Response of the tropical Indian Ocean SST to decay phase of La Nina and associated processes

被引:5
|
作者
Bhavani, T. S. D. [1 ,2 ]
Chowdary, J. S. [1 ]
Bharathi, G. [2 ]
Srinivas, G. [1 ,2 ]
Prasad, K. V. S. R. [2 ]
Deshpande, Aditi [3 ]
Parekh, Anant [1 ]
Gnanaseelan, C. [1 ]
机构
[1] IITM, Pune 411008, Maharashtra, India
[2] Andhra Univ, Dept Meteorol & Oceanog, Visakhapatnam 530003, Andhra Pradesh, India
[3] Savitribai Phule Pune Univ, Dept Atmospher & Space Sci, Pune 411007, Maharashtra, India
关键词
La Nina; Tropical Indian Ocean; Upwelling Rossby wave; Sea surface temperature; Heat flux; Arabian Sea; SEA-SURFACE TEMPERATURE; INDO-WESTERN PACIFIC; EL-NINO; INTERANNUAL VARIABILITY; ENSO TELECONNECTION; MIXED-LAYER; PART I; CIRCULATION; PERSISTENCE; IMPACTS;
D O I
10.1016/j.dynatmoce.2017.10.005
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
Delayed impact of El Nifio on Tropical Indian Ocean (TIO) Sea Surface Temperature (SST) variations and associated physical mechanisms are well documented by several studies. However, TIO SST evolution during the decay phase of La Nina and related processes are not adequately addressed before. Strong cooling associated with La Nina decay over the TIO could influence climate over the Indian Oceanic rim including Indian summer monsoon circulation and remotely northwest Pacific circulation. Thus understanding the TIO basin-wide cooling and related physical mechanisms during decaying La Nifia years is important. Composite analyses revealed that negative SST anomalies allied to La Nina gradually dissipate from its mature phase (winter) till subsequent summer in central and eastern Pacific. In contrast, magnitude of negative SST anomalies in TIO, induced by La Nifia, starts increasing from winter and attains their peak values in early summer. It is found that variations in heat flux play an-important role in SST cooling over the central and eastern equatorial Indian Ocean, Bay of Bengal and part of Arabian Sea from late winter to early summer during the decay phase of La Nifia. Ocean dynamical processes are mainly responsible for the evolution of southern TIO SST cooling. Strong signals of westward propagating upwelling Rossby waves between 10 degrees S to 20 degrees S are noted throughout (the decaying phase of La Nifia) spring and summer. Anomalous cyclonic wind stress curl to the south of the equator is responsible for triggering upwelling Rossby waves over the southeastern TIO. Further, upwelling Rossby waves are also apparent in the Arabian Sea from spring to summer and partly contributing to the SST cooling. Heat budget analysis reveals that negative SST/MLT (mixed layer temperature) anomalies over the Arabian Sea are mostly controlled by heat flux from winter to spring and vertical advection plays an important role during early summer. Vertical and horizontal advection terms primarily contribute to the SST cooling anomalies over southern TIO and the Bay of Bengal cooling is primarily dominated by heat flux. Further we have discussed influence of TIO cooling on local rainfall variations. (C) 2017 Elsevier B.V. All rights reserved.
引用
收藏
页码:110 / 123
页数:14
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