Simulation of SST fluctuations and circulation in the Equatorial Indian Ocean

被引:0
|
作者
Ganer, D. W. [1 ]
Deo, A. A. [1 ]
Salvekar, P. S. [2 ]
机构
[1] Indian Inst Trop Meteorol, Dr Homi Bhabha Rd, Pune 411008, Maharashtra, India
[2] Indian Inst Trop Meteorol, Theoret Studies Div, Pune 411008, Maharashtra, India
来源
JOURNAL OF INDIAN GEOPHYSICAL UNION | 2006年 / 10卷 / 03期
关键词
D O I
暂无
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Inter-annual variability in the equatorial Indian Ocean sometimes exhibits large Sea Surface Temperature (SST) fluctuations. The SST anomaly gradient between eastern and western equatorial Indian Ocean during summer season (June-October) becomes greater than 1(circle)C. This east-west SST anomaly gradient is independent of ENSO and may be a natural oscillation of the Indian Ocean. Such fluctuations are observed in many years during the decade 1990-2000. In the present study a 2(circle)layer thermodynamic ocean model has been used to simulate inter-annual variability in the circulation and SST anomaly (SSTA) fluctuations in the Indian Ocean. The model simulated SST over the Tropical Indian Ocean is in close agreement with observed SST. The warm SSTA in the western equatorial Indian Ocean and cold SSTA in the eastern equatorial Indian Ocean during the years 1994 and 1997 and, opposite SSTA during the years 1992 and 1996, are well simulated by the model.
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页码:209 / 218
页数:10
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