Preprints
https://doi.org/10.5194/egusphere-2024-3220
https://doi.org/10.5194/egusphere-2024-3220
04 Feb 2025
 | 04 Feb 2025
Status: this preprint is open for discussion and under review for Geoscientific Model Development (GMD).

Implementation of an intermediate complexity snow-physics scheme (ISBA-Explicit Snow) into a sea-ice model (SI3): 1D thermodynamic coupling and validation

Théo Brivoal, Virginie Guemas, Martin Vancoppenolle, Clément Rousset, and Bertrand Decharme

Abstract. Snow plays a crucial role in the formation and sustainability of sea ice. Due to its thermal properties, snow acts as an insulating layer, shielding the ice from the air above. This insulation reduces the heat transfer between the sea-ice and the atmosphere. Due to its reflective properties, the snow cover also strongly contributes to albedo over ice-covered regions, which gives it a significant role in the earth's climate system.

Current state-of-art climate models use over-simple representations of the snow cover overlaying the sea ice. The snow cover is often represented with a one-layer scheme, assuming a constant density, no wet or dry metamorphism or assuming that no liquid water is stored in the snow. Here we implemented an intermediate complexity snow-physics scheme (ISBA-Explicit Snow) into a sea-ice model (SI3), which serves as the sea-ice component for upcoming versions of the CNRM-CM climate model. This is, to our knowledge, the first time that a snow model with such level of complexity is incorporated into a sea-ice model designed for global to regional applications. We validated our model comparing 1D simulations with data from the Surface Heat Budget of the Arctic Ocean (SHEBA) but also simulations from another advanced snow-on-sea-ice model (SnowModel-LG), and simulations with the previous SI3 snow scheme.

Our model simulates realistic snow thicknesses, densities, and temperatures, aligning well with SHEBA observations and SnowModel-LG outputs, while capturing their temporal variability. We show that the thickness, density, and conductivity of the snowpack are significantly affected by the choices made in parameterization for calculating snowfall density, wind-induced snow compaction, and by the choice of the atmospheric forcing. Unlike the previous SI3 snow scheme that assumed constant density and thermal conductivity, our model realistically simulates the evolution of these properties, resulting in more accurate temperatures at the snow-ice interface. Ultimately, our study shows that modelling the temporal changes in the density and thermal conductivity of the snow layers leads to a more accurate representation of heat transfer between the underlying sea ice and the atmosphere.

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Théo Brivoal, Virginie Guemas, Martin Vancoppenolle, Clément Rousset, and Bertrand Decharme

Status: open (until 01 Apr 2025)

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Théo Brivoal, Virginie Guemas, Martin Vancoppenolle, Clément Rousset, and Bertrand Decharme
Théo Brivoal, Virginie Guemas, Martin Vancoppenolle, Clément Rousset, and Bertrand Decharme

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Short summary
Snow in polar regions is key to sea ice formation and the Earth's climate, but current climate models simplify snow cover on sea ice. This study integrates an intermediate complexity snow-physics scheme into a sea-ice model designed for climate applications. We show that modelling the temporal changes in properties such as the density and thermal conductivity of the snow layers leads to a more accurate representation of heat transfer between the underlying sea ice and the atmosphere.
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