Abstract

Abstract. The Antarctic continent is a vast desert and is the coldest and the most unknown area on Earth. It contains the Antarctic ice sheet, the largest continental water reservoir on Earth that could be affected by the current global warming, leading to sea level rise. The only significant supply of ice is through precipitation, which can be observed from the surface and from space. Remote-sensing observations of the coastal regions and the inner continent using CloudSat radar give an estimated rate of snowfall but with uncertainties twice as large as each single measured value, whereas climate models give a range from half to twice the space–time-averaged observations. The aim of this study is the evaluation of the vertical precipitation rate profiles of CloudSat radar by comparison with two surface-based micro-rain radars (MRRs), located at the coastal French Dumont d'Urville station and at the Belgian Princess Elisabeth station located in the Dronning Maud Land escarpment zone. This in turn leads to a better understanding and reassessment of CloudSat uncertainties. We compared a total of four precipitation events, two per station, when CloudSat overpassed within 10 km of the station and we compared these two different datasets at each vertical level. The correlation between both datasets is near-perfect, even though climatic and geographic conditions are different for the two stations. Using different CloudSat and MRR vertical levels, we obtain 10 km space-scale and short-timescale (a few seconds) CloudSat uncertainties from −13 % up to +22 %. This confirms the robustness of the CloudSat retrievals of snowfall over Antarctica above the blind zone and justifies further analyses of this dataset.

Highlights

  • In the context of global warming, predicting the evolution of the Antarctic ice sheet is a major challenge

  • Focusing on the Dumont d’Urville station, Fig. 3a shows a good agreement between CloudSat and the micro-rain radars (MRRs)’s snowfall rates for each vertical level

  • The MRR profile presents a maximum of the snowfall rate of 0.75 mm h−1 at 750 m and an inversion of the precipitation rate likely due to low-level sublimation processes, whereas the ground clutter prevents CloudSat from seeing the inversion

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Summary

Introduction

In the context of global warming, predicting the evolution of the Antarctic ice sheet is a major challenge. Snowfall is the main input of the ice sheet mass balance, but it is difficult to estimate its amount. Precipitation characteristics depend on the region of Antarctica. Precipitation is influenced by cyclones and fronts (Bromwich, 1988), and a few times a year these fronts intrude on the high continental plateau, likely bringing most of the snow accumulation (Genthon et al, 2016). The remaining annual precipitation rate is in the form of “diamond dust” (thin ice crystals) under clear-sky conditions (Bromwich, 1988; Fujita and Abe, 2006)

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