Consistent approximate models of the global atmosphere: shallow, deep, hydrostatic, quasi-hydrostatic and non-hydrostatic

被引:108
作者
White, AA
Hoskins, BJ
Roulstone, I
Staniforth, A
机构
[1] Met Off, Exeter EX1 3PB, Devon, England
[2] Univ Reading, Dept Meteorol, Reading, Berks, England
[3] Univ Surrey, Dept Math & Stat, Surrey, England
关键词
apparent gravity; conservation properties; Coriolis force; Lagrange's equations; primitive equations;
D O I
10.1256/qj.04.49
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
We study global atmosphere models that are at least as accurate as the hydrostatic primitive equations (HPEs), reviewing known results and reporting some new ones. The HPEs make spherical geopotential and shallow atmosphere approximations in addition to the hydrostatic approximation. As is well known, a consistent application of the shallow atmosphere approximation requires omission of those Coriolis terms that vary as the cosine of latitude and of certain other terms in the components of the momentum equation. An approximate model is here regarded as consistent if it formally preserves conservation principles for axial angular momentum, energy and potential vorticity, and (following R. Muller) if its momentum component equations have Lagrange's form. Within these criteria, four consistent approximate global models, including the HPEs themselves, are identified in a height-coordinate framework. The four models, each of which includes the spherical geopotential approximation, cor-respond to whether the shallow atmosphere and hydrostatic (or quasi-hydrostatic) approximations are individually made or not made. Restrictions on representing the spatial variation of apparent gravity occur. Solution methods and the situation in a pressure-coordinate framework are discussed.
引用
收藏
页码:2081 / 2107
页数:27
相关论文
共 59 条
[1]  
[Anonymous], ENCY ATMOSPHERIC SCI
[2]   ATMOSPHERIC ANGULAR-MOMENTUM FLUCTUATIONS, LENGTH-OF-DAY CHANGES AND POLAR MOTION [J].
BARNES, RTH ;
HIDE, R ;
WHITE, AA ;
WILSON, CA .
PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, 1983, 387 (1792) :31-73
[3]  
Batchelor David., 2000, An Introduction to Fluid Dynamics
[4]  
BRETHERTON FP, 1964, TELLUS, V16, P181
[5]  
CULLEN MJP, 1993, METEOROL MAG, V122, P81
[6]  
Daley R., 1988, Tellus, Series A (Dynamic Meteorology and Oceanography), V40A, P96, DOI 10.1111/j.1600-0870.1988.tb00409.x
[7]   A new dynamical core for the Met Office's global and regional modelling of the atmosphere [J].
Davies, T ;
Cullen, MJP ;
Malcolm, AJ ;
Mawson, MH ;
Staniforth, A ;
White, AA ;
Wood, N .
QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY, 2005, 131 (608) :1759-1782
[8]   FLOWS IN A ROTATING SPHERICAL-SHELL - THE EQUATORIAL CASE [J].
DEVERDIERE, AC ;
SCHOPP, R .
JOURNAL OF FLUID MECHANICS, 1994, 276 :233-260
[9]  
DRAGHICI I, 1989, SOV METEOROL HYDROL, V19, P13
[10]  
Durran DR, 2004, J ATMOS SCI, V61, P1982, DOI 10.1175/1520-0469(2004)061<1982:COTROT>2.0.CO