Potential impact of the tropical Indian Ocean-Indonesian seas on El Niño characteristics

H. Annamalai, Shinichiro Kida, Jan Hafner

Research output: Contribution to journalArticle

30 Citations (Scopus)

Abstract

Diagnostics performed with twentieth-century (1861-2000) ensemble integrations of the Geophysical Fluid Dynamics Laboratory Climate Model, version 2.1 (CM2.1) suggest that, during the developing phase, El Niño events that co-occur with the Indian Ocean Dipole Zonal Mode (IODZM; class 1) are stronger than those without (class 2). Also, during class 1 events coherent sea surface temperature (SST) anomalies develop in the Indonesian seas that closely follow the life cycle of IODZM. This study investigates the effect of these regional SST anomalies (equatorial Indian Ocean and Indonesian seas) on the amplitude of the developing El Niño. An examination of class 1 minus class 2 composites suggests two conditions that could lead to a strong El Niño in class 1 events: (i) during January, ocean-atmosphere conditions internal to the equatorial Pacific are favorable for the development of a stronger El Niño and (ii) during May-June, coinciding with the development of regional SST anomalies, an abrupt increase in westerly wind anomalies is noticeable over the equatorial western Pacific with a subsequent increase in thermocline and SST anomalies over the eastern equatorial Pacific. This paper posits the hypothesis that, under favorable conditions in the equatorial Pacific, regional SST anomalies may enable the development of a stronger El Niño. Owing to a wealth of feedbacks in CM2.1, solutions from a linear atmosphere model forced with May-June anomalous precipitation and anomalous SST from selected areas over the equatorial Indo-Pacific are examined. Consistent with our earlier study, the net Kelvin wave response to contrasting tropical Indian Ocean heating anomalies cancels over the equatorial western Pacific. In contrast, Indonesian seas SST anomalies account for about 60%-80% of the westerly wind anomalies over the equatorial western Pacific and also induce anomalous precipitation over the equatorial central Pacific. It is argued that the feedback between the precipitation and circulation anomalies results in an abrupt increase in zonal wind anomalies over the equatorial western Pacific. Encouraged by these results, the authors further examined the processes that cause cold SST anomalies over the Indonesian seas using an ocean model. Sensitivity experiments suggest that local wind anomalies, through stronger surface heat loss and evaporation, and subsurface upwelling are the primary causes. The present results imply that in coupled models, a proper representation of regional air-sea interactions over the equatorial Indo-Pacific warm pool may be important to understand and predict the amplitude of El Niño.

Original languageEnglish
Pages (from-to)3933-3952
Number of pages20
JournalJournal of Climate
Volume23
Issue number14
DOIs
Publication statusPublished - Jul 1 2010
Externally publishedYes

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temperature anomaly
sea surface temperature
anomaly
westerly
climate modeling
air-sea interaction
warm pool
Kelvin wave
sea
Indian Ocean
atmosphere
fluid dynamics
ocean
zonal wind
thermocline
twentieth century
upwelling
life cycle
evaporation
heating

All Science Journal Classification (ASJC) codes

  • Atmospheric Science

Cite this

Potential impact of the tropical Indian Ocean-Indonesian seas on El Niño characteristics. / Annamalai, H.; Kida, Shinichiro; Hafner, Jan.

In: Journal of Climate, Vol. 23, No. 14, 01.07.2010, p. 3933-3952.

Research output: Contribution to journalArticle

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