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		<title>Latest on the absolute age of the Paleocene–Eocene Thermal Maximum (PETM): New insights from exact stratigraphic position of key ash layers +19 and −17</title>
		<link>http://earthtime-eu.eu/earthtime/?p=486</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=486#comments</comments>
		<pubDate>Thu, 26 Nov 2009 18:40:23 +0000</pubDate>
		<dc:creator>heiko</dc:creator>
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		<description><![CDATA[Westerhold, T, Röhl, U., McKarren, H.K., Zachos, J.C. (2009), Latest on the absolute age of the Paleocene–Eocene Thermal Maximum (PETM): New insights from exact stratigraphic position of key ash layers +19 and −17, Earth and Planetary Science Letters 287, 412–419, doi:10.1016/j.epsl.2009.08.027.

Abstract
We constructed a precise early Eocene orbital cyclostratigraphy for DSDP Site 550 (Leg 80, Goban Spur, North [...]]]></description>
			<content:encoded><![CDATA[<p style="margin: 0.0px 0.0px 0.0px 0.0px; font: 13.4px Times; color: #221e20;">Westerhold, T, Röhl, U., McKarren, H.K., Zachos, J.C. (2009), Latest on the absolute age of the Paleocene–Eocene Thermal Maximum (PETM): New insights from exact stratigraphic position of key ash layers +19 and −17, Earth and Planetary Science Letters 287, 412–419, doi:<a style="color: #666666; font-weight: bold; text-decoration: none;" title="http://dx.doi.org/10.1016/j.epsl.2009.08.027" href="http://dx.doi.org/10.1016/j.epsl.2009.08.027" target="_blank">10.1016/j.epsl.2009.08.027</a>.</p>
<p style="margin: 0.0px 0.0px 0.0px 0.0px; font: 13.4px Times; color: #221e20;">
<p>Abstract</p>
<p>We constructed a precise early Eocene orbital cyclostratigraphy for DSDP Site 550 (Leg 80, Goban Spur, North Atlantic) utilizing precession related cycles as represented in a high-resolution X-ray <span style="font: 7.2px Helvetica;"><span style="font-family: Georgia, 'Times New Roman', 'Bitstream Charter', Times, serif; font-size: small;"><span style="line-height: 19px;">fl</span></span></span>uorescence based barium core log. Based on counting of those cycles, we constrain the exact timing of two volcanic ash layers in Site 550 which correlate to ashes +19 and <span style="font: 7.2px Helvetica;"><span style="font-family: Georgia, 'Times New Roman', 'Bitstream Charter', Times, serif; font-size: small;"><span style="line-height: 19px;">−</span></span></span>17 of the Fur Formation in Denmark. The ashes, relative to the onset of the Paleocene<span style="font: 7.2px Helvetica;"><span style="font-family: Georgia, 'Times New Roman', 'Bitstream Charter', Times, serif; font-size: small;"><span style="line-height: 19px;">–</span></span></span>Eocene Thermal Maximum (PETM), are offset by 862 kyr and 672 kyr, respectively. When combined with published absolute ages for ash <span style="font: 7.2px Helvetica;"><span style="font-family: Georgia, 'Times New Roman', 'Bitstream Charter', Times, serif; font-size: small;"><span style="line-height: 19px;">−</span></span></span>17, the absolute age for the onset of the PETM is consistent with astronomically calibrated ages. Using the current absolute age of 28.02 Ma for the Fish Canyon Tuff (FCT) standard for calibrating the absolute age of ash <span style="font: 7.2px Helvetica;"><span style="font-family: Georgia, 'Times New Roman', 'Bitstream Charter', Times, serif; font-size: small;"><span style="line-height: 19px;">−</span></span></span>17 is consistent with tuning option 2 in the astronomically calibrated Paleocene time scale of Westerhold et al. (2008) [Westerhold, T., Röhl, U., Raf<span style="font: 7.2px Helvetica;"><span style="font-family: Georgia, 'Times New Roman', 'Bitstream Charter', Times, serif; font-size: small;"><span style="line-height: 19px;">fi</span></span></span>, I., Fornaciari, E., Monechi, S., Reale, V., Bowles, J., and Evans, H.F., 2008, Astronomical calibration of the Paleocene time: Palaeogeography, Palaeoclimatology, Palaeoecology, v. 257, p. 377<span style="font: 7.2px Helvetica;"><span style="font-family: Georgia, 'Times New Roman', 'Bitstream Charter', Times, serif; font-size: small;"><span style="line-height: 19px;">–</span></span></span>403]. Using the recently recalibrated absolute age of 28.201 Ma for the FCT standard is consistent with tuning option 3 in the astronomically calibrated Paleocene time scale. The new results do not support the existence of any additional 405-kyr cycle in the early Paleocene astronomically tuned time scale.</p>
<p>© 2009 Elsevier B.V. All rights reserved.</p>
<pre></pre>
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		<title>High resolution cyclostratigraphy of the early Eocene</title>
		<link>http://earthtime-eu.eu/earthtime/?p=464</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=464#comments</comments>
		<pubDate>Mon, 06 Jul 2009 12:00:24 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Cyclostratigraphy]]></category>
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		<description><![CDATA[Clim. Past, 5, 309-327, 2009
www.clim-past.net/5/309/2009/
© Author(s) 2009. This work is distributed
under the Creative Commons Attribution 3.0 License.
High resolution cyclostratigraphy of the early Eocene – new insights into the origin of the Cenozoic cooling trend
T. Westerhold and U. Röhl
MARUM – Center for Marine Environmental Sciences, University of Bremen, Leobener Strasse, 28359 Bremen, Germany

Abstract. Here we present a high-resolution [...]]]></description>
			<content:encoded><![CDATA[<p><span style="font-size: 11px; font-family: Verdana, Arial, Helvetica; font-weight: normal; color: #000000;">Clim. Past, 5, 309-327, 2009<br />
www.clim-past.net/5/309/2009/<br />
© Author(s) 2009. This work is distributed<br />
under the Creative Commons Attribution 3.0 License.</span></p>
<p><span style="font-size: 16px; font-family: Verdana, Arial, Helvetica; font-weight: bold; color: #000000; line-height: normal;">High resolution cyclostratigraphy of the early Eocene – new insights into the origin of the Cenozoic cooling trend</span></p>
<p><span style="font-size: 12px; font-family: Verdana, Arial, Helvetica; font-weight: bold; color: #000000;">T. Westerhold and U. Röhl</span><br />
<span style="font-size: 11px; font-family: Verdana, Arial, Helvetica; font-weight: normal; color: #000000;">MARUM – Center for Marine Environmental Sciences, University of Bremen, Leobener Strasse, 28359 Bremen, Germany<br />
</span><br />
<span style="font-size: 12px; font-family: Verdana, Arial, Helvetica; font-weight: normal; color: #000000; line-height: 20px;"><span style="font-weight: bold;">Abstract.</span> Here we present a high-resolution cyclostratigraphy based on X-ray fluorescence (XRF) core scanning data from a new record retrieved from the tropical western Atlantic (Demerara Rise, ODP Leg 207, Site 1258). The Eocene sediments from ODP Site 1258 cover magnetochrons C20 to C24 and show well developed cycles. This record includes the missing interval for reevaluating the early Eocene part of the Geomagnetic Polarity Time Scale (GPTS), also providing key aspects for reconstructing high-resolution climate variability during the Early Eocene Climatic Optimum (EECO). Detailed spectral analysis demonstrates that early Eocene sedimentary cycles are characterized by precession frequencies modulated by short (100 kyr) and long (405 kyr) eccentricity with a generally minor obliquity component. Counting of both the precession and eccentricity cycles results in revised estimates for the duration of magnetochrons C21r through C24n. Our cyclostratigraphic framework also corroborates that the geochronology of the Eocene Green River Formation (Wyoming, USA) is still questionable mainly due to the uncertain correlation of the &#8220;Sixth tuff&#8221; to the GPTS.</span></p>
<p>Right at the onset of the long-term Cenozoic cooling trend the dominant eccentricity-modulated precession cycles of ODP Site 1258 are interrupted by strong obliquity cycles for a period of ~800 kyr in the middle of magnetochron C22r. These distinct obliquity cycles at this low latitude site point to (1) a high-latitude driving mechanism on global climate variability from 50.1 to 49.4 Ma, and (2) seem to coincide with a significant drop in atmospheric CO<sub>2</sub>concentration below a critical threshold between 2- and 3-times the pre-industrial level (PAL). The here newly identified orbital configuration of low eccentricity in combination with high obliquity amplitudes during this ~800-kyr period and the crossing of a critical <em>p</em>CO<sub>2</sub> threshold may have led to the formation of the first ephemeral ice sheet on Antarctica as early as ~50 Ma ago.<span style="font-size: 12px; font-family: Verdana, Arial, Helvetica; font-weight: normal; color: #000000;"><br />
</span></p>
<p><a href="http://www.clim-past.net/5/309/2009/cp-5-309-2009.html" target="_blank">http://www.clim-past.net/5/309/2009/cp-5-309-2009.html</a></p>
<p><a href="http://earthtime-eu.eu/earthtime/wp-content/uploads/2009/07/WR2009.png"><img class="aligncenter size-full wp-image-465" title="WR2009" src="http://earthtime-eu.eu/earthtime/wp-content/uploads/2009/07/WR2009.png" alt="WR2009" width="708" height="444" /></a></p>
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		<title>Correspondence: Rock clock synchronization</title>
		<link>http://earthtime-eu.eu/earthtime/?p=330</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=330#comments</comments>
		<pubDate>Fri, 02 May 2008 12:52:15 +0000</pubDate>
		<dc:creator>admin</dc:creator>
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		<description><![CDATA[Heiko Pälike and Frits Hilgen, Correspondence to Nature Geoscience (2008), Vol 1 (5), p. 282, doi:10.1038/ngeo197
To the EditorThe need for much improved knowledge of the durations and ages of climatic and geological events, such as the Palaeocene–Eocene Thermal Maximum (55 million years ago), has become urgent within the Earth science and climate modelling communities. The [...]]]></description>
			<content:encoded><![CDATA[<p><a href="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Entries/2008/5/2_Correspondence%3A_Rock_clock_synchronization_files/May08CorrPalike_Fig1_published.pdf"><img src="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Media/May08CorrPalike_Fig1_revised.png" style="float:left; padding-right:10px; padding-bottom:10px; width:228px; height:166px;"/></a>Heiko Pälike and Frits Hilgen, Correspondence to Nature Geoscience (2008), Vol 1 (5), p. 282, <a href="http://dx.doi.org/10.1038/ngeo197">doi:10.1038/ngeo197</a></p>
<p>To the Editor<br />The need for much improved knowledge of the durations and ages of climatic and geological events, such as the Palaeocene–Eocene Thermal Maximum (55 million years ago), has become urgent within the Earth science and climate modelling communities. The exact dating and timing of fluxes into and out of the marine carbon reservoir can differentiate between competing hypotheses of climatic change. Highly detailed reconstructions of the Earth&#8217;s history allow us to assess whether past climatic change can be used as an analogue for the current and future change of ocean acidification and climate. The Earthtime project is an international effort with the goal to further this quest for a well calibrated and stable timescale that will allow more precise dating of rock layers and minerals<a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523B1">1</a>.<br />Radioisotopic dating methods have small but significant errors that hinder our ability to assess geologically short-lived climate events. For instance, the most widely used method for the Cenozoic era is 40Ar/39 Ar, which has an error of up to 2.5% and few tie points of known age. Yet, over the last two decades much progress has been made in exploiting the imprint of the Earth&#8217;s orbital variations in palaeoclimatic records. This has dramatically increased the potential age resolution of approaches like cycle-counting and pattern matching, to less than 40,000 years throughout much of Cenozoic time (the past 66 million years, <a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523f1">Fig. 1</a>).<br />Unfortunately, there have been a number of inconsistencies and discrepancies between ages and durations derived from radioisotopic and astronomical dating. What is now needed is a more systematic and coordinated approach to provide a detailed intercalibration of radioisotopic clocks (U–Pb, Ar–Ar methods), the rock standards that are used for these methods, and geological tie-points with astronomical ages. At the same time, Cenozoic palaeoclimatic compilations need to be improved by closing existing gaps, verifying data from single sites and supplementing the database of magneto- and biostratigraphy so we can improve the accuracy of existing age calibrations.<br />In particular, a major advance towards a fully astronomically calibrated geological timescale needs to be accomplished in the middle Eocene epoch (40 to 50 million years). Very few suitable sections have been acquired so far for this period, presumably because the calcite compensation depth was very shallow during this time, which would have prevented the preservation of carbonate material in the deep-ocean marine sediments.<br />The Earthtime projects are open community efforts aimed at improving intercalibration between astronomical and radioisotope dating methods by finding ash layers that can be dated with radioisotopes within astronomically age-calibrated sections. The immediate aim is to arrive at a highly accurate and stable Cenozoic timescale.<br />REFERENCES<br />	1.	<a href="http://earthtime-eu.eu/">http://earthtime-eu.eu</a>; <a href="http://www.earth-time.org/">http://www.earth-time.org</a><br />	2.	Lourens, L. J. et al. in Geologic Time Scale 2004 (eds Gradstein, F. M., Ogg, J. G., Smith, A. G.) 409–440 (Cambridge Univ. Press, 2004).<br />	3.	Raffi, I. et al. Quat. Sci. Rev. 25, 3113–3137 (2006). | <a href="http://dx.doi.org/10.1016/j.quascirev.2006.07.007">Article</a> |<br />	4.	Billups, K. et al. Earth Planet. Sci. Lett. 224, 33–44 (2004). | <a href="http://dx.doi.org/10.1016/j.epsl.2004.05.004">Article</a> |<br />	5.	Pälike, H. et al. Science 314, 1894–1898 (2006). | <a href="http://dx.doi.org/10.1126/science.1133822">Article</a> |<br />	6.	Pälike, H., Shackleton, N. J. &amp; Röhl, U. Earth Planet. Sci. Lett. 193, 589–602 (2001). | <a href="http://dx.doi.org/10.1016/S0012-821X%252801%252900501-5">Article</a> |<br />	7.	Röhl, U., Norris, R. D. &amp; Ogg, J. G. Spec. Pap. Geol. Soc. Am. 369, 576–589 (2003).<br />	8.	Lourens, L. J. et al. Nature 435, 1083–1087 (2005). | <a href="http://www.nature.com/doifinder/10.1038/nature03814">Article</a> |<br />	9.	Westerhold, T. et al. Palaeogeogr. Palaeocl. 257, 377–403 (2008) . | <a href="http://dx.doi.org/10.1029/2007GC001784">Article</a> |<br />	10.	Kuiper, K. F. et al. Science (in the press).<br />	11.	Zachos, J. C., Dickens, G. R. &amp; Zeebe, R. E. Nature 451, 279–283 (2008). | <a href="http://www.nature.com/doifinder/10.1038/nature06588">Article</a> |<br />Please note correction:<br />Reference 7 should be:<br />Röhl, U, Brinkhuis, H, Fuller, M, Schellenberg, S A, Stickley, C E, Wefer, G., Williams, G L (2004) Cyclostratigraphy of middle and late Eocene sediments drilled on the East Tasman Plateau (Site 1172)- In Exon, NF, Malone, M, and Kennett, JP (Eds.), Climate evolution in the Southern Ocean and Australia’s Cenozoic flight northward from Antarctica. Am. Geophys. Union, Geophys. Monogr., 151, 127-152. </p>
<p>Reference 10 is published:<br /><a href="http://www.sciencemag.org/cgi/content/full/sci%253B320/5875/500">RESEARCH ARTICLE in SCIENCE:<br />Synchronizing Rock Clocks of Earth History<br />K. F. Kuiper, A. Deino, F. J. Hilgen, W. Krijgsman, P. R. Renne, and J. R. Wijbrans (25 April 2008)<br />Science 320 (5875), 500. [DOI: 10.1126/science.1154339]</a></p>
<p>Figure 1 Caption:<br />The upper part illustrates a selection of previous work that resulted in detailed age calibrations for the Neogene and Quaternary<a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523B2">2, </a><a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523B3">3</a>, and parts of the Palaeogene<a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523B5">5, </a><a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523B6">6, </a><a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523B7">7, </a><a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523B8">8, </a><a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523B9">9, </a><a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523B10">10</a>. The uppermost horizontal line indicates a fairly stable and accurate astronomical age calibration with multiple site coverage (solid line), and more tentative or unverified age calibrations (dashed line). There is a significant gap in the middle Eocene (approximately 42 to 53 Myr ago). Age calibrations are shown in the context of an updated multi-site compilation from the Cenozoic of benthic foraminiferal oxygen isotope data<a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523B11">11</a>, supplemented by the most recent age compilation for magnetic reversals during the Cenozoic<a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523B2">2</a>. The labels C1n, C2n, and so on, and respective black bars, correspond to the geomagnetic polarity timescale defined by Cande and Kent using the revised ages from the Geological Time Scale 2004<a href="http://www.nature.com/ngeo/journal/v1/n5/full/ngeo197.html%2523B2">2</a>.</p>
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		</item>
		<item>
		<title>Synchronizing Rock Clocks of Earth History</title>
		<link>http://earthtime-eu.eu/earthtime/?p=331</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=331#comments</comments>
		<pubDate>Fri, 25 Apr 2008 10:03:52 +0000</pubDate>
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		<description><![CDATA[RESEARCH ARTICLE in SCIENCE:Synchronizing Rock Clocks of Earth HistoryK. F. Kuiper, A. Deino, F. J. Hilgen, W. Krijgsman, P. R. Renne, and J. R. Wijbrans (25 April 2008)Science 320 (5875), 500. [DOI: 10.1126/science.1154339]
Also see commentary by Richard Kerr:Science 25 April 2008: Vol. 320. no. 5875, pp. 434 &#8211; 435 DOI: 10.1126/science.320.5875.434NEWS OF THE WEEKGEOCHEMISTRY: Two Geologic Clocks Finally [...]]]></description>
			<content:encoded><![CDATA[<p><a href="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Entries/2008/4/25_Entry_1_files/Kuiper_Science2008.pdf"><img src="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Media/Kuiper_Science2008.png" style="float:left; padding-right:10px; padding-bottom:10px; width:227px; height:191px;"/></a><a href="http://www.sciencemag.org/cgi/content/full/sci%253B320/5875/500">RESEARCH ARTICLE in SCIENCE:<br />Synchronizing Rock Clocks of Earth History<br />K. F. Kuiper, A. Deino, F. J. Hilgen, W. Krijgsman, P. R. Renne, and J. R. Wijbrans (25 April 2008)<br />Science 320 (5875), 500. [DOI: 10.1126/science.1154339]</a></p>
<p><a href="http://www.sciencemag.org/cgi/content/full/320/5875/434">Also see commentary by Richard Kerr:<br />Science 25 April 2008: Vol. 320. no. 5875, pp. 434 &#8211; 435 DOI: 10.1126/science.320.5875.434<br />NEWS OF THE WEEK<br />GEOCHEMISTRY: Two Geologic Clocks Finally Keeping the Same Time<br />Richard A. Kerr</a></p>
<p>Additional commentary from Science Daily:<br /><a href="http://www.sciencedaily.com/releases/2008/04/080424140400.htm">http://www.sciencedaily.com/releases/2008/04/080424140400.htm</a></p>
<p>and the Berkeley group:<br /><a href="http://www.berkeley.edu/news/media/releases/2008/04/24_argondating.shtml">http://www.berkeley.edu/news/media/releases/2008/04/24_argondating.shtml</a></p>
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		<title>Astronomical calibration of Paleocene time</title>
		<link>http://earthtime-eu.eu/earthtime/?p=332</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=332#comments</comments>
		<pubDate>Wed, 30 Jan 2008 09:51:28 +0000</pubDate>
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		<description><![CDATA[Westerhold, T., Rohl, U., Raffi, I., Fornaciari, E., Monechi, S., Reale, V., Bowles, J., and Evans, H. F., 2008, Astronomical calibration of the Paleocene time: Palaeogeography, Palaeoclimatology, Palaeoecology, 257, no. 4, p. 377-403, doi:10.1016/j.palaeo.2007.09.016
]]></description>
			<content:encoded><![CDATA[<p><a href="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Entries/2008/1/30_Astronomical_calibration_of_Paleocene_time_files/Westerhold2008.pdf"><img src="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Media/Westerhold2008.png" style="float:left; padding-right:10px; padding-bottom:10px; width:245px; height:83px;"/></a>Westerhold, T., Rohl, U., Raffi, I., Fornaciari, E., Monechi, S., Reale, V., Bowles, J., and Evans, H. F., 2008, Astronomical calibration of the Paleocene time: Palaeogeography, Palaeoclimatology, Palaeoecology, 257, no. 4, p. 377-403, <a href="http://dx.doi.org/10.1016/j.palaeo.2007.09.016">doi:10.1016/j.palaeo.2007.09.016</a></p>
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		<title>On the duration of the Paleocene-Eocene Thermal Maximum (PETM)</title>
		<link>http://earthtime-eu.eu/earthtime/?p=333</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=333#comments</comments>
		<pubDate>Tue, 11 Dec 2007 12:55:13 +0000</pubDate>
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		<description><![CDATA[Röhl, U., Westerhold, T., Bralower, T. J. and Zachos, J. C. (2007), On the duration of the Paleocene-Eocene thermal maximum (PETM), Geochem. Geophys. Geosyst., 8, Q12002, doi:10.1029/2007GC001784.
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			<content:encoded><![CDATA[<p><a href="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Entries/2007/12/11_Closing_the_Mid-Palaeocene_gap%3A_Toward_a_complete_astronomically_tuned_Palaeocene_Epoch_2_files/roehl2007G3.png"><img src="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Media/roehl2007G3.png" style="float:left; padding-right:10px; padding-bottom:10px; width:228px; height:194px;"/></a>Röhl, U., Westerhold, T., Bralower, T. J. and Zachos, J. C. (2007), On the duration of the Paleocene-Eocene thermal maximum (PETM), Geochem. Geophys. Geosyst., 8, Q12002, <a href="http://dx.doi.org/10.1029/2007GC001784">doi:10.1029/2007GC001784</a>.</p>
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		<title>Closing the Mid-Palaeocene gap: Toward a complete astronomically tuned Palaeocene Epoch</title>
		<link>http://earthtime-eu.eu/earthtime/?p=334</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=334#comments</comments>
		<pubDate>Tue, 30 Oct 2007 15:21:11 +0000</pubDate>
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		<description><![CDATA[Dinarès-Turell, J., Baceta, J. I., Bernaola, G., Orue-Etxebarria, X., Pujalte, V. (2007) Closing the Mid-Palaeocene gap: Toward a complete astronomically tuned Palaeocene Epoch and Selandian and Thanetian GSSPs at ZUmaia (Basque Basin, W Pyrenees), EPSL 262 (3-4), 450-467, doi:10.1017/j.epsl.2007.08.008
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			<content:encoded><![CDATA[<p><a href="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Entries/2007/10/30_Entry_1_files/Dinares_EPSL2007.png"><img src="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Media/Dinares_EPSL2007.png" style="float:left; padding-right:10px; padding-bottom:10px; width:306px; height:170px;"/></a>Dinarès-Turell, J., Baceta, J. I., Bernaola, G., Orue-Etxebarria, X., Pujalte, V. (2007) Closing the Mid-Palaeocene gap: Toward a complete astronomically tuned Palaeocene Epoch and Selandian and Thanetian GSSPs at ZUmaia (Basque Basin, W Pyrenees), EPSL 262 (3-4), 450-467, doi:<a href="http://dx.doi.org/10.1016/j.epsl.2007.08.008">10.1017/j.epsl.2007.08.008</a></p>
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		<title>On the duration of magnetochrons C24r and C25n and the timing of early Eocene global warming events</title>
		<link>http://earthtime-eu.eu/earthtime/?p=335</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=335#comments</comments>
		<pubDate>Fri, 06 Apr 2007 13:20:54 +0000</pubDate>
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		<description><![CDATA[Westerhold T., U. Röhl, J. Laskar, I. Raffi, J. Bowles, L. J. Lourens, J. C. Zachos (2007), On the duration of magnetochrons C24r and C25n and the timing of early Eocene global warming events: Implications from the Ocean Drilling Program Leg 208 Walvis Ridge depth transect, Paleoceanography, 22, PA2201, doi:10.1029/2006PA001322.
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			<content:encoded><![CDATA[<p><a href="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Entries/2007/4/6_Entry_1_files/westerhold2007.png"><img src="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Media/westerhold2007.png" style="float:left; padding-right:10px; padding-bottom:10px; width:229px; height:170px;"/></a>Westerhold T., U. Röhl, J. Laskar, I. Raffi, J. Bowles, L. J. Lourens, J. C. Zachos (2007), On the duration of magnetochrons C24r and C25n and the timing of early Eocene global warming events: Implications from the Ocean Drilling Program Leg 208 Walvis Ridge depth transect, Paleoceanography, 22, PA2201, doi:<a href="http://dx.doi.org/10.1029/2006PA001322">10.1029/2006PA001322</a>.</p>
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		<title>The heartbeat of the Oligocene climate system</title>
		<link>http://earthtime-eu.eu/earthtime/?p=336</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=336#comments</comments>
		<pubDate>Mon, 25 Dec 2006 19:06:56 +0000</pubDate>
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		<description><![CDATA[Pälike, H., Norris, R.D., Herrle, J.O., Wilson, P.A., Coxall, H.K., Lear, C.H., Shackleton, N.J., Tripati, A.K. and Wade, B.S. (2006) The heartbeat of the Oligocene climate system. Science, 314, (5807), 1894-1898. (doi:10.1126/science.1133822)
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			<content:encoded><![CDATA[<p><a href="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Entries/2006/12/25_The_heartbeat_of_the_Oligocene_climate_system_files/droppedImage.jpg"><img src="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Media/droppedImage_3.jpg" style="float:left; padding-right:10px; padding-bottom:10px; width:211px; height:301px;"/></a>Pälike, H., Norris, R.D., Herrle, J.O., Wilson, P.A., Coxall, H.K., Lear, C.H., Shackleton, N.J., Tripati, A.K. and Wade, B.S. (2006) The heartbeat of the Oligocene climate system. Science, 314, (5807), 1894-1898. (<a href="http://dx.doi.org/doi%253A10.1126/science.1133822">doi:10.1126/science.1133822</a>)</p>
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		<title>Telling the time</title>
		<link>http://earthtime-eu.eu/earthtime/?p=337</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=337#comments</comments>
		<pubDate>Thu, 09 Nov 2006 19:22:35 +0000</pubDate>
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		<description><![CDATA[      Editorial piece in Nature:http://www.nature.com/nature/journal/v444/n7116/full/444134a.html
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			<content:encoded><![CDATA[<p><a href="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Entries/2006/11/9_Telling_the_time_files/droppedImage_1.jpg"><img src="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Media/droppedImage_4.jpg" style="float:left; padding-right:10px; padding-bottom:10px; width:536px; height:170px;"/></a>      Editorial piece in Nature:<br /><a href="http://www.nature.com/nature/journal/v444/n7116/full/444134a.html">http://www.nature.com/nature/journal/v444/n7116/full/444134a.html</a></p>
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		<title>Unit stratotypes for global stages: The Neogene perspective:</title>
		<link>http://earthtime-eu.eu/earthtime/?p=338</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=338#comments</comments>
		<pubDate>Fri, 30 Sep 2005 18:37:11 +0000</pubDate>
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		<description><![CDATA[Hilgen, F. J., Brinkhuis, H., Zachariasse, W.-J. (2006), “Unit stratotypes for global stages: The Neogene perspective”, Earth Science Reviews 74 (1-2), 113-125.  doi:10.1016/j.earscirev.2005.09.003
Abstract:
Recent developments in integrated high-resolution stratigraphy and astronomical tuning of continuous deep marine successions invalidate arguments against the designation of unit stratotypes for global stages, the basic building blocks of the standard [...]]]></description>
			<content:encoded><![CDATA[<p><a href="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Entries/2005/9/30_Unit_stratotypes_for_global_stages%3A_The_Neogene_perspective%3A_files/hilgen2006.png"><img style="float: left; padding-right: 10px; padding-bottom: 10px; width: 227px; height: 152px;" src="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Media/hilgen2006.png" alt="" /></a>Hilgen, F. J., Brinkhuis, H., Zachariasse, W.-J. (2006), “Unit stratotypes for global stages: The Neogene perspective”, Earth Science Reviews 74 (1-2), 113-125.  <a href="http://dx.doi.org/10.1016/j.earscirev.2005.09.003">doi:10.1016/j.earscirev.2005.09.003</a></p>
<h3>Abstract:</h3>
<p>Recent developments in integrated high-resolution stratigraphy and astronomical tuning of continuous deep marine successions invalidate arguments against the designation of unit stratotypes for global stages, the basic building blocks of the standard Global Chronostratigraphic Scale (GCS). For the late Neogene, Global Stratotype Section and Point (GSSP) sections may also serve as unit stratotypes, covering the interval from the base of a stage up to the level that–time-stratigraphically–correlates with the base of the next younger stage in a continuous and well-tuned deep marine succession. The added value of such sections as unit stratotype lies in the integrated high-resolution stratigraphy and astronomical tuning, which combined, provides an excellent age control with an unprecedented resolution, precision and accuracy <em>within</em> the entire stage. As such they form the backbone of the new integrated late Neogene time scale and provide the basis for reconstructing Earth&#8217;s history. In this way a stage is also defined by its <em>content</em> and not only by its boundaries. Our unit stratotype concept strengthens the importance of time-rock units by allowing the introduction of astronomically defined chronozones as formal chronostratigraphic units, thereby arguing against the elimination of the dual classification of chronostratigraphy and geochronology.</p>
<p>Extending this concept to older time intervals requires that well-tuned, continuous deep marine sections are employed, thus necessitating the employment of multiple hole (I)ODP sites for defining (remaining) stages and stage boundaries in at least the Cenozoic and Cretaceous and possibly the entire Mesozoic. Evidently the construction of the Geological Time Scale (including the GCS) should be based on the most appropriate sections available while, where possible, taking the historical concept of global stages into account.</p>
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		<title>The Paleocene/Eocene transition</title>
		<link>http://earthtime-eu.eu/earthtime/?p=339</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=339#comments</comments>
		<pubDate>Wed, 08 Jun 2005 16:48:52 +0000</pubDate>
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		<description><![CDATA[Lourens, L. J., Sluijs, A., Kroon, D., Zachos, Z. C., Thomas, E., Röhl, U., Bowles, J., Raffi. I. (2005) Astronomical pacing of late Palaeocene to early Eocene global warming events. Nature 435, 1083-1087.(doi:10.1038/nature03814)
]]></description>
			<content:encoded><![CDATA[<p><a href="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Entries/2005/6/8_The_Paleocene_Eocene_transition_files/lourens2005.png"><img src="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Media/lourens2005.png" style="float:left; padding-right:10px; padding-bottom:10px; width:227px; height:176px;"/></a>Lourens, L. J., Sluijs, A., Kroon, D., Zachos, Z. C., Thomas, E., Röhl, U., Bowles, J., Raffi. I. (2005) Astronomical pacing of late Palaeocene to early Eocene global warming events. Nature 435, 1083-1087.(<a href="http://dx.doi.org/doi%253A10.1038/nature03814">doi:10.1038/nature03814</a>)</p>
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		<title>A long-term numerical solution for the insolation &#013;quantities of the Earth</title>
		<link>http://earthtime-eu.eu/earthtime/?p=340</link>
		<comments>http://earthtime-eu.eu/earthtime/?p=340#comments</comments>
		<pubDate>Wed, 11 Aug 2004 08:57:00 +0000</pubDate>
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		<description><![CDATA[Laskar, J., Robutel, P., Joutel, F., Gastineau, M., Correia, A.C.M., Levrard, B. (2004), A long-term numerical solution for the insolation quantities of the Earth, Astronomy &#38; Astrophysics 428, 261-285. doi:10.1051/0004-6361:20041335
]]></description>
			<content:encoded><![CDATA[<p><a href="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Entries/2004/8/11_Entry_1_files/droppedImage.jpg"><img src="http://www.earthtime-eu.eu/Earthtime_Europe/Publications/Media/droppedImage_5.jpg" style="float:left; padding-right:10px; padding-bottom:10px; width:226px; height:179px;"/></a>Laskar, J., Robutel, P., Joutel, F., Gastineau, M., Correia, A.C.M., Levrard, B. (2004), A long-term numerical solution for the insolation quantities of the Earth, Astronomy &amp; Astrophysics 428, 261-285. <a href="http://dx.doi.org/10.1051/0004-6361%253A20041335">doi:10.1051/0004-6361:20041335</a></p>
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