4.6 Article

Deep mixed ocean volume in the Labrador Sea in HighResMIP models

期刊

CLIMATE DYNAMICS
卷 57, 期 7-8, 页码 1895-1918

出版社

SPRINGER
DOI: 10.1007/s00382-021-05785-x

关键词

Deep oceanic convection in the Labrador Sea; High resolution global climate modeling; Impact of increasing the resolution in global climate models; Climate variability; Atlantic meridional overturning circulation

资金

  1. PRIMAVERA project - European Union's Horizon 2020 programme [641727]
  2. Ministry of Science and Higher Education of Russia [0128-2021-0014]
  3. Spanish Ministry of Economy, Industry and Competiveness [RYC-2017-22772]
  4. NOAA Climate Observations and Monitoring (COM) program
  5. NERC [noc010010] Funding Source: UKRI

向作者/读者索取更多资源

The study indicates that most climate models overestimate deep convection in the Labrador Sea, increasing ocean resolution leads to increased deep mixing, and increasing atmospheric resolution has a smaller effect. Simulated convection in the Labrador Sea is mainly influenced by heat release from the ocean to the atmosphere and vertical water mass stratification. Sub-grid scale mixing processes in the models might be imperfect and contribute to biases in deep convection.
Simulations from seven global coupled climate models performed at high and standard resolution as part of the high resolution model intercomparison project (HighResMIP) are analyzed to study deep ocean mixing in the Labrador Sea and the impact of increased horizontal resolution. The representation of convection varies strongly among models. Compared to observations from ARGO-floats and the EN4 data set, most models substantially overestimate deep convection in the Labrador Sea. In four out of five models, all four using the NEMO-ocean model, increasing the ocean resolution from 1 degrees to 1/4 degrees leads to increased deep mixing in the Labrador Sea. Increasing the atmospheric resolution has a smaller effect than increasing the ocean resolution. Simulated convection in the Labrador Sea is mainly governed by the release of heat from the ocean to the atmosphere and by the vertical stratification of the water masses in the Labrador Sea in late autumn. Models with stronger sub-polar gyre circulation have generally higher surface salinity in the Labrador Sea and a deeper convection. While the high-resolution models show more realistic ocean stratification in the Labrador Sea than the standard resolution models, they generally overestimate the convection. The results indicate that the representation of sub-grid scale mixing processes might be imperfect in the models and contribute to the biases in deep convection. Since in more than half of the models, the Labrador Sea convection is important for the Atlantic Meridional Overturning Circulation (AMOC), this raises questions about the future behavior of the AMOC in the models.

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