Articles | Volume 19, issue 10
https://doi.org/10.5194/tc-19-4125-2025
https://doi.org/10.5194/tc-19-4125-2025
Research article
 | 
01 Oct 2025
Research article |  | 01 Oct 2025

Age, thinning and spatial origin of the Beyond EPICA ice from a 2.5D ice flow model

Ailsa Chung, Frédéric Parrenin, Robert Mulvaney, Luca Vittuari, Massimo Frezzotti, Antonio Zanutta, David A. Lilien, Marie G. P. Cavitte, and Olaf Eisen

Viewed

Total article views: 3,750 (including HTML, PDF, and XML)
HTML PDF XML Total Supplement BibTeX EndNote
2,906 758 86 3,750 131 89 121
  • HTML: 2,906
  • PDF: 758
  • XML: 86
  • Total: 3,750
  • Supplement: 131
  • BibTeX: 89
  • EndNote: 121
Views and downloads (calculated since 14 Jun 2024)
Cumulative views and downloads (calculated since 14 Jun 2024)

Viewed (geographical distribution)

Total article views: 3,750 (including HTML, PDF, and XML) Thereof 3,686 with geography defined and 64 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 29 Jan 2026
Short summary
We applied an ice flow model to a flow line from the summit of Dome C to the Beyond EPICA ice core drill site on Little Dome C in Antarctica. Results show that the oldest ice at the drill site may be 1.12 Ma (at an age density of 20 kyr m-1) and originate from around 15 km upstream. We also discuss the nature of the 200–250 m thick basal layer which could be composed of stagnant ice, disturbed ice or even accreted ice (possibly containing debris).
Share