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@comment{{This file has been generated by bib2bib 1.95}}
@comment{{Command line: /usr/bin/bib2bib --quiet -c 'not journal:"Discussions"' -c 'not journal:"Polymer Science"' -c '  author:"Sadourny"  ' -c year=1982 -c $type="ARTICLE" -oc lmd_Sadourny1982.txt -ob lmd_Sadourny1982.bib /home/WWW/LMD/public/}}
  author = {{Sadourny}, R. and {Hoyer}, J.-M.},
  title = {{Inhibition of Baroclinic Instability in Low-Resolution Models.}},
  journal = {Journal of Atmospheric Sciences},
  year = 1982,
  month = oct,
  volume = 39,
  pages = {2138-2143},
  abstract = {{The inhibition of baroclinic instability in low-resolution
quasi-geostrophic models is studied using a simplified second-order
closure approximation. It is shown that this inhibition, which results
in systematic overestimation of baroclinic energy and systematic
underestimation of barotropic energy, is the result of spurious energy
dissipation due to the use of inadequate lateral diffusion.
Consequently, a possible methodology for the parameterization of
baroclinic instability in low-resolution models is proposed, based on
the construction of diffusion operators able to dissipate potential
enstrophy while conserving energy exactly.
  doi = {10.1175/1520-0469(1982)039<2138:IOBIIL>2.0.CO;2},
  adsurl = {},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
  author = {{Hoyer}, J.-M. and {Sadourny}, R.},
  title = {{Closure Modeling of Fully Developed Baroclinic Instability.}},
  journal = {Journal of Atmospheric Sciences},
  year = 1982,
  month = apr,
  volume = 39,
  pages = {707-721},
  abstract = {{Simple second-order closure models of quasi-geostrophic turbulence are
derived, applying either to two-layer flows within isentropic
boundaries, or to Eady-type frontogenesis with vanishing potential
vorticity; homogeneity and horizontal isotropy are used as simplifying
assumptions. Long-term numerical integrations of the two models are
performed to obtain the structure of regime flows under stationary
large-scale baroclinic forcing. The various cascade processes and the
corresponding inertial ranges are discussed and visualized, showing
characteristic differences between fully developed baroclinic
instability and the linear theory. Further applications of such models
may include studies of truncation effects on the efficiency of
baroclinic instability.
  doi = {10.1175/1520-0469(1982)039<0707:CMOFDB>2.0.CO;2},
  adsurl = {},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
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