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dc.contributor.author
Elsässer, Christoph
dc.contributor.author
Wagenbach, Dietmar
dc.contributor.author
Levin, Ingeborg
dc.contributor.author
Stanzick, A.
dc.contributor.author
Christl, Marcus
dc.contributor.author
Wallner, Anton
dc.contributor.author
Kipfstuhl, Sepp
dc.contributor.author
Seierstad, I.K.
dc.contributor.author
Wershofen, Herbert
dc.contributor.author
Dibb, Jack
dc.date.accessioned
2019-06-26T14:57:51Z
dc.date.available
2017-06-11T16:14:32Z
dc.date.available
2019-06-26T14:57:51Z
dc.date.issued
2015
dc.identifier.issn
1814-9324
dc.identifier.issn
1814-9332
dc.identifier.other
10.5194/cp-11-115-2015
en_US
dc.identifier.uri
http://hdl.handle.net/20.500.11850/98338
dc.identifier.doi
10.3929/ethz-b-000098338
dc.description.abstract
10Be ice core measurements are an important tool for paleoclimate research, e.g., allowing for the reconstruction of past solar activity or changes in the geomagnetic dipole field. However, especially on multi-millennial timescales, the share of production and climate-induced variations of respective 10Be ice core records is still up for debate. Here we present the first quantitative climatological model of the 10Be ice concentration up to the glacial–interglacial timescale. The model approach is composed of (i) a coarse resolution global atmospheric transport model and (ii) a local 10Be air–firn transfer model. Extensive global-scale observational data of short-lived radionuclides as well as new polar 10Be snow-pit measurements are used for model calibration and validation. Being specifically configured for 10Be in polar ice, this tool thus allows for a straightforward investigation of production- and non-production-related modulation of this nuclide. We find that the polar 10Be ice concentration does not immediately record the globally mixed cosmogenic production signal. Using geomagnetic modulation and revised Greenland snow accumulation rate changes as model input, we simulate the observed Greenland Summit (GRIP and GISP2) 10Be ice core records over the last 75 kyr (on the GICC05modelext timescale). We show that our basic model is capable of reproducing the largest portion of the observed 10Be changes. However, model–measurement differences exhibit multi-millennial trends (differences up to 87% in case of normalized to the Holocene records) which call for closer investigation. Focusing on the (12–37) b2k (before the year AD 2000) period, mean model–measurement differences of 30% cannot be attributed to production changes. However, unconsidered climate-induced changes could likely explain the model–measurement mismatch. In fact, the 10Be ice concentration is very sensitive to snow accumulation changes. Here the reconstructed Greenland Summit (GRIP) snow accumulation rate record would require revision of +28% to solely account for the (12–37) b2k model–measurement differences.
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/3.0/
dc.title
Simulating ice core 10Be on the glacial-interglacial timescale
en_US
dc.type
Journal Article
dc.rights.license
Creative Commons Attribution 3.0 Unported
dc.date.published
2015-02-03
ethz.journal.title
Climate of the Past
ethz.journal.volume
11
en_US
ethz.journal.issue
2
en_US
ethz.journal.abbreviated
Clim. past
ethz.pages.start
115
en_US
ethz.pages.end
133
en_US
ethz.version.deposit
publishedVersion
en_US
ethz.identifier.scopus
ethz.identifier.nebis
005583758
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)
en_US
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
2017-06-11T16:14:39Z
ethz.source
ECIT
ethz.identifier.importid
imp593652f2c1df121938
ethz.ecitpid
pub:153797
ethz.eth
yes
en_US
ethz.availability
Open access
en_US
ethz.rosetta.installDate
2017-07-14T15:26:18Z
ethz.rosetta.lastUpdated
2021-02-15T04:53:59Z
ethz.rosetta.versionExported
true
ethz.COinS
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