| Working Group I: The Scientific Basis | 
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14.2.3.2 Thermohaline circulationIn the oceanic component of climate models, ocean current patterns are represented 
  significantly better in models of higher resolution in large part because ocean 
  current systems (including mesoscale eddies), ocean variability (including ENSO 
  events), and the thermohaline circulation (and other vertical mixing processes) 
  and topography which greatly influence the ocean circulation, can be better 
  represented. Improved resolution and understanding of the important facets of 
  coupling in both atmosphere and ocean components of global climate models have 
  also been proven to reduce flux imbalance problems arising in the coupling of 
  the oceanic and the atmospheric components. However, it must still be noted 
  that uncertainties associated with clouds still cause problems in the computation 
  of surface fluxes. With the availability of computer power, a central impediment 
  to the gain in model accuracy is being reduced; however, there is still a long 
  way to go before many of the important processes are explicitly resolved by 
  the numerical grid. In addition there continues to be a necessary “concomitant” 
  increase in resources for process studies and for diagnosis as computer power 
  increases. It must still be remembered that the system presents chaotic characteristics 
  that can only be evaluated through an analysis of ensembles statistics, and 
  these ensembles must be generated by running suites of models under varied initial 
  and forcing conditions.  In a few model calculations, a large rate of increase in the radiative forcing 
  of the planet is enough to cause the ocean’s global thermohaline circulation 
  almost to disappear, though in some experiments it reappears given sufficiently 
  long integration times (see Chapter 7, Section 7.3.7 
  and Chapter 9, 9.3.4.3). This circulation is important 
  because in the present climate it is responsible for a large portion of the 
  heat transport from the tropics to higher latitudes, and it plays an important 
  role in the oceanic uptake of CO2. Palaeo-oceanographic investigations suggest 
  that aspects of longer-term climate change are associated with changes in the 
  ocean’s thermohaline circulation. We need appropriate observations of the 
  thermohaline circulation, and its natural variations, to compare with model 
  simulations (see Chapter 9, Section 9.3.4.3; see also 
  Chapter 7, Section 7.6 and Chapter 8, 
  Section 8.5.2.2). The coming decade will be important for ocean circulation in the context of 
  climate. A particularly exciting development is the potential for assimilating 
  synoptic ocean observations (e.g., the US/French ocean TOPography satellite 
  altimeter EXperiment (TOPEX-POSEIDON) and Argo) into ocean general circulation 
  models. Key questions, such as how well do the ocean models capture the inferred 
  heat flux or tracer distributions, are central to the use of these models in 
  climate studies. The effort of comparing models with data, as the direct path 
  for model rejection and model improvement, is central to increasing our understanding 
  of the system. 14.2.3.3 Arctic sea ice
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