Estimation of gravity-wave parameters to alleviate the delay in the Antarctic vortex breakup in general circulation models

被引:9
|
作者
Scheffler, Guillermo [1 ]
Pulido, Manuel [2 ,3 ]
机构
[1] Univ Nacl Nordeste, Dept Math, FACENA, Corrientes, Argentina
[2] Univ Nacl Nordeste, Dept Phys, FACENA, Ave Libertad 5400, RA-3400 Corrientes, Argentina
[3] Consejo Nacl Invest Cient & Tecn, Corrientes, Argentina
关键词
gravity-wave parametrizations; parameter estimation; model bias; final stratospheric warming; DATA ASSIMILATION PRINCIPLES; MIDDLE ATMOSPHERE; PLANETARY-WAVES; DRAG ESTIMATION; CLIMATE MODELS; COMPENSATION;
D O I
10.1002/qj.3074
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
The impact of optimal parameters in a non-orographic gravity-wave drag parametrization 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 offline estimation method and a 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 unresolved-resolved wave interactions and the zonal-wind transition. We show that the final warmings in the lower mesosphere are driven mainly by planetary-wave breaking. These are affected by changes in the gravity-wave drag that are responsible for 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.
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页码:2157 / 2167
页数:11
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