4.5 Article

The North Atlantic subpolar circulation in an eddy-resolving global ocean model

Journal

JOURNAL OF MARINE SYSTEMS
Volume 142, Issue -, Pages 126-143

Publisher

ELSEVIER
DOI: 10.1016/j.jmarsys.2014.10.007

Keywords

Ocean modelling; Eddy-resolving; NEMO; North Atlantic; Subpolar gyre warming; Physical oceanography

Funding

  1. People Programme (Marie Curie Actions) of the European Union 7th Framework Programme (FP7) [29020]
  2. FP7 through the NACLIM project [308299]
  3. MASTS pooling initiative (Marine Alliance for Science and Technology for Scotland - Scottish Funding Council) [HR09011]
  4. NERC's National Capability Programme
  5. NERC [NE/K010700/1, NE/M005097/1, NE/K010875/1, noc010010] Funding Source: UKRI
  6. Natural Environment Research Council [NE/K010700/1, NE/M005097/1, noc010012, NE/K010875/1, noc010010] Funding Source: researchfish

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The subpolar North Atlantic represents a key region for global climate, but most numerical models still have well-described limitations in correctly simulating the local circulation patterns. Here, we present the analysis of a 30year run with a global eddy-resolving (1/12 degrees) version of the NEMO ocean model. Compared to the 1 degrees and 1/4 degrees equivalent versions, this simulation more realistically represents the shape of the Subpolar Gyre, the position of the North Atlantic Current, and the Gulf Stream separation. Other key improvements are found in the representation of boundary currents, multi-year variability of temperature and depth of winter mixing in the Labrador Sea, and the transport of overflows at the Greenland-Scotland Ridge. However, the salinity, stratification and mean depth of winter mixing in the Labrador Sea, and the density and depth of overflow water south of the sill, still present challenges to the model. This simulation also provides further insight into the spatio-temporal development of the warming event observed in the Subpolar Gyre in the mid 1990s, which appears to coincide with a phase of increased eddy activity in the southernmost part of the gyre. This may have provided a gateway through which heat would have propagated into the gyre's interior. (C) 2014 The Authors. Published by Elsevier B.V.

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