Dynamic model of mesoscale eddies. Eddy parameterization for coarse resolution ocean circulation models

被引:6
|
作者
Dubovikov, MS
Canuto, VM
机构
[1] NASA, Goddard Inst Space Studies, New York, NY 10025 USA
[2] Columbia Univ, Ctr Climate Syst Res, New York, NY 10025 USA
[3] Columbia Univ, Dept Appl Phys & Math, New York, NY 10027 USA
来源
基金
美国国家航空航天局;
关键词
density and momentum large scale equations; isopycnal and level coordinates; bolus and eddy-induced velocity; residual density flux; Reynolds stress; vorticity flux;
D O I
10.1080/03091920412331336406
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the framework of the eddy dynamic model developed in two previous papers (Dubovikov, M.S., Dynamical model of mesoscale eddies, Geophys. Astophys. Fluid Dyn., 2003, 97, 311-358; Canuto, V.M. and Dubovikov, M.S., Modeling mesoscale eddies, Ocean Modelling, 2004, 8, 1-30 reterred as I-II), we compute the contribution of unresolved mesoscale eddies to the large-scale dynamic equations of the ocean. In isopycnal coordinates, in addition to the bolus velocity discussed in I-II, the mesoscale contribution to the large scale momentum equation is derived. Its form is quite different from the traditional down-gradient parameterization. The model solutions in isopycnal coordinates are transformed to level coordinates to parameterize the eddy contributions to the corresponding large scale density and momentum equations. In the former, the contributions due to the eddy induced velocity and to the residual density flux across mean isopycnals (so called Sigma-term) are derived, both contributions being shown to be of the same order. As for the large scale momentum equation, as well as in isopycnal coordinates, the eddy contribution has a form which is quite different from the down-gradient expression.
引用
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页码:19 / 47
页数:29
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