Abstract

Accurate circum-Antarctic sea-ice thickness is urgently required to better understand the different sea-ice cover evolution in both polar regions. Satellite radar and laser altimetry are currently the most promising tools for sea-ice thickness retrieval. We present qualitative inter-comparisons of winter and spring circum-Antarctic sea-ice thickness computed with different approaches from Ice Cloud and land Elevation Satellite (ICESat) laser altimeter total (sea ice plus snow) freeboard estimates. We find that approach A, which assumes total freeboard equals snow depth, and approach B, which uses empirical linear relationships between freeboard and thickness, provide the lowest sea-ice thickness and the smallest winter-to-spring increase in seasonal average modal and mean sea-ice thickness: A: 0.0 m and 0.04 m, B: 0.17 and 0.16 m, respectively. Approach C uses contemporary snow depth from satellite microwave radiometry, and we derive comparably large sea-ice thickness. Here we observe an unrealistically large winter-to-spring increase in seasonal average modal and mean sea-ice thickness of 0.68 m and 0.65 m, respectively, which we attribute to biases in the snow depth. We present a conceptually new approach D. It assumes that the two-layer system (sea ice, snow) can be represented by one layer. This layer has a modified density, which takes into account the influence of the snow on sea-ice buoyancy. With approach D we obtain thickness values and a winter-to-spring increase in average modal and mean sea-ice thickness of 0.17 m and 0.23 m, respectively, which lay between those of approaches B and C. We discuss retrieval uncertainty, systematic uncertainty sources, and the impact of grid resolution. We find that sea-ice thickness obtained with approaches C and D agrees best with independent sea-ice thickness information—if we take into account the potential bias of in situ and ship-based observations.

Highlights

  • Antarctic sea ice plays a key role in the ocean-atmosphere heat, impulse, and matter exchange and is of profound importance for species as living and hatching ground

  • What alternatives do exist? Ship-based visual observations carried out according to the Antarctic Sea Ice Processes and Climate (ASPeCt) protocol [5,6] are of limited spatio-temporal coverage as well, as illustrated by the track maps shown in [7]

  • Thicker sea ice is found along the East Antarctic coast, in some coastal areas in the Amundsen Sea, and in the Weddell Sea

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Summary

Introduction

Antarctic sea ice plays a key role in the ocean-atmosphere heat, impulse, and matter exchange and is of profound importance for species as living and hatching ground. One of the key shortcoming in future climate scenario investigations as well as in the understanding of the inter-annual regional Antarctic sea-ice extent variability is given by the still widely unknown Antarctic sea-ice thickness distribution. Upward looking sonar (ULS) data are—in contrast to the Arctic—only available from moorings [8,9] and provide very useful temporal but quite limited spatial information about sea-ice thickness. Satellite remote sensing is required to obtain a circum-Antarctic sea-ice thickness distribution

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