EGU26-13087, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-13087
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Friday, 08 May, 15:35–15:45 (CEST)
 
Room 0.49/50
Revisiting radiocarbon production and the glacial carbon cycle during the Laschamps geomagnetic excursion
Vincent Wall1, Frank Lamy1, Lester Lembke-Jene1, Johannes Lachner2, Stella Winkler2, and Florian Adolphi1,3
Vincent Wall et al.
  • 1Alfred Wegener Institute, Helmholtz Centre for Polar and Marine Research, Bremerhaven, Germany
  • 2Accelerator Mass Spectrometry and Isotope Research, Helmholtz-Zentrum Dresden-Rossendorf, Dresden, Germany
  • 3Department of Geosciences, University Bremen, Bremen, Germany

Reconstructions of atmospheric radiocarbon during the Laschamps geomagnetic excursion show a pronounced increase in Δ14C. The amplitude of this increase remains poorly reproduced by current carbon cycle models driven by independent 14C-production rates derived from 10Be ice-core records or geomagnetic field intensity reconstructions. This mismatch has commonly been attributed to uncertainties in cosmogenic 14C production rates, potentially arising from the underestimation of global production-rate changes in polar ice-core 10Be records during periods of strongly reduced geomagnetic field intensity.

Here we present a new global compilation of 10Be records from ice cores and marine sediments spanning the Laschamps event, providing an improved, globally integrated estimate of cosmogenic nuclide production for the period from 30,000 to 60,000 years BP. This compilation overcomes previous limitations of polar-only ice-core records, is more representative of global production, and is consistent with latest geomagnetic field intensity reconstructions. However, while the revised production rate implies larger 14C production-rate changes than previous estimates, it remains insufficient to reproduce the full amplitude of the observed Δ14C increase when implemented in carbon cycle models under conservative parameterization.

Using transient tuning of a simple carbon cycle model, we show that the remaining model–data mismatch is closely linked to signals observed in independent climate proxies, in particular ice-core δ18O records. This similarity suggests that the interactions between climate changes and carbon cycle dynamics during the glacial period are not adequately represented in current models.

Our results indicate that uncertainties in cosmogenic production alone cannot explain the radiocarbon anomaly associated with the Laschamps event. Instead, they point to a need for improved representations of climate–carbon cycle interactions under glacial conditions. This finding highlights the importance of revisiting carbon cycle dynamics, including carbon reservoir sizes, exchange rates, and circulation changes, in glacial climates, and demonstrates the value of globally integrated cosmogenic isotope records for disentangling production and carbon cycle effects in past radiocarbon variations.

How to cite: Wall, V., Lamy, F., Lembke-Jene, L., Lachner, J., Winkler, S., and Adolphi, F.: Revisiting radiocarbon production and the glacial carbon cycle during the Laschamps geomagnetic excursion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13087, https://doi.org/10.5194/egusphere-egu26-13087, 2026.