Three Types of Positive Indian Ocean Dipoles and Their Relationships with the South Asian Summer Monsoon

• Published in: Journal of climate Vol. 35; no. 1; pp. 405 - 424
• Main Authors: Jiang, Jilan, Liu, Yimin, Mao, Jiangyu, Li, Jianping, Zhao, Shuwen, Yu, Yongqiang
• Format: Journal Article
• Language: English
• Published: Boston American Meteorological Society 01.01.2022
• Subjects: Amplitudes; Anomalies; Autumn; Cold; Cooling; Data analysis; Data assimilation; Datasets; Dipoles; El Nino; Mathematical models; Monsoons; Numerical experiments; Numerical simulations; Oceanic analysis; Oceans; Poles; Precipitation; Sea surface; Sea surface temperature; Sea surface temperature anomalies; Summer; Summer monsoon; Surface temperature; Temperature anomalies; Time series; Tropical climate; Wind; Indian Ocean
• ISSN: 0894-8755; 1520-0442
• DOI: 10.1175/JCLI-D-21-0089.1

Abstract The relationship between the Indian Ocean dipole (IOD) and the South Asian summer monsoon (SASM), which remains a subject of controversy, was investigated using data analyses and numerical experiments. We categorized IOD events according to their sea surface temperature anomaly (SSTA) pattern: type W and type E are associated with stronger SSTA amplitudes in the western and eastern poles of the IOD, respectively, while type C has comparable SSTA amplitudes in both poles during boreal autumn. Type W is associated with a weak SASM from May to summer, which contributes to substantial warming of the western pole in autumn; the east–west SST gradient linked to the warming of the western pole causes weak southeasterly wind anomalies off Sumatra and feeble and cold SSTAs in the eastern pole during the mature phase. Type E is associated with a strong SASM and feeble warming of the western pole; interaction between the strong SASM and cold SSTAs in the eastern pole in summer results in strong southeasterly wind anomalies off Sumatra and substantial cooling of the eastern pole during the mature phase. For type C, warming of the western pole and cooling of the eastern pole develop synchronously without apparent SASM anomalies and reach comparable intensities during the mature phase. Observations and numerical simulation results both indicate the role of disparate SASM anomalies in modulating SSTA patterns during the development of positive IODs. Warming of the tropical Indian Ocean becomes established in the winter and spring following type W and type C IODs but not following type E events.