印度洋偶极子
温跃层
副热带印度洋偶极子
气候学
海洋热含量
海面温度
罗斯比波
构造盆地
地质学
海洋环流模式
海洋动力学
海洋学
强迫(数学)
赤道波
洋流
气候变化
大气环流模式
赤道
纬度
古生物学
大地测量学
作者
Jing Wang,Shouwen Zhang,Hua Jiang,Dongliang Yuan
出处
期刊:Journal of Climate
[American Meteorological Society]
日期:2024-01-01
卷期号:37 (1): 145-163
标识
DOI:10.1175/jcli-d-22-0741.1
摘要
Abstract The Indian Ocean basin (IOB) mode is the dominant mode of the interannual sea surface temperature (SST) variability in the Indian Ocean, with the Indian Ocean dipole (IOD) as the second mode. An IOB event normally occurs after an El Niño or a concurrent IOD–El Niño event, the dynamics of which are traditionally believed as forced by ENSO through the Walker circulation anomalies over the tropical Indian Ocean. A strong IOB in 2020 took place after the strongest 2019 IOD on record but independent of El Niño, which challenges the traditional atmospheric bridge dynamics of the IOB event. In this study, the dynamics of the 2020 IOB event are investigated using the numerical seasonal climate prediction system of the National Marine Environmental Forecasting Center of China. It is found that the initialization of the Indian Ocean subsurface temperature during the 2019 IOD event has led to the outburst of the 2020 IOB event successfully, the dynamics of which are the propagation and the western boundary reflection of the equatorial and off-equatorial Rossby waves, inducing heat content recharge over the tropical Indian Ocean upper thermocline. In comparison, experiments of SST initialization over the tropical Indian Ocean, with the subsurface temperature in a climatological state, were unable to reproduce the onset of the 2020 IOB event, suggesting that the local air–sea interaction within the Indian Ocean basin is of secondary importance. The numerical experiments suggest that the thermocline ocean wave dynamics play an important role in forcing the IOB event. The revealed thermocline dynamics are potentially useful in climate prediction associated with IOB events.
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