Parameterized Gravity Wave Momentum Fluxes from Sources Related to Convection and Large-Scale Precipitation Processes in a Global Atmosphere Model

被引:45
|
作者
Bushell, Andrew C. [1 ]
Butchart, Neal [2 ]
Derbyshire, Stephen H. [1 ]
Jackson, David R. [1 ]
Shutts, Glenn J. [1 ]
Vosper, Simon B. [1 ]
Webster, Stuart [1 ]
机构
[1] Met Off, Exeter EX1 3PB, Devon, England
[2] Met Off Hadley Ctr, Exeter, Devon, England
基金
英国自然环境研究理事会; 欧盟第七框架计划;
关键词
Circulation; Dynamics; Gravity waves; Quasibiennial oscillation; Models and modeling; General circulation models; Model evaluation; performance; Parameterization; Subgrid-scale processes; QUASI-BIENNIAL OSCILLATION; OFFICE UNIFIED MODEL; GENERAL-CIRCULATION MODELS; MIDDLE ATMOSPHERE; CLIMATE MODELS; NUMERICAL-MODEL; STRATOSPHERE; DRAG; FRONTOGENESIS; DISTRIBUTIONS;
D O I
10.1175/JAS-D-15-0022.1
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
Analysis of a high-resolution, convection-permitting simulation of the tropical Indian Ocean has revealed empirical relationships between precipitation and gravity wave vertical momentum flux on grid scales typical of earth system models. Hence, the authors take a rough functional form, whereby the wave flux source spectrum has an amplitude proportional to the square root of total precipitation, to represent gravity wave source strengths in the Met Office global model's spectral nonorographic scheme. Key advantages of the new source are simplicity and responsiveness to changes in convection processes without dependence upon model-specific details of their representation. Thus, the new source scheme is potentially a straightforward adaptation for a class of spectral gravity wave schemes widely used for current state-of-the-art earth system models. Against an invariant source, the new parameterized source generates launch-level flux amplitudes with greater spatial and temporal variability, producing probability density functions for absolute momentum flux over the ocean that have extended tails of large-amplitude, low-occurrence events. Such distributions appear more realistic in comparison with reported balloon observations. Source intermittency at the launch level affects mean fluxes at higher levels in two ways: directly, as a result of upward propagation of the new source variation, and indirectly, through changes in filtering characteristics that arise from intermittency. Initial assessment of the new scheme in the Met Office global model indicates an improved representation of the quasi-biennial oscillation and sensitivity that offers potential for further impact in the future.
引用
收藏
页码:4349 / 4371
页数:23
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