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<front>
<journal-meta>
<journal-id journal-id-type="publisher">EGUsphere</journal-id>
<journal-title-group>
<journal-title>EGUsphere</journal-title>
<abbrev-journal-title abbrev-type="publisher">EGUsphere</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">EGUsphere</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub"></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/egusphere-2022-1323</article-id>
<title-group>
<article-title>Unraveling the burial and exhumation history of foreland basins using the spread of apatite (U-Th-Sm)/He single grain ages</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Frings</surname>
<given-names>Kevin Alexander</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Luijendijk</surname>
<given-names>Elco</given-names>
<ext-link>https://orcid.org/0000-0003-4140-2455</ext-link>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Dunkl</surname>
<given-names>István</given-names>
<ext-link>https://orcid.org/0000-0001-8438-2867</ext-link>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kukla</surname>
<given-names>Peter</given-names>
<ext-link>https://orcid.org/0000-0001-8847-4435</ext-link>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Villamizar-Escalante</surname>
<given-names>Nicolas</given-names>
<ext-link>https://orcid.org/0000-0003-0951-4473</ext-link>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Madritsch</surname>
<given-names>Herfried</given-names>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
<xref ref-type="aff" rid="aff7">
<sup>7</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>von Hagke</surname>
<given-names>Christoph</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Institute for Tectonics and Geodynamics, RWTH Aachen University, Aachen, 52064, Germany</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Department of Environment and Biodiversity, Division of Geology &amp; Physical Geography, Salzburg University PLUS, Salzburg, 5020, Austria</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Department of Earth Science, University of Bergen, Bergen, 5020, Norway</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Geoscience Center, Department of Sedimentology and Environmental Geology, University of Göttingen, Göttingen, 37077, Germany</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Geological Institute, RWTH Aachen University, Aachen, 52062, Germany</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>Nagra, Wettingen, 5430, Switzerland</addr-line>
</aff>
<aff id="aff7">
<label>7</label>
<addr-line>now at: Swisstopo, Swiss Geological Survey, Seftigenstrasse 264, 3084 Wabern</addr-line>
</aff>
<pub-date pub-type="epub">
<day>05</day>
<month>12</month>
<year>2022</year>
</pub-date>
<volume>2022</volume>
<fpage>1</fpage>
<lpage>51</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2022 Kevin Alexander Frings et al.</copyright-statement>
<copyright-year>2022</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://egusphere.copernicus.org/preprints/2022/egusphere-2022-1323/">This article is available from https://egusphere.copernicus.org/preprints/2022/egusphere-2022-1323/</self-uri>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2022/egusphere-2022-1323/egusphere-2022-1323.pdf">The full text article is available as a PDF file from https://egusphere.copernicus.org/preprints/2022/egusphere-2022-1323/egusphere-2022-1323.pdf</self-uri>
<abstract>
<p>&lt;p&gt;Reconstructing the evolution of foreland basins that experienced late exhumation is challenging due to an incomplete sedimentary record. Thermochronometry has been applied successfully to reconstruct basin evolution, but the method is subject to uncertainties. For the Swiss Molasse Basin, a wide range of exhumation magnitude and timing has been proposed based on thermochronometry. We aim to reduce uncertainty by dating larger numbers of grains and samples, to obtain statistically more robust data. New apatite (U-Th-Sm)/He (AHe) data from a single borehole shows ages of 4 to 30 Ma in the upper 500 meters and ages of 3 to 80 Ma below 1300 meters. This is counterintuitive as a total reset is expected at depths exceeding approximately 600 m. To arrive at a single consistent thermal history including our and previously published data, we conduct thermal modeling with different software. In particular we test the influence of different provenance histories and distinguish between cooling associated with changes in heat flow vs changes in exhumation.&lt;/p&gt;
&lt;p&gt;We determine 1050 m +/- 100 m of exhumation, starting slowly at 13 Ma and accelerating at 9 Ma. Coinciding with exhumation, heat flow begins to rise sharply, causing heating until 5 Ma, despite ongoing exhumation. We show that this discrepancy between start of exhumation and start of cooling is the main reason for differing estimates for the burial and exhumation history of the basin. We suggest that the remaining misfit between modeled and measured Molasse AHe ages can be explained by post-Miocene hydrothermal flux in the Neogene sediment fill above a sealing layer, potentially the Opalinus Clay or Triassic evaporites.&lt;/p&gt;
&lt;p&gt;In summary, we show that a single consistent model for basin exhumation relies on large sets of grains and samples, as well as inclusion of provenance ages in the models. With timing of the main exhumation phase constrained to start at 9 Ma, we can rule out a 5 Ma climatic event as exhumation driver. As the region is not affected by extensive faulting, deep seated processes related to mantle dynamics remain as exhumation driving process.&lt;/p&gt;</p>
</abstract>
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