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Sea ice motion and open water area at the Ronne Polynia, Antarctica: Synthetic aperture radar observations versus model results
Author(s) -
Hollands T.,
Haid V.,
Dierking W.,
Timmermann R.,
Ebner L.
Publication year - 2013
Publication title -
journal of geophysical research: oceans
Language(s) - English
Resource type - Journals
eISSN - 2169-9291
pISSN - 2169-9275
DOI - 10.1002/jgrc.20158
Subject(s) - forcing (mathematics) , geology , katabatic wind , sea ice , climatology , satellite , synthetic aperture radar , radar , meteorology , remote sensing , geography , physics , telecommunications , computer science , astronomy
This study deals with observations and simulations of the evolution of coastal polynias focusing on the Ronne Polynia. We compare differences in polynia extent and ice drift patterns derived from satellite radar images and from simulations with the Finite Element Sea Ice Ocean Model, employing three atmospheric forcing data sets that differ in spatial and temporal resolution. Two polynia events are analyzed, one from austral summer and one from late fall 2008. The open water area in the polynia is of similar size in the satellite images and in the model simulations, but its temporal evolution differs depending on katabatic winds being resolved in the atmospheric forcing data sets. Modeled ice drift is slower than the observed and reveals greater turning angles relative to the wind direction in many cases. For the summer event, model results obtained with high‐resolution forcing are closer to the drift field derived from radar imagery than those from coarse resolution forcing. For the late fall event, none of the forcing data yields outstanding results. Our study demonstrates that a dense (1–3 km) model grid and atmospheric forcing provided at high spatial resolution ( < 50 km) are critical to correctly simulate coastal polynias with a coupled sea‐ice ocean model.