2001
DOI: 10.1007/s10236-001-8173-5
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The effect of flow at Maud Rise on the sea-ice cover – numerical experiments

Abstract: The role of seamounts in the formation and evolution of sea ice is investigated in a series of numerical experiments with a coupled sea ice±ocean model. Bottom topography, strati®cation and forcing are con®gured for the Maud Rise region in the Weddell Sea. The speci®c¯ow regime that develops at the seamount as the combined response to steady and tidal forcing consists of free and trapped waves and a vortex cap, which is caused by mean¯ow and tidal¯ow recti®cation. The enhanced variability through tidal motion … Show more

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Cited by 34 publications
(32 citation statements)
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“…After the sea ice melted, high CFC fluxes persist (see Section 4.1) until sea ice growth again suppresses the gas exchange. This is confirmed 663 by independent simulations of the complex flow regime at Maud Rise (Beckmann et al, 2001) and by observed upwelling of subsurface water masses (Muench et al, 2001).…”
supporting
confidence: 60%
“…After the sea ice melted, high CFC fluxes persist (see Section 4.1) until sea ice growth again suppresses the gas exchange. This is confirmed 663 by independent simulations of the complex flow regime at Maud Rise (Beckmann et al, 2001) and by observed upwelling of subsurface water masses (Muench et al, 2001).…”
supporting
confidence: 60%
“…In September, the Antarctic sea-ice edge in the ACCESS runs tends to extend too far north as illustrated by the positive sea-ice concentration biases in Figs 5(f) and 5(g). Around Maud Rise, however, negative sea-ice concentration biases along with a deep mixed layer exist consistent with a too convective ocean releasing oceanic heat to melt the ice in winter (Beckmann et al 2001, Sirevaag et al 2010, Marsland et al 2012. CSIRO-Mk3.6 sea-ice concentration biases in September are relatively small with too much sea-ice in the northern Weddell Sea and too little sea-ice in the Amundsen Sea.…”
Section: Resultsmentioning
confidence: 97%
“…This was followed, from 11 to 29 August, by a larger polynya in the Cosmonaut Sea (~40°-50°E, 66°S). Polynyas are thought to recur in these areas due to a combination of oceanic and atmospheric forcing (e.g., Holland 2000; Beckmann et al 2001;Arbetter et al 2004). Analysis within the Southern Ocean section of this chapter (6g) suggests that the Maud Rise polynya in 2016 was probably related to increased deep convection due to the higher-thanaverage salinity in that region.…”
Section: E Seasonal Melt Extent and Duration-l Wang And H Liumentioning
confidence: 84%