The ST22 chronology for the Skytrain Ice Rise ice core – Part 2: An age model to the last interglacial and disturbed deep stratigraphy
dc.contributor.author
Mulvaney, Robert
dc.contributor.author
Wolff, Eric W.
dc.contributor.author
Grieman, Mackenzie M.
dc.contributor.author
Hoffmann, Helene H.
dc.contributor.author
Humby, Jack D.
dc.contributor.author
Nehrbass-Ahles, Christoph
dc.contributor.author
Rhodes, Rachael H.
dc.contributor.author
Rowell, Isobel F.
dc.contributor.author
Parrenin, Frédéric
dc.contributor.author
Schmidely, Loïc
dc.contributor.author
Fischer, Hubertus
dc.contributor.author
Stocker, Thomas F.
dc.contributor.author
Christl, Marcus
dc.contributor.author
Muscheler, Raimund
dc.contributor.author
Landais, Amaelle
dc.contributor.author
Prié, Frédéric
dc.date.accessioned
2023-05-19T12:30:49Z
dc.date.available
2023-05-19T03:21:51Z
dc.date.available
2023-05-19T12:30:49Z
dc.date.issued
2023-04-27
dc.identifier.issn
1814-9324
dc.identifier.issn
1814-9332
dc.identifier.other
10.5194/cp-19-851-2023
en_US
dc.identifier.uri
http://hdl.handle.net/20.500.11850/612668
dc.identifier.doi
10.3929/ethz-b-000612668
dc.description.abstract
We present an age model for the 651 m deep ice core from Skytrain Ice Rise, situated inland of the Ronne Ice Shelf, Antarctica. The top 2000 years have previously been dated using age markers interpolated through annual layer counting. Below this, we align the Skytrain core to the AICC2012 age model using tie points in the ice and air phase, and we apply the Paleochrono program to obtain the best fit to the tie points and glaciological constraints. In the gas phase, ties are made using methane and, in critical sections, δ18Oair; in the ice phase ties are through 10Be across the Laschamps event and through ice chemistry related to long-range dust transport and deposition. This strategy provides a good outcome to about 108 ka (∼ 605 m). Beyond that there are signs of flow disturbance, with a section of ice probably repeated. Nonetheless values of CH4 and δ18Oair confirm that part of the last interglacial (LIG), from about 117–126 ka (617–627 m), is present and in chronological order. Below this there are clear signs of stratigraphic disturbance, with rapid oscillation of values in both the ice and gas phase at the base of the LIG section, below 628 m. Based on methane values, the warmest part of the LIG and the coldest part of the penultimate glacial are missing from our record. Ice below 631 m appears to be of age > 150 ka.
en_US
dc.format
application/pdf
en_US
dc.language.iso
en
en_US
dc.publisher
Copernicus
en_US
dc.rights.uri
http://creativecommons.org/licenses/by/4.0/
dc.title
The ST22 chronology for the Skytrain Ice Rise ice core – Part 2: An age model to the last interglacial and disturbed deep stratigraphy
en_US
dc.type
Journal Article
dc.rights.license
Creative Commons Attribution 4.0 International
ethz.journal.title
Climate of the Past
ethz.journal.volume
19
en_US
ethz.journal.issue
4
en_US
ethz.journal.abbreviated
Clim. Past
ethz.pages.start
851
en_US
ethz.pages.end
864
en_US
ethz.version.deposit
publishedVersion
en_US
ethz.identifier.wos
ethz.identifier.scopus
ethz.publication.place
Göttingen
en_US
ethz.publication.status
published
en_US
ethz.leitzahl
ETH Zürich::00002 - ETH Zürich::00012 - Lehre und Forschung::00007 - Departemente::02010 - Dep. Physik / Dep. of Physics::02532 - Institut für Teilchen- und Astrophysik / Inst. Particle Physics and Astrophysics::08619 - Labor für Ionenstrahlphysik (LIP) / Laboratory of Ion Beam Physics (LIP)
ethz.leitzahl.certified
ETH Zürich::00002 - ETH Zürich::00012 - Lehre und Forschung::00007 - Departemente::02010 - Dep. Physik / Dep. of Physics::02532 - Institut für Teilchen- und Astrophysik / Inst. Particle Physics and Astrophysics::08619 - Labor für Ionenstrahlphysik (LIP) / Laboratory of Ion Beam Physics (LIP)
ethz.date.deposited
2023-05-19T03:21:52Z
ethz.source
SCOPUS
ethz.eth
yes
en_US
ethz.availability
Open access
en_US
ethz.rosetta.installDate
2024-02-02T23:15:56Z
ethz.rosetta.lastUpdated
2024-02-02T23:15:56Z
ethz.rosetta.exportRequired
true
ethz.rosetta.versionExported
true
ethz.COinS
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