EGU26-19245, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-19245
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Monday, 04 May, 09:45–09:55 (CEST)
 
Room F1
Halogen Records from the Beyond EPICA Ice Core: Insights from the Holocene to the Mid-Pleistocene Transition
Ginevra Chelli1, Federica Bruschi2, David Cappelletti2,5, Mirko Severi3, Rita Traversi3, Elena Di Stefano4, Azzurra Spagnesi1,5, Valentina Raspagni4, Barbara Stenni1, Elena Barbaro1,5, Marco Roman1,5, Chiara Venier1,5, Warren Cairns1,5, Barbara Delmonte4, Carlo Barbante1,5, Chiara Petroselli2, and Andrea Spolaor1,5
Ginevra Chelli et al.
  • 1Ca’ Foscari University of Venice, Department of Environmental Sciences, Informatics and Statistics, Venice-Mestre, Italy
  • 2Department of Chemistry, Biology and Biotechnology, University of Perugia, Perugia, Italy
  • 3Department of Chemistry, University of Florence, Florence, Italy
  • 4University Milano-Bicocca, DISAT – Dept. Earth and Environmental Sciences, Milano, Italy
  • 5Institute of Polar Sciences - National Research Council of Italy (CNR-ISP), Venezia-Mestre (VE), Italy

Halogens (Br, I) and their enrichment relative to seawater abundance preserved in polar ice cores are powerful tracers for reconstructing past sea-ice dynamics and marine primary productivity. Within the framework of the Beyond EPICA Oldest Ice (BEOI) project, we present a new halogen concentration record derived from discrete ice core samples. Analytical measurements were performed in Italy (ISP-CNR, Ca’ Foscari University), focusing on the relatively stable climatic conditions of the Holocene and on the Mid-Pleistocene Transition (MPT).

The Holocene record, combined with previously published datasets, provides a critical baseline for understanding the environmental processes and transport mechanisms controlling halogen deposition on the central Antarctic plateau. To validate the halogen signal, we investigate the behaviour of bromine and iodine measured in the Younger Ice section of the BEOI ice core during the Holocene, comparing these records with independent paleoclimatic parameters from earlier studies, including temperature reconstructions (ΔT), stable water isotopes (δD), and sea surface temperatures (SST). These comparisons support the interpretation of halogen variability as a proxy for changes in sea-ice conditions.

While the Holocene analysis aims to constrain the halogen signal using well-established climatic parameters, the primary objective of the Beyond EPICA mission is to extend this approach back to 1.5 million years. As drilling reaches the deepest sections of the BEOI ice core, halogen records offer a unique opportunity to investigate changes in sea-ice dynamics across the MPT, when Earth’s climate system transitioned from a dominant 41-kyr to a 100-kyr glacial cyclicity. Ongoing chemical analyses of the oldest ice will help assess whether sea-ice feedbacks played a causal role in the emergence of the 100-kyr cycles or primarily acted as an amplifier of late-Pleistocene glacial intensification.

How to cite: Chelli, G., Bruschi, F., Cappelletti, D., Severi, M., Traversi, R., Di Stefano, E., Spagnesi, A., Raspagni, V., Stenni, B., Barbaro, E., Roman, M., Venier, C., Cairns, W., Delmonte, B., Barbante, C., Petroselli, C., and Spolaor, A.: Halogen Records from the Beyond EPICA Ice Core: Insights from the Holocene to the Mid-Pleistocene Transition, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19245, https://doi.org/10.5194/egusphere-egu26-19245, 2026.