights drawn from <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> data.</p>
<sec id="Ch1.S1.SS1">
  <label>1.1</label><title>Application of <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> and its potential limitations</title>
      <p id="d2e609">The stable isotope signature of nitrogen in the sedimentary organic matter (<inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">bulk</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is an established proxy for water-column denitrification and for understanding changes associated with nutrient utilization (Thunell et al., 2004; Robinson et al., 2009; Martinez and Robinson, 2010; Dubois et al., 2011, 2014; Tesdal et al., 2013; Wang et al., 2019; Riechelson et al., 2024). An increase (or decrease) in nutrient availability in relation to nutrient demand results in an increase (or decrease) in <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N values (Wada and Hattori, 1978; Montoya et al., 1990). When the oxygen in the ocean is depleted, either due to global warming or increased remineralization, denitrification rates in the water column are also increasing and so is <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N (Wang et al., 2019). Therefore, <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> can be an important tool for reconstructing past changes in denitrification in the ODZs.</p>
      <p id="d2e678">The <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N records from the bulk sediment can be subject to interlinked processes/or sources which can complicate their interpretation. For example, diagenetic alteration during sinking in the water column and burial in the sediment (Altabet and Francois, 1994; Lourey et al., 2003), as well as terrestrial or shelf sources of organic and inorganic nitrogen (Schubert and Calvert, 2001; Kienast et al., 2005; Meckler et al., 2011), and remotely advected water masses with different <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N values (for e.g., Southern Californian margin; Liu and Kaplan, 1989), could influence the <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N signatures in sediments. Nevertheless, Tesdal et al. (2013) proposed that <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> can be a reliable indicator for individual locations reflecting the oceanographic conditions of the surrounding environments.</p>
      <p id="d2e734">The nitrogen isotopes of organic matter bound and protected within the calcite shell of planktic foraminifera (<inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>FB</sub>) are less subjected to diagenesis or sedimentary contamination than <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> and can be used to understand major nitrogen transformations occurring in the ocean (Ren et al., 2012; Studer et al., 2021). There are well-documented disagreements between bulk sediment <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N and foraminifera-bound <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N records, particularly in glacial-interglacial comparisons (Studer et al., 2021). While <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> suggests strong variability in water-column denitrification between the LGM and deglaciation, <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>FB</sub> records indicate a more moderate change, with a peak during deglaciation but relatively stable values during the LGM and Holocene. This highlights that <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> and <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>FB</sub> may reflect different aspects of the nitrogen cycle (Studer et al., 2021). Recent studies (Auderset et al., 2022; Hess et al., 2023; Moretti et al., 2024) based on <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>FB</sub> have shown that water column denitrification decreased and ODZs contracted during warmer-than-present periods of the Cenozoic. In contrast, Riechelson et al. (2024) used <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> and hypothesized that the decrease in <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values over the Holocene is related to a decrease in Southern Ocean nutrient utilization and not due to a decrease in denitrification.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e945">The <bold>(a)</bold> schematic view of nitrate (NO<inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) uptake, and the excretion of nitrogen gas (N<sub>2</sub>) by the benthic foraminifera <italic>Bolivina spissa</italic>. The step-wise denitrification pathway from NO<inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> to N<sub>2</sub> involving enzymes such as nitrate reductase (Nr Nar), nitrite reductase (Nir), nitric-oxide reductase (Nor), and nitrous oxide reductase (Nos) is also shown. <bold>(b)</bold> Correlation between pore density of <italic>Bolivina spissa</italic> from Peru, off Costa Rica, Sagami Bay, and <italic>Bolivina subadvena </italic> with bottom-water nitrate [NO<inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> from Govindankutty Menon et al. (2023). If no species name is indicated in the legend, the analysed species was <italic>B. spissa</italic>. The error bars are 1 standard error of the mean.</p></caption>
          <graphic xlink:href="https://cp.copernicus.org/articles/21/1853/2025/cp-21-1853-2025-f01.png"/>

        </fig>

</sec>
<sec id="Ch1.S1.SS2">
  <label>1.2</label><title>Pore density of benthic foraminifera as a bottom-water nitrate proxy</title>
      <p id="d2e1046">Foraminifera account for a major part of benthic denitrification in the ODZs (up to 100 % in some environments) (Piña-Ochoa et al., 2010a, b; Glock et al., 2013; Dale et al., 2016; Choquel et al., 2021; Rakshit et al., 2025). Some species, for example <italic>B. spissa</italic>, which are abundant in ODZs in and around the Pacific Ocean (Glock et al., 2011; Fontanier et al., 2014) can use NO<inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> as an electron acceptor (see Fig. 1a) and thus can denitrify (Risgaard-Petersen et al., 2006; Piña-Ochoa et al., 2010a, b). A study by Glock et al. (2019) proposed for some denitrifying foraminifera, denitrification is their preferred respiration pathway. The uptake of NO<inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> by  these  foraminifera is likely through pores in the test (see Fig. 1a). Nitrate is completely denitrified to dinitrogen gas (N<sub>2</sub>) partly by the foraminifera themselves (Risgaard-Petersen et al., 2006; Woehle and Roy et al., 2018; Orsi et al., 2020; Gomaa et al., 2021), and partly supported by prokaryotic endobionts (Bernhard et al., 2012a, Woehle and Roy et al., 2022). To date, benthic foraminifera are the only eukaryote holobiont known to perform complete heterotrophic denitrification (Risgaard-Petersen et al., 2006; Kamp et al., 2015). Every <italic>Bolivina</italic> species tested so far (including <italic>Bolivina seminuda</italic>), can denitrify (Piña-Ochoa et al., 2010a; Bernhard et al., 2012b), suggesting that denitrification is a common survival strategy of Bolivinidae under oxygen-depleted conditions (Glock et al., 2019). This makes species of this genus particularly suitable candidates for reconstructing past nitrate levels using pore characteristics as a proxy. In low-oxygen environments, such as the ODZs off Peru, Costa Rica, and the hypoxic Sagami Bay, <italic>B. spissa</italic> increase their pore density with decreasing ambient NO<inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> availability (Govindankutty Menon et al., 2023). Thus, the pore density of several <italic>Bolivina</italic> species, such as <italic>B. spissa</italic>, and <italic>B. subadvena</italic>, is an empirically calibrated proxy that shows the strongest correlation with the bottom-water nitrate concentration (see Fig. 1b) (Glock et al., 2011; Govindankutty Menon et al., 2023) rather than bottom-water oxygen, temperature, water depth, salinity or pore water nitrate.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e1118">Location of sediment cores used in the current study and mean annual oxygen concentrations at 700 m depth (Garcia et al., 2019). Sediment cores are indicated by yellow triangles: Sea of Okhotsk (core MD01-2415; water depth: 822 m), Gulf of California (DSDP Site- 480; water depth: 747 m), Mexican Margin (core MAZ-1E-04; water depth: 1463 m), and Gulf of Guayaquil (core M77/2-59-01; water depth: 997 m). Map created with Ocean Data View (Schlitzer,  2023).</p></caption>
          <graphic xlink:href="https://cp.copernicus.org/articles/21/1853/2025/cp-21-1853-2025-f02.png"/>

        </fig>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e1129">Modern <bold>(a)</bold> salinity and <bold>(b)</bold> nitrate distribution along a N–S transect across the Pacific (Garcia et al., 2019) with major subsurface and deep-water masses (blue arrows) and formation areas of North Pacific Intermediate Water (NPIW) and Southern Ocean Intermediate Water (SOIW) are included. Sediment cores used for [NO<inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> reconstruction are shown (red crosses) projected to the N-S hydrographic transect. Equatorial Pacific Intermediate Water (EqPIW), Equatorial Undercurrent (EUC), NPIW, SOIW, Pacific Deep Water (PDW), Antarctic Bottom Water (AABW), and Circumpolar Deep Water (CDW). Profiles generated by Ocean Data View (Schlitzer,  2023) using the data from World Ocean Atlas 2018 (Garcia et al., 2019).</p></caption>
          <graphic xlink:href="https://cp.copernicus.org/articles/21/1853/2025/cp-21-1853-2025-f03.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Materials and methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Study area and sampling of sediment cores</title>
      <p id="d2e1181">We used downcore samples from the Eastern Tropical South Pacific, ETSP (Gulf of Guayaquil (M77/2-59-01), Eastern Tropical North Pacific the ETNP (Mexican Margin, MAZ-1E-04), the Gulf of California (Guaymas Basin, DSDP-64-480), and the Sea of Okhotsk (MD01-2415), over the last <inline-formula><mml:math id="M79" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 20 000 years (Fig. 3). The Gulf of Guayaquil sediment core M77/2-59-01 (03°57.01<sup>′</sup> S, 81°19.23<sup>′</sup> W, recovery 13.59 m) was collected from the northern edge of the ODZ at a water depth of 997 m during the RV Meteor cruise M77/2 in 2008 (Mollier-Vogel et al., 2013, 2019; Nürnberg et al., 2015). The piston core MAZ-1E-04, Mexican Margin (22.9° N, 106.91° W) was collected on board the RV El Puma at a water depth of 1463 m. The CALYPSO giant piston core MD01-2415 (53°57.09<sup>′</sup> N, 149°57.52<sup>′</sup> E, recovery 46.23 m) was recovered from the northern slope of the Sea of Okhotsk at 822 m water depth during the WEPAMA cruise MD122 of the RV Marion Dufresne (Holbourn et al., 2002; Nürnberg and Tiedemann, 2004). The Deep-Sea Drilling Project core DSDP-480 (27°54<sup>′</sup> N, 111°39<sup>′</sup> W) from the Gulf of California was retrieved at a water depth of 747 m close to the Guaymas Basin. For details on the sampling procedure of foraminiferal specimens, please refer to the Supplement Methods section in the Supplement.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Automated image analysis</title>
      <p id="d2e1254">All specimens of <italic>B. spissa</italic> and <italic>B. subadvena</italic> were imaged using a Scanning Electron Microscope (Hitachi Tabletop SEM TM4000 series) at Hamburg University, Germany with an accelerating voltage of 15 kV using a back-scattered electron (BSE) detector (Further methodological details are provided in the Supplement).</p>
      <p id="d2e1263">Following the image analysis, pore density data of benthic foraminifera from the four ODZs were used for the quantitative reconstruction of [NO<inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> (Fig. 4). We distinguished five different time intervals, including the Last Glacial Maximum (LGM; 22–17 ka BP), Heinrich Stadial 1 (H1; 17–15 ka BP), Bølling – Allerød (BA; 14.7–12.9 ka BP), Younger Dryas (YD; 12.9–11.7 ka BP), Early Holocene (EH; 11.7–8.2 ka BP) and Middle to Late Holocene (MLH; 8–0 ka BP) to describe the [NO<inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> in the East Pacific and the Sea of Okhotsk. We present updated chronostratigraphies of the studied cores, primarily based on accelerator mass spectrometry (AMS) radiocarbon (<sup>14</sup>C) dating, as detailed in the Supplement Methods.</p>
      <p id="d2e1317">The [NO<inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> from all cores were calculated using the calibration equation;

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M93" display="block"><mml:mrow><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow><mml:msub><mml:mo>]</mml:mo><mml:mi mathvariant="normal">BW</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3896</mml:mn><mml:mo>(</mml:mo><mml:mo>±</mml:mo><mml:mn mathvariant="normal">350</mml:mn><mml:mo>)</mml:mo><mml:mi mathvariant="normal">PD</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">61</mml:mn><mml:mo>(</mml:mo><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></disp-formula>

          where PD is the pore density of benthic foraminifera (Govindankutty Menon et al., 2023).</p>
      <p id="d2e1391">The standard error of the mean (SEM) for one sample was calculated using the equation;

            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M94" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="normal">SEM</mml:mi><mml:mrow><mml:mo>[</mml:mo><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup><mml:msub><mml:mo>]</mml:mo><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="normal">SD</mml:mi><mml:mrow><mml:mo>[</mml:mo><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup><mml:msub><mml:mo>]</mml:mo><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow><mml:msqrt><mml:mi mathvariant="normal">n</mml:mi></mml:msqrt></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M95" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> is the number of specimens analyzed in each sample and SD is 1 standard deviation of mean reconstructed [NO<inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub>.

            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M98" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="normal">SD</mml:mi><mml:mrow><mml:mo>[</mml:mo><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup><mml:msub><mml:mo>]</mml:mo><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msqrt><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">350</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi>X</mml:mi><mml:mi mathvariant="normal">PD</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3896</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>X</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">SD</mml:mi><mml:mi mathvariant="normal">PD</mml:mi></mml:msub><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:msqrt></mml:mrow></mml:math></disp-formula>

          A complete error propagation was done for the calculation of the errors of the reconstructed [NO<sub>3</sub>]<sub>BW</sub> including both the uncertainty of the mean PD within the samples and the uncertainties of the calibration function. The reconstructed [NO<inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> and the calculated SEM and SD of each sample are shown in the Supplement.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Sedimentary nitrogen isotope (<inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub>) measurements</title>
      <p id="d2e1619">We have measured sedimentary nitrogen isotope (<inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">bulk</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> rather than <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>FB</sub> from cores taken from the Sea of Okhotsk, and Gulf of California, because the low abundances of foraminifera were utilized for other analysis. The analysis of bulk sediments allows for high-resolution records. Prior to the <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> measurements, the Total Nitrogen (TN %) content of 20 sediment samples from the Sea of Okhotsk and 54 samples from the Gulf of California were measured at the Institute for Geology, Hamburg University, Germany using a flash combustion method with a Eurovector EA-3000 analyzer. The <inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> measurements for both the Sea of Okhotsk and the Gulf of California were accomplished at the Max Planck Institute for Chemistry (Mainz), Germany using a DELTA V ADVANTAGE Isotope Ratio Mass Spectrometer (IRMS) equipped with a FLASH 2000 Organic Elemental Analyzer. The results were expressed in standard <inline-formula><mml:math id="M113" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>-notation (Eq. 4). The standard deviation (<inline-formula><mml:math id="M114" display="inline"><mml:mo lspace="0mm">±</mml:mo></mml:math></inline-formula> SD) of all individual analysis runs based on a certified international reference standard (USGS65) and internal laboratory standards (L-Phenylalanine and L-Glutamic acid) referenced to certified international reference standards was <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">‰</mml:mi></mml:mrow></mml:math></inline-formula>. The <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> data for the Sea of Okhotsk and the Gulf of California are shown in Supplement Table S1.

            <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M118" display="block"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">N</mml:mi></mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="normal">‰</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mo>[</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup><mml:mi mathvariant="normal">N</mml:mi><mml:msup><mml:mo>:</mml:mo><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:mi mathvariant="normal">N</mml:mi></mml:mrow><mml:mi mathvariant="normal">sample</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup><mml:mi mathvariant="normal">N</mml:mi><mml:msup><mml:mo>:</mml:mo><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:mi mathvariant="normal">N</mml:mi></mml:mrow><mml:mi mathvariant="normal">air</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>]</mml:mo><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></disp-formula>

          For the Gulf of Guayaquil core M77/2-59-01, the <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> data published by Mollier-Vogel et al. (2019) was used. Their measurements were done on <inline-formula><mml:math id="M121" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 5–50 mg of homogenized and freeze-dried bulk sediments using a Carlo-Erba CN analyzer 2500 interfaced directly to a Micromass-Isoprime mass spectrometer at Bordeaux University. Results are expressed in standard <inline-formula><mml:math id="M122" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>-notation (Eq. 4) relative to atmospheric dinitrogen gas (N<sub>2</sub>).</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Nitrate offset to present conditions</title>
      <p id="d2e1881">The reconstructed [NO<inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> from each location is subtracted from the modern [NO<inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] present at the respective locations from similar water depths the cores were retrieved from. This provided the [NO<inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] offset which is the difference (<inline-formula><mml:math id="M128" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>[NO<inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] (<inline-formula><mml:math id="M130" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>M)) between the modern [NO<inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] and the past reconstructed [NO<inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub>. The modern [NO<inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] for each location was taken from World Ocean Atlas 2018 (Garcia et al., 2019). The details are given in the Supplement.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
      <p id="d2e2011">We reconstructed deglacial [NO<inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> using downcore sediment samples from the Sea of Okhotsk (MD01-2415), the Gulf of California (DSDP- 480), the Mexican Margin (MAZ-1E-04), and the Gulf of Guayaquil (M77/2-59-01). The reconstructed [NO<inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> was compared to <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> records of all cores (Fig. 4). All data records presented cover the time period starting from the Last Glacial Maximum, except for the core from the Sea of Okhotsk, which covers the late deglacial to the Holocene.</p>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Sea of Okhotsk (MD01-2415)</title>
      <p id="d2e2084">The Sea of Okhotsk core MD01-2415 covers the Younger Dryas, (YD, 12.8 ka BP) until the Middle to Late Holocene (MLH, 4.9 ka BP). The reconstructed [NO<inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> values range from 32.8 to 44.1 <inline-formula><mml:math id="M143" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup> (Fig. 4a). A gradual increase in [NO<inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> is observed from the Younger Dryas to the Middle to Late Holocene. At the beginning of the Younger Dryas at 12.8 ka BP, [NO<inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> were relatively high and then decreased to a minimum value of 32.8 <inline-formula><mml:math id="M149" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup> at 12.4 ka BP. Since then, [NO<inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> steadily increased until the Middle to Late Holocene (MLH, 44.1 <inline-formula><mml:math id="M153" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup>) (Fig. 4a). The [NO<inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> during the Middle to Late Holocene (mean <inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">41.2</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M158" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup>) is significantly (<inline-formula><mml:math id="M160" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>-test, <inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.023</mml:mn></mml:mrow></mml:math></inline-formula>) higher than during the Younger Dryas (mean <inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">36.7</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M163" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup>). The sedimentary <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> record covers the interval from the Late Heinrich Stadial 1 (H1, 15.4 ka BP) to the Middle Holocene (6.1 ka BP). The <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values were relatively high ranging from 7.1 ‰ to 9.4 ‰ with an average of 8.7 ‰. The <inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values increased steadily from the Late Heinrich Stadial 1 (15.4 ka BP) to the Early Holocene (EH, 10 ka BP) with higher values centered between the Late Younger Dryas (11.9 ka BP) and the beginning of the Early Holocene. Since then, the <inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values decreased until the Middle to Late Holocene.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Gulf of California (DSDP-480)</title>
      <p id="d2e2424">The analyzed sections of DSDP Site 480 covered the Last Glacial Maximum (22 ka BP) until the Early Holocene (10.8 ka BP). The reconstructed [NO<inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> ranged from 41.4  to 49.1 <inline-formula><mml:math id="M175" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup>. The highest [NO<inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> of 49.1 <inline-formula><mml:math id="M179" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup> occurred during the Last Glacial Maximum (18.2 ka BP). The data points from the Early Holocene (11.6–10.8 ka BP) were the only Holocene data from this core providing the lowest [NO<inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> estimate of 42.1 <inline-formula><mml:math id="M183" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup> during the Early Holocene (10.8 ka BP) (Fig. 4b). A distinct difference in [NO<inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> between the glacial period (mean <inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">46.1</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M188" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup>) and the Early Holocene (42.7 <inline-formula><mml:math id="M190" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup>) was observed with [NO<inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> found to be substantially higher during the glacial period (<inline-formula><mml:math id="M194" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>-test, <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.0067</mml:mn></mml:mrow></mml:math></inline-formula>) (Fig. 4b). Accordingly, the [NO<inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> followed a decreasing pattern from the glacial period to the Early Holocene. The <inline-formula><mml:math id="M198" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values varied between 6.4 ‰ and 13 ‰ with an average of 10.2 ‰ (Fig. 4b). The <inline-formula><mml:math id="M200" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values from the Guaymas Basin were similar to the <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values (average 9.6 ‰) of Pride (1997) and Altabet et al. (1999). During the last glacial period, the <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values were low ranging from 8.5 ‰ to 9 ‰. At the onset of the deglaciation, the <inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values increased by more than 2 ‰ with large-scale changes reaching a maximum of 13 ‰ during the Younger Dryas. Afterward, we observed a gradual decline in <inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values throughout the Middle to Late Holocene (mean 10.7 ‰) and this pattern continued to the present.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Mexican Margin (MAZ-1E-04)</title>
      <p id="d2e2816">This core MAZ-1E-04 covered the Last Glacial Maximum (20.5 ka BP) until the Early Holocene (10.47 ka BP). The [NO<inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> values range from 37.7 to 43.5 <inline-formula><mml:math id="M212" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup>. We observed the highest [NO<inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> during the Younger Dryas. From the beginning to the end of the Last Glacial Maximum, [NO<inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> followed a decreasing trend (Fig. 4c). The [NO<inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> levels continued to steadily decrease until Heinrich Stadial 1 and consistently stayed low throughout this period. There was a strong change in [NO<inline-formula><mml:math id="M220" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> from the end of Heinrich Stadial 1 to the end of Younger Dryas (Fig. 4c). We observed a peak in [NO<inline-formula><mml:math id="M222" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> from the beginning of Bølling-Allerød, BA (14.29 ka BP) and it continued throughout the Younger Dryas (Fig. 4c). Afterwards, [NO<inline-formula><mml:math id="M224" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> declined during the Early Holocene. The <inline-formula><mml:math id="M226" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values taken from Alcorn et al. (2025) followed an increasing trend from the glacial towards the deglacial period (Fig. 4c).</p><fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e3011">Quantitative [NO<inline-formula><mml:math id="M228" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> reconstruction using the pore density of fossil specimens of <italic>B. spissa, B. subadvena</italic> from <bold>(a)</bold> the Sea of Okhotsk (MD01-2415), <bold>(b)</bold> the Gulf of California (DSDP-480), <bold>(c)</bold> the Mexican Margin (MAZ-1E-04), and <bold>(d)</bold> Gulf of Guayaquil (M77/2-59-01). The sedimentary nitrogen isotope (<inline-formula><mml:math id="M230" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<inline-formula><mml:math id="M231" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">bulk</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> records from the Sea of Okhotsk, and the Gulf of California are measured in this study, and the Gulf of Guayaquil is from Mollier-Vogel et al. (2019), and the Mexican Margin <inline-formula><mml:math id="M232" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> data is from Alcorn et al. (2025). The error bars of [NO<inline-formula><mml:math id="M234" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> represent 1 SEM including a complete error propagation (using Eqs. 3 and 4). The accumulation rate of total organic carbon (Supplement) calculated from published literature (Bubenshchikova et al., 2015; Leclaire and Kerry, 1982; Mollier-Vogel et al., 2019) is shown in blue dashed lines for the Sea of Okhotsk, the Gulf of California and the Gulf of Guayaquil cores respectively. The black dashed lines indicate the modern nitrate concentration of each location. Time intervals Middle to Late Holocene (MLH), Early Holocene (EH), Younger Dryas (YD), Bølling-Allerød (BA), Heinrich Stadial 1 (H1), and Last Glacial Maximum (LGM) are shown in the figure.</p></caption>
          <graphic xlink:href="https://cp.copernicus.org/articles/21/1853/2025/cp-21-1853-2025-f04.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Gulf of Guayaquil (M77/2-59-01)</title>
      <p id="d2e3131">This core covered the Last Glacial Maximum (18 ka BP) until the Middle to Late Holocene (0.18 ka BP). The reconstructed [NO<inline-formula><mml:math id="M236" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> values range from 40.5 to 46.5 <inline-formula><mml:math id="M238" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup>. The highest [NO<inline-formula><mml:math id="M240" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> occurred during the Last Glacial Maximum (Fig. 4d). The reconstructed [NO<inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> levels during the Last Glacial Maximum (mean <inline-formula><mml:math id="M244" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">45.6</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M245" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup>) were slightly higher than during the Middle to Late Holocene (mean <inline-formula><mml:math id="M247" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">44.9</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M248" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>mol kg<sup>−1</sup>) (<inline-formula><mml:math id="M250" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>-test, <inline-formula><mml:math id="M251" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.046</mml:mn></mml:mrow></mml:math></inline-formula>). The <inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values were relatively low ranging between 4 ‰ and 6 ‰ (Fig. 4d). During the Last Glacial Maximum, the <inline-formula><mml:math id="M254" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values were low, varying between 4.4 ‰ and 4.6 ‰, close to the typical mean range of dissolved nitrate in the ocean (Sigman et al., 1997). Subsequently, the <inline-formula><mml:math id="M256" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values increased from 16.7 ka BP (4.9 ‰), where we observed a decline in [NO<inline-formula><mml:math id="M258" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> to 8.9 ka BP (5.6 ‰). The highest <inline-formula><mml:math id="M260" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values centered at <inline-formula><mml:math id="M262" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 14 ka BP (5.9 ‰). From 8.9 ka BP onwards, a long-term decrease in <inline-formula><mml:math id="M263" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> (<inline-formula><mml:math id="M265" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">4.4</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">‰</mml:mi></mml:mrow></mml:math></inline-formula>) was observed until the Latest Holocene, consistent with higher [NO<inline-formula><mml:math id="M266" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> levels during the Holocene (Fig. 4d). Despite higher [NO<inline-formula><mml:math id="M268" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> levels, our reconstruction doesn't show any strong variations during the Holocene.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d2e3493">The pore density of benthic foraminifera represents a promising but still developing proxy for reconstructing past nitrate dynamics. Like most proxies based on biology, it reflects an indirect physiological response rather than a direct measure of nitrate. In addition, species-specific variability requires careful taxonomic control or its interpretation carries inherent limitations especially since not many records are available, yet, for this proxy. Thus, we used a multiproxy approach and combined it with <inline-formula><mml:math id="M270" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub>, which provides a complementary perspective that strengthens reconstructions of nitrogen-cycling processes in oxygen-deficient zones.</p>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Sea of Okhotsk</title>
      <p id="d2e3523">Our data show that [NO<inline-formula><mml:math id="M272" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> levels gradually increased through time and reached modern concentrations during the Middle-Holocene (Fig. 4a). Most of the nutrients in the northwestern Pacific including the Sea of Okhotsk are supplied by the upwelling of the North Pacific Deep Water (NPDW) (Gorbarenko et al., 2014). The weakened Kuroshio current (Ujiié and Ujiié, 1999) and increased sea ice extent (Ternois et al., 2001) weakened the upwelling of NPDW during the Last Glacial Maximum (LGM). Subsequent studies (Gray et al., 2020; Rae et al., 2020) have shown that the expansion of the North Pacific Gyre also resulted in less upwelling of NPDW during the LGM.</p>
      <p id="d2e3547">During the LGM, the subpolar North Pacific was better ventilated at intermediate depths (Keigwin, 1998) and export productivity was reduced (Ternois et al., 2001; Narita et al., 2002; Seki et al., 2004). This is consistent with a strengthened meridional overturning circulation, with enhanced formation of intermediate waters and advection of nutrient-depleted subtropical waters to high latitudes (Rae et al., 2020). Furthermore, the North Pacific subpolar gyre extended <inline-formula><mml:math id="M274" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 3° further south during the LGM (Gray et al., 2020), which shifted the westerly winds southward. This may have resulted in less upwelling of the NPDW during the LGM.</p>
      <p id="d2e3557">The prolonged ice cover with low biological productivity (Ternois et al., 2001; Narita et al., 2002; Seki et al., 2004; Rae et al., 2020) and well-oxygenated water masses (Keigwin, 1998) might have prevented the formation of an oxygen deficient zone (ODZ) in the Sea of Okhotsk (Bubenshchikova et al., 2015). This is supported by the absence of <italic>B. spissa</italic>, which are adapted to living in dysoxic conditions, in our records during the LGM.</p>
      <p id="d2e3563">Deglacial low [NO<inline-formula><mml:math id="M275" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> which correspond to higher <inline-formula><mml:math id="M277" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values (Fig. 4a) could be due to enhanced primary productivity. It is important to note, however, that <inline-formula><mml:math id="M279" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> is influenced by diagenetic alteration and the incorporation of allochthonous nitrogen, which can obscure the local denitrification signal. Therefore, interpretations of <inline-formula><mml:math id="M281" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> trends should be made cautiously and ideally corroborated with complementary proxies, such as foraminiferal pore density. Increased nutrient supply from the Asian continental shelves and sea-ice retreat (Ternois et al., 2001) strengthened primary productivity. Indeed, the accumulation rate of total organic carbon was relatively higher during the Younger Dryas (Bubenshchikova et al., 2015) in our core (Fig. 4a). The increased oxygen demand and weakened ventilation of intermediate waters in the subarctic Pacific (Lembke-Jene et al., 2018) gradually intensified the ODZ. These poorly oxygenated conditions conceivably strengthened denitrification, resulting in low deglacial [NO<inline-formula><mml:math id="M283" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> levels. However, during the Middle to Late Holocene (MLH) a reorganization in atmospheric circulation favored enhanced formation of oxygenated North Pacific Intermediate Water (NPIW) (Wang et al., 2020). Thus, mid-depth ventilation was closely associated with atmospheric circulation in the Holocene and a weakened ODZ (Ohkushi et al., 2013; Bubenshchikova et al., 2015; Wang et al., 2020). These rising oxygen concentrations probably reduced denitrification (low <inline-formula><mml:math id="M285" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">bulk</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in the Sea of Okhotsk, resulting in higher [NO<inline-formula><mml:math id="M287" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> comparable to today's conditions (Fig. 4). The <inline-formula><mml:math id="M289" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values show a maximum from 13 ka to 10 ka BP, which indicates increased water-column denitrification during that time. Nevertheless, the [NO<inline-formula><mml:math id="M291" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> increased during this time, which indicates a decoupling from denitrification in the oxygen minimum in the water column and the [NO<inline-formula><mml:math id="M293" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub>. This could be related to the sea level rise during that time (Waelbroeck et al., 2008), which increased the vertical distance of the sediments (i.e., bottom water) at the sampling site from the center of denitrification.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Gulf of California</title>
      <p id="d2e3785">The Gulf of California ODZ is influenced by both intermediate and deep-water properties, similar to that of the open Pacific Ocean. Thus, the ODZ intensity in the Guaymas Basin is largely dependent on the oxygen content and ventilation of inflowing NPIW from the Sea of Okhotsk (Pride et al., 1999) and the demand for oxygen at depth. During the glacial period, the dissolved oxygen concentrations were higher due to better-ventilated NPIW at intermediate depths of the Northeast Pacific (Keigwin and Jones, 1990; Ganeshram et al., 1995; Keigwin 1998; Duplessy et al., 1988; Herguera et al., 2010; Cartapanis et al., 2011). Modeling studies show that the Laurentide and Cordilleran ice sheets increased in size (Benson et al., 2003),  lowering the temperature of North America (Romanova et al., 2006) during the glacial period. The cold sinking air over the ice sheet established a semi-permanent high-pressure cell (Kutzbach and Wright Jr., 1985; Romanova et al., 2006) causing a substantially weaker North Pacific High (Ganeshram and Pedersen, 1998) or the southward displacement of the Inter Tropical Convergence Zone (Cheshire and Thurow, 2013). This resulted in a weak California Current along the coast and reduced upwelling-favorable winds (Cartapanis et al., 2011) along the North American coastline and reduced primary productivity (Ganeshram and Pedersen, 1998; Hendy et al., 2004; Cartapanis et al., 2011; Chang et al., 2015) within the ETNP and the Gulf of California during the glacial period. The nitrogen isotope ratios in the Guaymas Basin can be affected by subsurface denitrification in the Gulf and in the ETNP (Pride et al 1999). The increase in dissolved oxygen during the glacial period might have reduced water column denitrification (low <inline-formula><mml:math id="M295" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<inline-formula><mml:math id="M296" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">bulk</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> thereby increasing the [NO<inline-formula><mml:math id="M297" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> (Fig. 4b).</p>
      <p id="d2e3832">Our study finds a declining trend in reconstructed [NO<inline-formula><mml:math id="M299" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> during the Early Holocene, slowly approaching modern concentrations. This coincides with a maximum in <inline-formula><mml:math id="M301" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values, suggesting elevated denitrification. This agrees with previous studies in the ETNP (Kienast et al., 2002) and within the Gulf of California (Pride et al., 1999), which showed that high denitrification most likely was associated with warming temperatures that occurred during this period. Furthermore, the scarcity of benthic foraminifera after the Early Holocene in our study coincides with laminations of the sediment core (Keigwin and Jones, 1990) below 10.8 ka BP, where reconstructed [NO<inline-formula><mml:math id="M303" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> begins to decrease. It is possible that redox conditions were too hostile for benthic foraminifers in the time periods when laminated sediments formed. We acknowledge limitations in our Holocene reconstruction due to the low abundance of <italic>B. subadvena</italic> and the limited calibration dataset available for this species, which may introduce a systematic offset (Govindankutty Menon et al., 2023). <italic>Bolivina subadvena</italic> was used in this core due to the unavailability of <italic>B. spissa</italic>, and some values fall outside the existing calibration range. We also cannot rule out other factors influencing the proxy signal, such as microhabitat variability. Additional data and further proxy calibration are therefore essential to improve the robustness of Holocene bottom-water nitrate reconstructions.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Mexican Margin</title>
      <p id="d2e3915">Our study finds a steep rise in [NO<inline-formula><mml:math id="M305" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> between the Bølling-Allerød (BA) and the Younger Dryas (YD) (Fig. 4c). The transition period from the BA to the Holocene involved rapid oxygenation with increased oxygen levels at the onset of the YD (Jaccard and Galbraith, 2012; Ohkushi et al., 2013; Taylor et al., 2017). This has been linked to active ventilation by increased NPIW production at high latitudes in the North Pacific (Van Geen et al., 1996; Emmer and Thunell, 2000; Okazaki et al., 2010; Cartapanis et al., 2011; Chang et al., 2014). In addition, there was low primary productivity (Hendy et al., 2004; Pospelova et al., 2015), and a higher influx of freshwater (Broecker et al., 1985; Clark et al., 2002) during the YD. However, considering the deep location of the Mexican Margin core below the direct influence of intermediate water masses (Fig. 3), it is less likely to be reflected in the [NO<inline-formula><mml:math id="M307" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub>. Bulk sediment <inline-formula><mml:math id="M309" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N records in the ETNP (Ganeshram et al., 1995; Pride et al., 1999; Emmer and Thunell, 2000;  Kienast et al., 2002; Hendy et al., 2004) found a decrease in <inline-formula><mml:math id="M310" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> during the YD due to reduced denitrification. Furthermore, a foraminifera-bound nitrogen isotope (<inline-formula><mml:math id="M312" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>FB</sub>) study (Studer et al., 2021) in the eastern tropical Pacific also found a decrease in <inline-formula><mml:math id="M314" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>FB</sub> signatures during the Younger Dryas (Fig. 4c). In contrast to this, a bulk sediment <inline-formula><mml:math id="M316" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N record of MAZ-1E-04 (Alcorn et al., 2025) depicts an increase in water column denitrification during the Younger Dryas. Thus, reduced denitrification may not be the dominant factor that led to the elevated [NO<inline-formula><mml:math id="M317" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> during this time. Instead, the Mexican Margin may be more influenced by the NO<inline-formula><mml:math id="M319" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> variability from the Pacific Deep Water, PDW (see Fig. 3). Deep-sea reorganization and ventilation during the deglaciation may have influenced the [NO<inline-formula><mml:math id="M320" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub>. At the onset of the deglaciation, deep Southern Ocean ventilation (reduced <sup>14</sup>C ventilation ages) and atmospheric carbon dioxide (CO<inline-formula><mml:math id="M323" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> synchronously increased (Robinson et al., 2009; Burke and Robinson, 2012; Rae et al., 2018). This deglacial increase in <sup>14</sup>C ventilation in the Pacific Ocean suggests that most of the increase in atmospheric CO<sub>2</sub> is derived from old carbon in the Southern and Pacific Oceans (Rafter et al., 2022). The increase in reconstructed [NO<inline-formula><mml:math id="M326" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> during the YD may thus reflect the release of sequestered nutrient- and carbon dioxide-rich waters during the deglaciation (Robinson et al., 2009; Rafter et al., 2022).</p>
      <p id="d2e4159">The relatively high [NO<inline-formula><mml:math id="M328" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> during the glacial period (Fig. 4c), before its decline in Heinrich Stadial 1, is likely indicative of reduced water-column denitrification (Ganeshram et al., 1995, 2000) due to reduced productivity (Ganeshram et al., 1995; Ganeshram and Pedersen, 1998) and low organic matter flux through the oxygen minimum zone (Ganeshram et al., 2000). In the ETNP, including the Mexican Margin, coastal upwelling is driven by trade winds generated by subtropical high-pressure centers. These high-pressure centers largely result from differential heating of the land and the ocean. As a result of glacial cooling on land, these high-pressure systems and the associated trade winds that drive the upwelling have likely been weakened (Ganeshram and Pedersen, 1998).</p>
</sec>
<sec id="Ch1.S4.SS4">
  <label>4.4</label><title>Gulf of Guayaquil</title>
      <p id="d2e4192">The core M77/2-59-01 is in a region that is sensitive to changes in subsurface denitrification in the ETSP (Robinson et al., 2007, 2009; Dubois et al., 2011, 2014). The elevated reconstructed [NO<inline-formula><mml:math id="M330" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> levels (Fig. 4d) during the glacial period suggest decreased water-column denitrification (Salvatteci et al., 2014; Erdem et al., 2020; Glock et al., 2022) and relatively low local productivity (Ganeshram et al., 2000; Robinson et al 2007, 2009; Martinez and Robinson et al., 2010; Salvatteci et al., 2016). Nutrient export to the deep Southern Ocean waters increased due to the sluggish Atlantic Meridional Overturning Circulation (Skinner et al., 2010), and increased atmospheric iron (Fe) deposition (Somes et al., 2017) during the glacial period. This reduced the transport of preformed NO<inline-formula><mml:math id="M332" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> to the tropics via the Subantarctic Mode Water (SAMW), limiting productivity. In fact, the total organic carbon (Fig. 4d) depicts low productivity during this period. Furthermore, the colder sea surface temperature (SST) and the accelerated formation of SAMW and Antarctic Intermediate Water masses (Russell and Dickson, 2003; Galbraith et al., 2004) and the stronger high-latitude winds in the Southern Hemisphere (Karstensen and Quadfasel, 2002) increased the ventilation rate (Meissner et al., 2005; Jaccard and Galbraith, 2012; Muratli et al., 2010) during the glacial period. The resulting increased oxygen concentrations (Robinson et al., 2005; Robinson et al., 2007) decreased the volume of ODZs, and nitrogen loss processes (lower <inline-formula><mml:math id="M333" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values, Fig. 4d) during the glacial period. In addition, enhanced Fe deposition (Somes et al., 2017), and the glacial low sea level (Clark and Mix, 2002; Wallmann et al., 2016), may have influenced the nitrate inventory in the tropical and subtropical southern hemisphere.</p>
      <p id="d2e4248">A study by Glock et al. (2018) on core M77/2-52-2 from Peru applying the pore density of <italic>B. spissa</italic> also shows elevated [NO<inline-formula><mml:math id="M335" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> during the Last Glacial Maximum, a similar decline in [NO<inline-formula><mml:math id="M337" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> during the Heinrich Stadial 1 and thereafter a steady decrease in [NO<inline-formula><mml:math id="M339" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> throughout the Holocene.</p>
      <p id="d2e4318">The deglacial decline in [NO<inline-formula><mml:math id="M341" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub>, especially during Heinrich Stadial 1 in this study (Fig. 4d), indicates a gradual increase in surface productivity and bottom-water deoxygenation. High export production strengthened the expansion of the ETSP ODZ during the deglaciation as compared to LGM and MLH (Salvatteci et al., 2016; Glock et al., 2018; Mollier-Vogel et al., 2019). This is consistent with the denitrification signal in the Eastern Equatorial Pacific through westward advection from the Southeast Pacific margins (Martinez and Robinson, 2010).</p>
      <p id="d2e4342">The shift towards generally higher reconstructed [NO<inline-formula><mml:math id="M343" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> from the Middle-Holocene, (Fig. 4d), implies a profound change in the climatic state of the Peruvian upwelling system and the associated ODZ during this time. From the deglaciation toward the Late Holocene, there was a general increase in productivity (Mollier-Vogel et al., 2019) as shown by organic carbon accumulation rates (Fig. 4d). This increase in organic matter input and/or preservation was likely related to an increase in upwelling-driven delivery of nutrients towards the surface. The gradual decrease in <inline-formula><mml:math id="M345" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N<sub>bulk</sub> values and higher [NO<inline-formula><mml:math id="M347" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> was  likely related  to a relaxation in nutrient utilization with a nutrient supply exceeding the biological demand (Riechelson et al., 2024). Moreover, the core M77/2-59-01 was retrieved outside of the core ODZ and is under the strong influence of the oxygen and nutrient-rich Equatorial Under Current subsurface waters (Salvatteci et al., 2019; Mollier-Vogel et al., 2019). These waters might have ventilated the Northern Peruvian margin and deepened the oxycline at this site during the Middle-Holocene. Furthermore, enhanced zonal SST (Koutavas et al., 2006) and a northward shift of the ITCZ strengthened the Pacific Walker and Hadley circulation during the Middle-Holocene across the tropical Pacific (Koutavas et al., 2006; Mollier-Vogel et al., 2013; Salvatteci et al., 2019). These enhanced atmospheric circulations brought oxygen-rich waters to intermediate depths off Peru via the equatorial subsurface countercurrents (Koutavas et al., 2006; Mollier-Vogel et al., 2013; Salvatteci et al., 2019). Hence, increased ventilation of subsurface water masses reduced the strength of nitrogen loss processes and nutrient uptake during the MLH.</p>
      <p id="d2e4409">At present, the only quantitative reconstruction of bottom-water oxygen from these locations is the core M77/2-59-01 from the Gulf of Guayaquil reported by Erdem et al. (2020). Their record suggests a decline in bottom-water oxygen from the deglacial period to the Holocene. Future more detailed comparisons of the nitrate reconstructions with quantitative bottom water oxygen records at the same cores will further improve our understanding about variability in redox conditions and nitrogen cycling.</p>
</sec>
<sec id="Ch1.S4.SS5">
  <label>4.5</label><title>Comparison of past and present [NO<inline-formula><mml:math id="M349" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] at the studied locations</title>
      <p id="d2e4433">The [NO<inline-formula><mml:math id="M350" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] during the present and past are compared to assess the resilience of our chosen study locations towards environmental and ecological impacts of climate change. The generally positive <inline-formula><mml:math id="M351" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>[NO<inline-formula><mml:math id="M352" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] that we found (Fig. 4b) in the Gulf of California (Guaymas Basin) and the Gulf of Guayaquil indicate that today the [NO<inline-formula><mml:math id="M353" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]  is lower than in the past. This suggests that today the nitrogen loss processes at these two core sites are stronger, most likely related to ocean warming and a decline in oxygen concentration of bottom waters. The Gulf of California core is within the heart of the oxygen-deficient zone, and thus changes in ODZ oxygenation or denitrification will be more evident in this core than in any other core studied. Under nitrogen limitation, negative feedbacks (e.g., anammox) result in a decline in productivity (Naafs et al., 2019; Wallmann et al., 2022), which will stabilize the oxygen concentration. In the case of the Gulf of California, sediments are enriched in reactive iron (Fe) (Scholz et al., 2019). The decreasing NO<inline-formula><mml:math id="M354" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations in the bottom water reduce the flux of NO<inline-formula><mml:math id="M355" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> into the surface sediment. This leads to the release of sedimentary Fe, which enhances nitrogen fixation in the Guaymas Basin (Scholz et al., 2019). Thus, increased denitrification might not act as negative feedback in the Gulf of California because it might be countered by increased nitrogen fixation (White et al., 2013).</p>
      <p id="d2e4504">In the case of the Gulf of Guayaquil (Fig. 4d), whether today's elevated denitrification could enhance N<sub>2</sub> fixation also depends on the availability of Fe (Pennington et al., 2006). The primary productivity of the Peruvian ODZ is Fe limited due to the reduction of particular Fe oxides in shelf and slope sediments (Scholz et al., 2014). Modeling studies show that primary productivity will be amplified in the Peruvian ODZ due to the release of Fe from shelf and slope sediments (Wallmann et al., 2022). This may induce deoxygenation and drive the expansion and intensification of Peruvian ODZ resulting in a positive feedback loop, like in the Gulf of California. This situation is indicated by lower [NO<inline-formula><mml:math id="M357" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] today compared to the past <inline-formula><mml:math id="M358" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 20 000 years.</p>
      <p id="d2e4535">The negative nitrate <inline-formula><mml:math id="M359" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>[NO<inline-formula><mml:math id="M360" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] in the Sea of Okhotsk and the Mexican Margin (Fig. 4a and c) indicates that modern [NO<inline-formula><mml:math id="M361" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] levels are higher than in the reconstructed past. This suggests that modern nitrogen loss is decreased at these two core sites compared to the last deglaciation. The higher modern [NO<inline-formula><mml:math id="M362" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] in the Sea of Okhotsk is likely associated with less primary productivity and more oxygen in the water column similar to the situation established in the MLH. The higher modern [NO<inline-formula><mml:math id="M363" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> in the case of the Mexican Margin could be associated with sea level rise. The ODZ in the Mexican Continental Margin might have shifted to shallower depths today with less/or no benthic denitrification in intermediate water depths at the core site, resulting in high [NO<inline-formula><mml:math id="M365" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> levels. During the glacial period, continental shelves were exposed due to sea-level lowstands (Clark and Mix, 2002; Kuhlmann et al., 2004; Wallmann et al., 2016), the main areas of primary productivity may have migrated offshore from the shallow shelf towards the continental slope relative to their Holocene positions. A similar situation occurred at the Benguela upwelling system during the LGM: TOC accumulation at the continental slope increased during the LGM in response to the seaward shift of centers of enhanced productivity (Mollenhauer et al., 2002). This offshore shift of the productivity centers and the most likely reduced remineralization rates, due to lower temperatures, indicate that the center of the ODZ at the Mexican Margin before sea level rise was possibly deeper than today. However, with the deglacial eustatic sea-level rise, the ODZ may have shifted to shallower depths. This shifted the main zone of denitrification further away from the seafloor, resulting in the increased modern [NO<inline-formula><mml:math id="M367" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> in comparison to the LGM.</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions</title>
      <p id="d2e4655">The quantitative reconstruction of [NO<inline-formula><mml:math id="M369" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> using the pore density of denitrifying benthic foraminifera over the last deglaciation at the four studied ODZs provides a comprehensive understanding of the past [NO<inline-formula><mml:math id="M371" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]. The Gulf of Guayaquil and Gulf of California data shows elevated [NO<inline-formula><mml:math id="M372" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> during the glacial period compared to deglacial and modern conditions. Considering the well-ventilated intermediate water masses in the Sea of Okhotsk, the Sea of Okhotsk may have also elevated [NO<inline-formula><mml:math id="M374" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> in the glacial period. For the Mexican Margin core, [NO<inline-formula><mml:math id="M376" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> was particularly strong during the Younger Dryas. The reconstructed [NO<inline-formula><mml:math id="M378" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> from the Sea of Okhotsk, the Gulf of California, and the Gulf of Guayaquil are influenced by the formation of the North Pacific Intermediate Water. However, the [NO<inline-formula><mml:math id="M380" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>]<sub>BW</sub> in the deeper site, the Mexican Margin is likely influenced by the NO<inline-formula><mml:math id="M382" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> variability in Pacific Deep Water. The modern Gulf of Guayaquil and the Gulf of California have low [NO<inline-formula><mml:math id="M383" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] associated with increased denitrification and a strengthening ODZ. In contrast, higher modern [NO<inline-formula><mml:math id="M384" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>] was observed in the Sea of Okhotsk and the Mexican Margin, suggesting that these two study areas have higher oxygen.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d2e4838">All data generated or analyzed during this study are available in the Supplement.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e4841">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/cp-21-1853-2025-supplement" xlink:title="pdf">https://doi.org/10.5194/cp-21-1853-2025-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e4850">A.G.M wrote the core manuscript, did the sample preparation, electron microscopy, image and statistical analyses of all the fossil foraminifera. N.G. planned the study design and sampling strategy. G.S. hosted the research group, and provided access to SEM, and lab facilities at the University of Hamburg. D.N. provided sampling material for cores MD01-2415 and M77/2-59-01. C.D. provided sampling material for core MAZ-1E-04. N.L., R.S., and A.B. facilitated the measurement of nitrogen isotopes in the sediment samples of core MD01-2415 and DSDP-480. R.A. contributed to the age model development of core MAZ-1E-04, and H.F helped in the image processing of core DSDP-480. All authors contributed to the discussion and preparation of the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e4856">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e4862">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e4868">We are grateful to the micropaleontology group at the University of Hamburg, Germany. We thank Alfredo Martinez-Garcia, Max Planck Institute for Chemistry, Mainz, Germany for the support with the measurement of nitrogen isotopes in the sediment samples. We acknowledge the help of Jutta Richarz, Kaya Oda for lab support, PhD student Sven Brömme (Max Planck Institute for Chemistry, Mainz) and student assistant Hannah Krüger. We thank Yvon Balut, Agnes Baltzer, and the Shipboard Scientific Party of RV Marion Dufresne cruise WEPAMA 2001 for their kind support. We thank IODP for providing the sample for core DSDP-480. The study is a contribution to the Center for Earth System Research and Sustainability (CEN) of University of Hamburg.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e4873">Funding was provided by the Deutsche Forschungsgemeinschaft (DFG) through both N.G.'s Heisenberg grant GL 999/3-1 and grant GL 999/4-1. Funding for the core MD01-2415 recovery was provided by the German Science Foundation (DFG) within project Ti240/11-1. The recovery of core M77-59 recovery was a contribution of the German Science Foundation (DFG) Collaborative Research Project “Climate–Biogeochemistry interactions in the Tropical Ocean” (SFB 754).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e4879">This paper was edited by Luc Beaufort and reviewed by two anonymous referees.</p>
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