Preprints
https://doi.org/10.5194/egusphere-2025-2104
https://doi.org/10.5194/egusphere-2025-2104
21 May 2025
 | 21 May 2025
Status: this preprint is open for discussion and under review for Climate of the Past (CP).

Ice core site considerations from modeling CO2 and O2/N2 ratio diffusion in interior East Antarctica

Marc J. Sailer, Tyler J. Fudge, John D. Patterson, Shuai Yan, Duncan A. Young, Shivangini Singh, Don Blankenship, and Megan Kerr

Abstract. Obtaining a continuous ice core record to 1.5 million years (Ma), which spans the Mid-Pleistocene Transition (MPT, 1.2 to 0.7 Ma) is a goal of multiple international efforts in Antarctica. Ice of such age is likely to be highly thinned and located in warm ice near the bed, conditions which promote diffusion of the stored atmospheric gases. Here, we assess the preservation of CO2 and the O2/N2 ratio in the ice sheet between South Pole and Dome A where the NSF Center for Oldest Ice Exploration has surveyed with airborne radar. We employ two models: 1) a 1D, steady state ice and heat flow model to calculate the temperature and age of ice with respect to depth, and 2) a vertical gas diffusion model for clathrate ice. We analyze the preservation of CO2 signals with a period of 40 kyr to match pre-MPT glacial cycles and the preservation of O2/N2 signals with a period of 20 kyr to match precession cycles. 1.5 Ma ice is lost to basal melt in much of the study area where ice thickness exceeds 3000 m. In locations that preserve 1.5 Ma ice, vertical gas diffusion is most sensitive to accumulation rate; high accumulation rate sites have more highly thinned old ice, and the steeper gas concentration gradients enhance diffusion. The most promising region for recovering 1.5 Ma ice is the foothills of Dome A, approximately 400 km from both South Pole and Dome A, due to low accumulation rates and moderate ice thickness. CO2 signals lose on average 14 % of their amplitude, while O2/N2 signals lose on average 95 % for 1.5 Ma ice, suggesting precession cycles may not be identifiable. Unknown geothermal heat flow is a large uncertainty for both ice loss from basal melt and gas signal preservation.

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Marc J. Sailer, Tyler J. Fudge, John D. Patterson, Shuai Yan, Duncan A. Young, Shivangini Singh, Don Blankenship, and Megan Kerr

Status: open (until 16 Jul 2025)

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Marc J. Sailer, Tyler J. Fudge, John D. Patterson, Shuai Yan, Duncan A. Young, Shivangini Singh, Don Blankenship, and Megan Kerr

Model code and software

Ice sheet gas diffusion model Marc Sailer et al. https://doi.org/10.5281/zenodo.15347004

Marc J. Sailer, Tyler J. Fudge, John D. Patterson, Shuai Yan, Duncan A. Young, Shivangini Singh, Don Blankenship, and Megan Kerr

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Short summary
In this study, we model vertical atmospheric gas diffusion in ice older than 1 million years in the Antarctic ice sheet. We estimate climate signal preservation and help identify a potential region for a future deep ice core in East Antarctica. We find that regions with low accumulation rates and moderate ice thickness result in lower diffusion rates. In particular, the foothills of Dome A is a promising location for a deep ice core that extends the present ice core record.
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