The SAO and Kelvin waves in the EuroGRIPS GCMS and the UK Met. Office analyses

被引:11
作者
Amodei, M [1 ]
Pawson, S
Scaife, AA
Langematz, U
Lahoz, W
Li, DM
Simon, P
机构
[1] Meteo France, CNRM, Toulouse, France
[2] NASA, Goddard Space Flight Ctr, Data Assimilat Off, Greenbelt, MD 20771 USA
[3] Univ Space Res Assoc, Seabrook, MD USA
[4] Meteorol Off, Bracknell RB12 2SZ, Berks, England
[5] Free Univ Berlin, D-1000 Berlin, Germany
[6] Univ Reading, Ctr Global Atmospher Modelling, Reading RG6 2AH, Berks, England
关键词
meteorology and atmospheric dynamics (middle; atmosphere dynamics; tropical meterology; waves and tides);
D O I
10.5194/angeo-19-99-2001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We compare the tropical oscillations and planetary scale Kelvin waves in four troposphere-stratosphere climate models and the assimilated dataset produced by the United Kingdom Meteorological Office (UKMO). The comparison has been made in the GRIPS framework "GCM-Reality Intercomparison Project for SPARC", where SPARC is Stratospheric Processes and their Role in Climate, a project of the World Climate Research Program. The four models evaluated are European members of GRIPS: the UKMO Unified Model (UM), the model of the Free University in Berlin (FUB-GCM), the ARPEGE-climat model of the French National Centre for Meteorological Research (CNRM), and the Extended UGAMP GCM (EUGCM) of the Centre for Global Atmospheric Modelling (CGAM). The integrations were performed with different, but annually periodic external conditions (e.g., sea-surface temperature, sea ice, and incoming solar radiation). The structure of the tropical winds and the strengths of the Kelvin waves are examined. In the analyses where the SAO (Semi-Annual Oscillation) and the QBO (Quasi-Biennal Oscillation) are reasonably well captured, the amplitude of these analysed Kelvin waves is close to that observed in independent data from UARS (Upper Atmosphere Research Satellite). In agreement with observations, the Kelvin waves generated in the models propagate into the middle atmosphere as wave packets, consistent with a convective forcing origin. In three of the models, slow Kelvin waves propagate too high and their amplitudes are overestimated in the upper stratosphere and in the mesosphere, the exception is the UM which has weaker waves. None of the modelled waves are sufficient to force realistic eastward phases of the QBO or SAG. Although the SAO is represented by all models, only two of them are able to generate westerlies between 10 hPa and 50 hPa. The importance of the role played in the SAO by unresolved gravity waves is emphasized. Although it exhibits some unrealistic features, the EUGCM, which includes a parametrization of gravity waves with a non-zero phase speed, is able to simulate clear easterly to westerly transitions as well as westerlies with downward propagation. Thermal damping is also important for the westerly forcing in the stratosphere.
引用
收藏
页码:99 / 114
页数:16
相关论文
共 81 条
[1]  
BERGMAN JW, 1994, J ATMOS SCI, V51, P3791, DOI 10.1175/1520-0469(1994)051<3791:EWADFF>2.0.CO
[2]  
2
[3]  
Betts AK, 1993, REPRESENTATION CUMUL
[4]  
Bossuet C, 1998, ANN GEOPHYS-ATM HYDR, V16, P238, DOI 10.1007/s00585-998-0238-z
[5]  
BOUGEAULT P, 1985, MON WEATHER REV, V113, P2108, DOI 10.1175/1520-0493(1985)113<2108:ASPOTL>2.0.CO
[6]  
2
[7]  
Butchart N, 1998, J ATMOS SCI, V55, P2782, DOI 10.1175/1520-0469(1998)055<2782:MACFTT>2.0.CO
[8]  
2
[9]  
CANZIANI PO, 1994, J ATMOS SCI, V51, P3053, DOI 10.1175/1520-0469(1994)051<3053:EKWAUM>2.0.CO
[10]  
2