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Surface and Subsurface Oceanic Variability Observed in the Eastern Equatorial Indian Ocean During Three Consecutive Indian Ocean Dipole Events: 2006-2008

机译:在三个连续的印度洋偶极子事件:2006-2008年期间,在赤道东印度洋观测到的地表和地下海洋变化

摘要

8-year and 4-year long velocity time series records from the equatorial Indian Ocean successfully captured, for the first time, complete evolution of subsurface currents associated with three consecutive Indian Ocean Dipole (IOD) events in 2006 –2008. It is found that strong eastward subsurface zonal currents in the layer between about 90 m and 150 m were observed, which were opposite to the normal conditions. Vertical structure of the zonal currents resembles that of the typical zonal currents in the equatorial Pacific with an eastward subsurface current lies beneath the surface westward currents. This vertical structure of the zonal currents was associated with anomalous easterly winds along the equatorial Indian Ocean during the maturing phase of the IOD events. In addition, subsurface temperature structures obtained from RAMA buoy network show negative temperature anomalies preceded the surface temperature evolution associated with the IOD events. The negative subsurface temperature anomaly lasted for several months before it changes into positive anomaly as the IOD terminated. The surface temperature structure indicated by the Dipole Mode Index (DMI) revealed that the 2006 IOD was a strong event, while the 2007 and 2008 events were weaker and short-lived events. The evolution of the IOD events were linked to the dynamics of oceanic equatorial wave. It is found that upwelling equatorial Kelvin waves forced by anomalous easterly wind stress play an important role in generating cooling tendency during the development and maturing phase of the IOD events. The demise of the IOD events, on the other hand, was linked to eastern-boundary-reflected Rossby waves that terminated the cooling tendency in the eastern Indian Ocean induced by the wind-forced Kelvin waves. Weakening of the zonal heat advection, then, provided a favor condition for the surface heat flux to warm the sea surface temperature in the eastern equatorial Indian Ocean.
机译:来自赤道印度洋的8年和4年长速度时间序列记录首次成功地捕获了与2006年至2008年连续3次印度洋偶极子(IOD)事件相关的地下洋流的完整演化。结果发现,在该层约90 m至150 m之间观测到强东向地下纬向气流,这与正常情况相反。地带流的垂直结构类似于赤道太平洋中典型的地带流,东向地下电流位于地表西向流下方。在IOD事件成熟阶段,纬向气流的这种垂直结构与沿赤道印度洋的异常东风有关。此外,从RAMA浮标网络获得的地下温度结构在与IOD事件相关的表面温度演变之前显示出负温度异常。负地下温度异常持续了几个月,之后随着IOD终止变为正异常。偶极模式指数(DMI)表示的表面温度结构表明,2006年的IOD是强事件,而2007年和2008年的事件是弱事件和短暂事件。 IOD事件的演变与海洋赤道波的动力学有关。发现在异常IOD事件的发展和成熟阶段,由异常东风引起的上升赤道开尔文波在产生冷却趋势中起重要作用。另一方面,IOD事件的消退与东部边界反射的罗斯比海浪有关,后者终止了由风力开尔文波引起的印度洋东部的降温趋势。然后,纬向平流的减弱为赤道东印度洋海表热通量加热海面温度提供了有利条件。

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