dc.creatorScheffler, Guillermo Federico
dc.creatorPulido, Manuel Arturo
dc.date.accessioned2017-09-13T17:47:34Z
dc.date.accessioned2018-11-06T14:32:32Z
dc.date.available2017-09-13T17:47:34Z
dc.date.available2018-11-06T14:32:32Z
dc.date.created2017-09-13T17:47:34Z
dc.date.issued2017-05-19
dc.identifierScheffler, Guillermo Federico; Pulido, Manuel Arturo; Estimation of gravity wave parameters to alleviate the delay in the Antarctic vortex breakup in general circulation models; John Wiley & Sons Ltd; Quarterly Journal of the Royal Meteorological Society; 143; 706; 19-5-2017; 2157-2167
dc.identifier0035-9009
dc.identifierhttp://hdl.handle.net/11336/24158
dc.identifier1477-870X
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1887505
dc.description.abstractThe impact of optimal parameters in a non-orographic gravity wave drag parameterization on the middle atmosphere circulation of the Southern hemisphere is examined. Optimal parameters are estimated using a data assimilation technique.  The proposed technique aims to reduce the delay in the winter vortex breakdown of the Southern Hemisphere found in general circulation models, which may be associated with a poor representation of gravity wave activity.  We introduce two different implementations of the parameter estimation method: an emph{offline} estimation method and a emph{sequential} estimation method. The delay in the zonal-mean zonal-wind transition  is largely alleviated by the optimal gravity wave parameters. The sequential method diminishes the model biases during winter vortex evolution, through gravity wave drag alone. On the other hand, the offline method accounts better for the unresolved-resolved wave interactions and the zonal-wind transition. We show that the final warmings in the lower mesosphere are mainly driven by planetary wave breaking. These are affected by changes in the gravity wave drag which are responsible for the stratospheric preconditioning. Parameter estimation during the vortex breakdown is a challenging task that requires the use of sophisticated estimation techniques, because there are strong interactions  between unresolved gravity wave drag and planetary waves.
dc.languageeng
dc.publisherJohn Wiley & Sons Ltd
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1002/qj.3074/abstract
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1002/qj.3074
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rights2018-02-01
dc.rightsinfo:eu-repo/semantics/embargoedAccess
dc.subjectGRAVITY WAVE PARAMETERIZATIONS
dc.subjectPARAMETER ESTIMATION
dc.subjectMODEL BIAS
dc.subjectFINAL STRATOSPHERIC WARMING
dc.titleEstimation of gravity wave parameters to alleviate the delay in the Antarctic vortex breakup in general circulation models
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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