EGU25-20052, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-20052
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Friday, 02 May, 14:00–15:45 (CEST), Display time Friday, 02 May, 14:00–18:00
 
Hall X4, X4.26
Snow Microstructure over Antarctic Landfast Ice
Ruzica Dadic1,2, Julia Martin2, Roberta Pirazzini3, Brian Anderson2, Martin Schneebeli1, Matthias Jaggi1, Amy Macfarlane4, Michael Lehning1, Nander Wever1, and Petra Heil5
Ruzica Dadic et al.
  • 1WSL Institute for Snow and Avalanche Research SLF, Snow and Atmosphere, Davos Dorf, Switzerland (ruzica.dadic@slf.ch)
  • 2Antarctic Research Centre, Victoria University of Wellington, Wellington, New Zealand
  • 3Finnish Meteorological Institute FMI, Helsinki, Finnland
  • 4UiT The Arctic University of Norway, Tromsø, Norway
  • 5Australian Antarctic Program, Hobart, Australia
Landfast ice plays a significant role in climate and ecosystems in Antarctic coastal regions. From October to December 2022, we investigated the physical properties of snow and sea ice on Antarctic landfast ice in McMurdo Sound, following the protocols from the MSOAiC expedition. Our measurements confirmed some findings from MOSAiC (e.g. the potential mass transfer from the sea ice surface to snow , the high spatial variability of snow depth}, and the discrepancy between meteorological snowfall and snow accumulation),  but we also had observations that were contrasting our MOSAiC data, for example: 1) presence of salt up to 15 cm of snow height (as opposed to MOSAiC's 5 cm for a relatively similar total snow height), 2) the lack of the surface scattering layer on melting sea ice, which caused significantly lower albedos of bare sea ice (0.45, as opposed to MOSAiC's 0.65), 3) average densities of non-melting snow of 450 kg/m3 (as opposed to MOSAIC'S 350 kg/m3 ). Here, we will discuss the microCT measurements from our samples and relate them to the macroscale obervations of parameters like snow density, snow height, snow surface roughness, salinity or stable water isotopes. The main focus in this study in on the prevalance of a prominent depth hoar layer at the snow-ice interface, which we to be caused by the mass transfer between snow and ice because of the large vertical temperature gradients. This is also visible by the microscale roughness of the interface. Additionally, we will discuss the microstructure of the extremely dense wind slab that dominates most of the snow profile and the implications of these findings for modelling and remote sensing of snow on sea ice. 
 
 

How to cite: Dadic, R., Martin, J., Pirazzini, R., Anderson, B., Schneebeli, M., Jaggi, M., Macfarlane, A., Lehning, M., Wever, N., and Heil, P.: Snow Microstructure over Antarctic Landfast Ice, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20052, https://doi.org/10.5194/egusphere-egu25-20052, 2025.