Abstract
In recent decades computer modelling of iceberg drift has passed through two cycles of interest. Navigation in ice-infested waters and the security of off-shore structures motivated such studies in the 1970s whereas in the 1990s the focus shifted to paleoclimate and ocean dynamics. Although the underlying physics remains the same, the requirements of the two types of models differ. We characterize these separate questions as the “Titanic problem” and the “Heinrich problem.” In the Titanic problem the objective is to predict the trajectory of individual icebergs with the aim of evaluating the risk of collision with maritime traffic or fixed offshore structures. In the Heinrich problem the objective is to predict the temporally-evolving spatial pattern of iceberg meltwater and the associated pattern and provenance of ice-rafted marine sedimentation.
And out there in the starlight, with no trace
Upon it of its deed but the last wave
Prom the Titanic fretting at its base,
Silent, composed, ringed by its icy broods,
The grey shape with the palaeolithic face,
Was still the master of the longitudes.
(E. J. Pratt, from The Titanic)
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Clarke, G.K.C., La Prairie, D.I. (2001). Modelling Iceberg Drift and Ice-Rafted Sedimentation. In: Straughan, B., Greve, R., Ehrentraut, H., Wang, Y. (eds) Continuum Mechanics and Applications in Geophysics and the Environment. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-04439-1_11
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DOI: https://doi.org/10.1007/978-3-662-04439-1_11
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