lmd_Codron2012.bib

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@article{2012JAtS...69.3788A,
  author = {{Arakelian}, A. and {Codron}, F.},
  title = {{Southern Hemisphere Jet Variability in the IPSL GCM at Varying Resolutions}},
  journal = {Journal of Atmospheric Sciences},
  year = 2012,
  month = dec,
  volume = 69,
  pages = {3788-3799},
  doi = {10.1175/JAS-D-12-0119.1},
  adsurl = {http://adsabs.harvard.edu/abs/2012JAtS...69.3788A},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2012JCli...25.1847B,
  author = {{Brachet}, S. and {Codron}, F. and {Feliks}, Y. and {Ghil}, M. and 
	{Le Treut}, H. and {Simonnet}, E.},
  title = {{Atmospheric Circulations Induced by a Midlatitude SST Front: A GCM Study}},
  journal = {Journal of Climate},
  year = 2012,
  month = mar,
  volume = 25,
  pages = {1847-1853},
  doi = {10.1175/JCLI-D-11-00329.1},
  adsurl = {http://adsabs.harvard.edu/abs/2012JCli...25.1847B},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2012ClDy...38..379C,
  author = {{Codron}, F.},
  title = {{Ekman heat transport for slab oceans}},
  journal = {Climate Dynamics},
  keywords = {Slab ocean, Ekman, Heat transport},
  year = 2012,
  month = jan,
  volume = 38,
  pages = {379-389},
  abstract = {{A series of schemes designed to include various representations of the
Ekman-driven heat fluxes in slab-ocean models is introduced. They work
by computing an Ekman mass flux, then deducing heat fluxes by the
surface flow and an opposite deep return flow. The schemes differ by the
computation of the return flow temperature: either diagnosed from the
SST or given by an active second layer. Both schemes conserve energy,
and use as few parameters as possible. Simulations in an aquaplanet
setting show that the schemes reproduce well the structure of the
meridional heat transport by the ocean. Compared to a diffusive
slab-ocean, the simulated SST is more flat in the tropics, and presents
a relative minimum at the equator, shifting the ITCZ into the summer
hemisphere. In a realistic setting with continents, the slab model
simulates correctly the mean state in many regions, especially in the
tropics. The lack of other dynamical features, such as barotropic gyres,
means that an optimal mean-state in regions such as the mid-latitudes
will require additional flux corrections.
}},
  doi = {10.1007/s00382-011-1031-3},
  adsurl = {http://adsabs.harvard.edu/abs/2012ClDy...38..379C},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}