On the spring stratospheric final warming in CMIP5 and CMIP6 models

被引:5
|
作者
Hu, Jinggao [1 ]
Liu, Zexuan [1 ]
Xu, Haiming [1 ]
Ren, Rongcai [1 ,2 ]
Jin, Dachao [1 ]
机构
[1] Nanjing Univ Informat Sci & Technol, Joint Int Res Lab Climate & Environm Change ILCEC, Collaborat Innovat Ctr Forecast & Evaluat Meteoro, Key Lab Meteorol Disaster,Minist Educ KLME, Nanjing 210044, Peoples R China
[2] Chinese Acad Sci, Inst Atmospher Phys, State Key Lab Numer Modeling Atmospher Sci & Geop, Beijing 100029, Peoples R China
基金
中国国家自然科学基金;
关键词
Stratospheric final warming events; CMIP5 and CMIP6 models; Historical simulation; Southern and Northern Hemispheres; POLAR VORTEX; HIGH-TOP; VARIABILITY; EVENTS; CIRCULATION; PRECURSOR;
D O I
10.1007/s11430-021-9971-y
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
This study evaluates the performance in simulating the stratospheric final warming events (SFWs) that lead to the final collapse of the stratospheric polar vortex in spring in both Southern and Northern Hemispheres (SH and NH, respectively) based on the historical simulations provided by the Coupled Model Intercomparison Project Phases 5 and 6 (CMIP5 and CMIP6, respectively). Overall, CMIP5 and CMIP6 models can reproduce the main characteristics of the occurrence of SFWs. However, the SFW onset date (SFWOD) is 7 and 9 days later than in observations in the SH and NH, respectively. Moreover, the intensity of SFWs in models is 50% to 70% of that in observations. Compared with CMIP5 models, CMIP6 models have an ameliorated capability to simulate NH SFWs. However, this improvement does not manifest as significantly earlier SFW onset, but as more intense stratospheric planetary wave activities before the SFW and as a larger interannual variability of the SFWOD. By contrast, in the SH, the capability of CMIP6 models is roughly unchanged, even deteriorated in the simulation of SFWOD and stratospheric planetary wave activities before the SFW onset. The performance of CMIP6 high-top models is better than that of low-top models. Specifically, in the NH, high-top models are considerably improved in terms of intensity of circumpolar zonal wind around the SFWOD and stratospheric planetary wave activities before the SFW onset. In the SH, high-top models show fairly earlier SFWOD by 11 days, which is closer to observations.
引用
收藏
页码:129 / 145
页数:17
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