Abstract
In polar regions, the exchange of heat, fresh water and salt water, and
momentum between ocean and atmosphere is strongly affected by the presence
of sea-ice cover. As a growing number of climate models include a
dynamic–thermodynamic sea-ice component to take these effects into account,
it might be asked whether sea ice is adequately represented in these
simulations, and how far these simulations fit with physical
observations.Sea ice in the classical models (Hibler,
1979; Parkinson and Washington,
1979) that have been available for two decades, is regarded as a
two-dimensional (2-D) continuum covering the ocean surface. The prognostic
variables describing the ice pack are horizontal ice velocity, areal
coverage (ice concentration), and ice thickness. In numerical models, these
variables and their evolution in space and time are solved on an Eulerian
grid.A number of observational data are available to verify the model results.
Sea-ice drift is observed from drifting buoys deployed on ice floes. Areal
sea-ice coverage can be observed with satellite-borne passive-microwave
sensors (SMMR, SSM/I). For ice thickness, which cannot be observed with
remote-sensing techniques, rather few, scattered observations from
upward-looking sonars on submarines and moorings are available.This article gives an overview of three additional variables representing
sea ice in large-scale climate models. These are (1) roughness, (2) age of
the ice, introduced as two prognostic variables, and (3) simulated
trajectories of ice motion, which are diagnosed from the Eulerian velocity
grid. The new variables enable a more detailed look at sea ice in models,
helping to understand better the coupled dynamic–thermodynamic processes
determining the polar ice cover. Further, the new variables offer important,
additional possibilities for comparing the simulated sea-ice properties with
available observations.
Publisher
International Glaciological Society
Cited by
11 articles.
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