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- W2286585385 abstract "Calving of Antarctic tabular icebergs is a decisive factor in the overall mass budget of the Antarctic ice sheet. With an ice loss of about 2000 Gt per year it is by far the largest negative term in the mass balance equation (surface ablation ~30 Gt yr, basal melting ~550 Gt yr. Jacobs et al., 1992). The processes triggering melting and decay of tabular icebergs are of great relevance within many domains. Being a source of cold freshwater during their drift and especially during their final decay, tabular icebergs have a significant impact on Southern Ocean water masses (Gladstone et al., 2001). Dust particles enclosed in the ice, released during melting processes, can have a fertilizing effect on algae in the upper water column. Thus, melting icebergs can also affect biology (Arrigo et al, 2002). Furthermore the decay processes of icebergs are of great interest to shipping, as fast disintegrating icebergs, releasing a huge amount of smaller icebergs in short time, can be a severe threat to shipping lines in the Southern Ocean. In spite of its apparent relevance, little is known about tabular iceberg evolution and decay at the moment. To learn more about the role of ice dynamics in these processes, we simulate the inherent dynamics and evolution of gigantic tabular icebergs, by applying the numerical iceberg model COMBATIS (Computer-based Tabular Iceberg Simulator) based on the fundamental equations of ice shelf dynamics. In the following we will depict the evolution of a typical Antarctic tabular iceberg and present results of a simulation with the model COMBATIS (Jansen et al., submitted)." @default.
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- W2286585385 date "2005-01-01" @default.
- W2286585385 modified "2023-09-27" @default.
- W2286585385 title "Evolution of tabular iceberg A-38B, observation and simulation" @default.
- W2286585385 hasPublicationYear "2005" @default.
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