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	<journal>
		<journal_title>Climate of the Past Discussions</journal_title>
		<journal_url>www.clim-past-discuss.net</journal_url>
		<issn>1814-9340</issn>
		<eissn>1814-9359</eissn>
		<volume_number>3</volume_number>
		<issue_number>1</issue_number>
		<publication_year>2007</publication_year>
	</journal>
	<doi>10.5194/cpd-3-63-2007</doi>
	<article_url>http://www.clim-past-discuss.net/3/63/2007/</article_url>
	<abstract_html>http://www.clim-past-discuss.net/3/63/2007/cpd-3-63-2007.html</abstract_html>
	<fulltext_pdf>http://www.clim-past-discuss.net/3/63/2007/cpd-3-63-2007.pdf</fulltext_pdf>
	<start_page>63</start_page>
	<end_page>93</end_page>
	<publication_date>2007-01-16</publication_date>
	<article_title content_type="html">Anomalous flow below 2700 m in the EPICA Dome C ice core detected using &amp;delta;&lt;sup&gt;18&lt;/sup&gt;O of atmospheric oxygen measurements</article_title>
	<authors>
		<author numeration="1" affiliations="1,2">
			<name>G. B. Dreyfus</name>
			<email>gabrielle.dreyfus@cea.fr</email>
		</author>
		<author numeration="2" affiliations="3">
			<name>F. Parrenin</name>
		</author>
		<author numeration="3" affiliations="3">
			<name>B. Lemieux-Dudon</name>
		</author>
		<author numeration="4" affiliations="4">
			<name>G. Durand</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>V. Masson-Delmotte</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>J. Jouzel</name>
		</author>
		<author numeration="7" affiliations="3">
			<name>J.-M. Barnola</name>
		</author>
		<author numeration="8" affiliations="5">
			<name>L. Panno</name>
		</author>
		<author numeration="9" affiliations="5">
			<name>R. Spahni</name>
		</author>
		<author numeration="10" affiliations="6">
			<name>A. Tisserand</name>
		</author>
		<author numeration="11" affiliations="5">
			<name>U. Siegenthaler</name>
		</author>
		<author numeration="12" affiliations="5">
			<name>M. Leuenberger</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">LSCE/IPSL, CEA-CNRS-UVSQ, CE Saclay, 91191, Gif-sur-Yvette, France</affiliation>
		<affiliation numeration="2" content_type="html">Department of Geosciences, Princeton University, Princeton, New Jersey, USA</affiliation>
		<affiliation numeration="3" content_type="html">Laboratoire de Glaciologie et Geophysique de l&apos;Environnement (CNRS), St Martin d&apos;Heres, France</affiliation>
		<affiliation numeration="4" content_type="html">Niels Bohr Institute for Astronomy, Physics and Geophysics, University of Copenhagen, Copenhagen, Denmark</affiliation>
		<affiliation numeration="5" content_type="html">Physics Institute, University of Bern, Bern, Switzerland</affiliation>
		<affiliation numeration="6" content_type="html">Université Bordeaux I, UMR 5805 EPOC, Environnements et Paleoenvironnements Océaniques et Côtiers, Talence Cedex 33405, France</affiliation>
	</affiliations>
	<abstract content_type="html">While there are no indications of mixing back to 800 000 years in the EPICA
Dome C ice core record, comparison with marine sediment records shows
significant differences in the timing and duration of events prior to stage
11 (~430 ka, thousand of years before 1950). A relationship between
the isotopic composition of atmospheric oxygen (&amp;delta;&lt;sup&gt;18&lt;/sup&gt;O of
O&lt;sub&gt;2&lt;/sub&gt;, noted &amp;delta;&lt;sup&gt;18&lt;/sup&gt;O&lt;sub&gt;atm&lt;/sub&gt;) and daily northern hemisphere
summer insolation has been observed for the youngest four climate cycles.
Here we use this relationship with new &amp;delta;&lt;sup&gt;18&lt;/sup&gt;O of O&lt;sub&gt;2&lt;/sub&gt;
measurements to show that anomalous flow in the bottom 500 m of the core
distorts the duration of events by up to a factor of 2. By tuning &amp;delta;&lt;sup&gt;18&lt;/sup&gt;O&lt;sub&gt;atm&lt;/sub&gt; to orbital precession we derive a corrected thinning
function and present a revised age scale for the interval corresponding to
Marine Isotope Stages 11&amp;ndash;20 in the EPICA Dome C ice core. Uncertainty in the
phasing of &amp;delta;&lt;sup&gt;18&lt;/sup&gt;O&lt;sub&gt;atm&lt;/sub&gt; with respect to insolation variations
in the precession band limits the accuracy of this new agescale to &amp;plusmn;6 kyr (thousand of years). The previously reported ~30 kyr duration of
interglacial stage 11 is unchanged. In contrast, the duration of stage 15.1
is reduced by a factor of 2, from 31 to 16 kyr.</abstract>
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