Ningaloo Nio simulated in the CMIP5 models

被引:20
|
作者
Kido, Shoichiro [1 ]
Kataoka, Takahito [2 ]
Tozuka, Tomoki [1 ]
机构
[1] Univ Tokyo, Grad Sch Sci, Dept Earth & Planetary Sci, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
[2] Univ Tokyo, Atmosphere & Ocean Res Inst, Kashiwa, Chiba, Japan
关键词
INDIAN-OCEAN DIPOLE; EL-NINO; VARIABILITY; REANALYSIS; FREQUENCY; EVENTS; REMOTE; ENSO;
D O I
10.1007/s00382-015-2913-6
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
The ability of coupled general circulation models (CGCMs) to simulate a newly-discovered climate mode called Ningaloo Nio/Nia is examined using outputs from 17 CGCMs that participated in the Coupled Model Inter-comparison Project, phase 5. It is shown that 8 out of 17 models reproduce sea surface temperature (SST) anomalies associated with Ningaloo Nio/Nia with a pattern correlation coefficient of 0.7 or higher, but the location of peak SST anomalies is very different from the observation in 2 models. Also, fundamental features such as the seasonality and associated anomalous atmospheric circulation and precipitation are fairly well reproduced in most models, but the amplitude varies significantly among the models. The inter-model difference in the amplitude is found to be mainly due to that in the magnitude of remote influences from the El Nio-Southern Oscillation via oceanic and atmospheric teleconnections. On the other hand, the strength of local air-sea interaction does not contribute much to the inter-model difference. This study may pave the way for an improved representation of Ningaloo Nio/Nia in CGCMs.
引用
收藏
页码:1469 / 1484
页数:16
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