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  Constraints on the use of cosmogenic beryllium isotopes for synchronizing marine sediments and ice cores

Loftfield, J., Nowaczyk, N., Lembke-Jene, L., Frederichs, T., Lachner, J., Lamy, F., Rugel, G., Stübner, K., Adolphi, F. (2025): Constraints on the use of cosmogenic beryllium isotopes for synchronizing marine sediments and ice cores. - Earth and Planetary Science Letters, 671, 119665.
https://doi.org/10.1016/j.epsl.2025.119665

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Loftfield, Julia1, Author
Nowaczyk, N.2, Author                 
Lembke-Jene, Lester1, Author
Frederichs, Thomas1, Author
Lachner, Johannes1, Author
Lamy, Frank1, Author
Rugel, Georg1, Author
Stübner, Konstanze1, Author
Adolphi, Florian1, Author
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1External Organizations, ou_persistent22              
22.3 Geomagnetism, 2.0 Geophysics, Departments, GFZ Publication Database, GFZ Helmholtz Centre for Geosciences, ou_146030              

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 Abstract: Changes in the atmospheric production of cosmogenic 10Be leave a global fingerprint in 10Be deposition fluxes which makes them a powerful tool for the synchronization of different paleo-climate archives. However, for a robust synchronization we must understand the pathways of 10Be from its production in the upper atmosphere to its deposition in ice cores and sediments. While 10Be is deposited in ice within one to two years from its production, the less direct deposition within marine sediments, complicates its use for synchronization. Here, we investigate the response of the authigenic 10Be/9Be ratio in marine sediments to a sudden increase in atmospheric 10Be production rates. For this, we measured the 10Be/9Be ratios of three sediment cores from the Southern Ocean, influenced by the Antarctic Circumpolar Current (ACC), covering the time of the geomagnetic field minimum during the Laschamps excursion (∼ 41 ka BP), and compared them to 10Be records from ice cores. In all cores we observe an increase in the 10Be/9Be ratio during the Laschamps excursion. The marine records, however, show site-specific divergencies from the ice core records with respect to their amplitude and response time. We discuss the cause of these differences and the role of the local oceanic residence time of Be, bioturbation of sediments, diagenetic Be fluxes, re-mobilization of sediments, and varying terrestrial sources of Be. We conclude that the achievable precision of 10Be-based synchronization depends on the a-priori knowledge of these factors. Especially the marine residence time of 10Be provides an upper limit on the achievable resolution from marine sediment 10Be/9Be records and leads to a lag of the recorded 10Be/9Be changes with respect to the atmospheric production rate increase. Furthermore, input of terrestrial material may lead to non-production influences on the 10Be/9Be ratio in marine sediments even at pelagic locations, as terrigenous sediments carry a lower 10Be/9Be ratio. In an ideal setting, marine sediments can record 10Be/9Be signals that are very similar to ice cores, highlighting the potential of 10Be/9Be ratios as a future chronostratigraphic tool for synchronizing marine and terrestrial climate records.

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 Dates: 2025-12-012025
 Publication Status: Finally published
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 Identifiers: DOI: 10.1016/j.epsl.2025.119665
GFZPOF: p4 MESI
OATYPE: Hybrid Open Access
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Title: Earth and Planetary Science Letters
Source Genre: Journal, SCI, Scopus
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Pages: - Volume / Issue: 671 Sequence Number: 119665 Start / End Page: - Identifier: ISSN: 0012-821X
ISSN: 1385-013X
Publisher: Elsevier
CoNE: https://gfzpublic.gfz.de/cone/journals/resource/journals99