EGU26-22482, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-22482
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Monday, 04 May, 14:00–15:45 (CEST), Display time Monday, 04 May, 14:00–18:00
 
Hall X5, X5.210
Windblown diatoms at Little Dome C and their potential for reconstructing Southern Hemisphere Westerly Winds during the MPT 
Dieter Tetzner1, Claire Allen1, Delia Segato2,3, James Veale1, Romilly Harris-Stuart4, and Julien Westhoff5
Dieter Tetzner et al.
  • 1British Antarctic Survey, Ice Dynamics and Paleoclimate, Cambridge, CB3 0ET, UK
  • 2European Commission Joint Research Centre, Ispra (VA), Italy
  • 3Department of Environmental Sciences, Informatics and Statistics, Ca’ Foscari University of Venice, Venice-Mestre, Italy
  • 4College of Earth, Ocean and Atmospheric Sciences, Oregon State University, Corvallis OR 97331, USA
  • 5Niels Bohr Institute, University of Copenhagen, 2200 Copenhagen, Denmark

The Southern Hemisphere Westerly Winds play a crucial role in the Earth's climate system and may have influenced the physical and biological processes that drove CO2 exchange in the Southern Ocean during the Mid-Pleistocene Transition (MPT). Numerous paleoclimate archives have been utilised to reconstruct past westerly winds over different timescales; however, many are limited by their reliance on precipitation or temperature proxies to infer SHWW changes. Marine diatoms found in Antarctic ice core layers have recently established as a reliable proxy for directly reconstructing historical changes in wind strength and atmospheric circulation within the Southern Hemisphere Westerly Wind belt.

In this study, we present diatom records preserved in two snow pits from Little Dome C and in Holocene samples from the EPICA Dome C ice core. The annual abundance of diatoms preserved in Little Dome C snow layers strongly correlates with wind strength over South America and the South Atlantic sector of the Southern Ocean. Backward trajectory analyses enable us to trace the pathways of air masses before reaching the Little Dome C site, aiming to identify potential primary source regions for the Little Dome C diatoms. The strong positive correlation between Little Dome C diatoms and wind strength in South America and the South Atlantic highlights the potential to use diatoms preserved in the BE-OI as a proxy for reconstructing past changes in mid-latitude winds. This study lays the groundwork for further exploration of diatom records preserved in excess meltwater collected during the BE-OI slow CFA campaign.

How to cite: Tetzner, D., Allen, C., Segato, D., Veale, J., Harris-Stuart, R., and Westhoff, J.: Windblown diatoms at Little Dome C and their potential for reconstructing Southern Hemisphere Westerly Winds during the MPT , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22482, https://doi.org/10.5194/egusphere-egu26-22482, 2026.