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      <header>
        <identifier>doi:10.1594/pangaea.741863</identifier>
        <datestamp>2024-08-16T05:32:43Z</datestamp>
        <setSpec>PANGAEA</setSpec>
        <setSpec>PANGAEA.REPOSITORY</setSpec>
      </header>
      <metadata>
        <oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
          <dc:title>Isotope measurements from late Paleocene - early Eocene of 5 cores from Atlantic and Pacific Ocean</dc:title>
          <dc:creator>Cramer, Benjamin S</dc:creator>
          <dc:creator>Wright, James D</dc:creator>
          <dc:creator>Kent, Dennis V</dc:creator>
          <dc:creator>Aubry, Marie-Pierre</dc:creator>
          <dc:publisher>PANGAEA</dc:publisher>
          <dc:date>2003</dc:date>
          <dc:date>Issued: 2003</dc:date>
          <dc:relation>doi:10.1029/2003pa000909</dc:relation>
          <dc:subject>Drilling/drill rig</dc:subject>
          <dc:subject>Leg80</dc:subject>
          <dc:subject>Leg86</dc:subject>
          <dc:subject>Leg113</dc:subject>
          <dc:subject>Leg171B</dc:subject>
          <dc:subject>Glomar Challenger</dc:subject>
          <dc:subject>Joides Resolution</dc:subject>
          <dc:subject>Deep Sea Drilling Project (DSDP)</dc:subject>
          <dc:subject>Ocean Drilling Program (ODP)</dc:subject>
          <dc:description>High-resolution stable carbon isotope records for upper Paleocene - lower Eocene sections at Ocean Drilling Program Sites 1051 and 690 and Deep Sea Drilling Project Sites 550 and 577 show numerous rapid (40 - 60 kyr duration) negative excursions of up to 1 per mill. We demonstrate that these transient decreases are the expected result of nonlinear insolation forcing of the carbon cycle in the context of a long carbon residence time. The transients occur at maxima in Earth's orbital eccentricity, which result in high-amplitude variations in insolation due to forcing by climatic precession. The construction of accurate orbital chronologies for geologic sections older than ~ 35 Ma relies on identifying a high-fidelity recorder of variations in Earth's orbital eccentricity. We use the carbon isotope records as such a recorder, establishing a robust orbitally tuned chronology for latest Paleocene-earliest Eocene events. Moreover, the transient decreases provide a means of precise correlation among the four sites that is independent of magnetostratigraphic and biostratigraphic data at the &amp;lt;10^5-year scale. While the eccentricity-controlled transient decreases bear some resemblance to the much larger-amplitude carbon isotope excursion (CIE) that marks the Paleocene/Eocene boundary, the latter event is found to occur near a minimum in the ~400-kyr eccentricity cycle. Thus the CIE occurred during a time of minimal variability in insolation, the dominant mechanism for forcing climate change on 104-year scales. We argue that this is inconsistent with mechanisms that rely on a threshold climate event to trigger the Paleocene/Eocene thermal maximum since any threshold would more likely be crossed during a period of high-amplitude climate variations.</dc:description>
          <dc:description>Supplement to: Cramer, Benjamin S; Wright, James D; Kent, Dennis V; Aubry, Marie-Pierre (2003): Orbital climate forcing of d13C excursions in the late Paleocene-early Eocene (chrons C24n–C25n). Paleoceanography, 18(4), 1097</dc:description>
          <dc:language>en</dc:language>
          <dc:type>Collection</dc:type>
          <dc:type>Supplementary Publication Series of Datasets</dc:type>
          <dc:format>application/zip</dc:format>
          <dc:rights>Creative Commons Attribution 3.0 Unported</dc:rights>
          <dc:rights>https://creativecommons.org/licenses/by/3.0/legalcode</dc:rights>
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