EGU25-1189, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-1189
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Friday, 02 May, 10:45–12:30 (CEST), Display time Friday, 02 May, 08:30–12:30
 
Hall X5, X5.246
Neogene circulation in Princess Elizabeth Trough, Southern Ocean, driven by gyres?
Gabriele Uenzelmann-Neben
Gabriele Uenzelmann-Neben
  • Alfred-Wegener-Institut, Geophysics, Bremerhaven, Germany (gabriele.uenzelmann-neben@awi.de)

The atmospheric CO2 content has been discussed as one of the major factors influencing global climate. In the framework of the deep ocean forming the main reservoir of carbon dioxide, the Southern Ocean plays a crucial role in partitioning carbon between the atmosphere and the deep ocean. The processes resulting in the variability of atmospheric CO2 and carbon uptake in the deep ocean have not yet been fully identified. Sedimentary structures imaged with seismic reflection data are interpreted regarding direction and intensity of pathways of deep/bottom water masses to contribute to the knowledge on potential locations of carbon subsidence. Under the assumption that the general circulation scheme has been similar during the Neogene, i.e., driven by gyres, the positions and sizes of palaeo-gyres have been reconstructed, which were then interpreted regarding the intensity of carbon uptake. This has been compared with published reconstruction of warming/cooling trends of the global climate. While the method applied is equivocal it links observed sedimentary structures with the development of gyres thus potential sports of carbon uptake. This way the presented reconstruction provides pieces to the climate variability puzzle, which can be tested using numerical simulation.

How to cite: Uenzelmann-Neben, G.: Neogene circulation in Princess Elizabeth Trough, Southern Ocean, driven by gyres?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1189, https://doi.org/10.5194/egusphere-egu25-1189, 2025.