Brine flow in permafrost, time constraints by Ra isotopes&nbsp;

Yishai Weinstein; Dotan Rotem; Yehudit Harlavan; Hanne H. Christiansen

doi:https://doi.org/10.5194/egusphere-egu26-12264

[Back] [Session CR6.8]

EGU26-12264, updated on 14 Mar 2026

https://doi.org/10.5194/egusphere-egu26-12264

EGU General Assembly 2026

© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.

Brine flow in permafrost, time constraints by Ra isotopes

Yishai Weinstein¹, Dotan Rotem^1,2, Yehudit Harlavan³, and Hanne H. Christiansen⁴

Yishai Weinstein et al.

¹Bar-Ilan University, Department of Environment, Planning and Sustainability, Ramat-Gan, 52900 Israel
²Arctic Geophysics Department, the University Centre in Svalbard, UNIS, Longyearbyen, Norway
³Geological Survey of Israel, 32 Yesha'yahu Leibowitz, Jerusalem 9692100, Israel
⁴Department of Environmental Sciences, Aarhus University, Risø, Denmark

How to cite: Weinstein, Y., Rotem, D., Harlavan, Y., and Christiansen, H. H.: Brine flow in permafrost, time constraints by Ra isotopes , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12264, https://doi.org/10.5194/egusphere-egu26-12264, 2026.

This abstract has been withdrawn after no-show on 11 Aug 2026.