日本地球惑星科学連合2022年大会

講演情報

[E] 口頭発表

セッション記号 A (大気水圏科学) » A-CG 大気海洋・環境科学複合領域・一般

[A-CG35] 熱帯におけるマルチスケール大気海洋相互作用

2022年5月25日(水) 13:45 〜 15:15 201A (幕張メッセ国際会議場)

コンビーナ:東塚 知己(東京大学大学院理学系研究科地球惑星科学専攻)、コンビーナ:Richter Ingo(JAMSTEC Japan Agency for Marine-Earth Science and Technology)、今田 由紀子(気象庁気象研究所)、コンビーナ:大庭 雅道(電力中央研究所)、座長:東塚 知己(東京大学大学院理学系研究科地球惑星科学専攻)、大庭 雅道(電力中央研究所)

14:45 〜 15:00

[ACG35-05] New emergence of the Southern Indian Ocean Dipole as a trigger for Central Pacific El Niño since the 2000s

*Hyun-Su Jo1 (1.Chonnam National University)

キーワード:Southern Indian Ocean Dipole (SIOD), ENSO, Interbasin interaction

Despite decades of effort, predicting the El Niño-Southern Oscillation (ENSO) since the 2000s has become increasingly challenging(Barnston et al., 2012). This is partly caused by a weakened coupling between the ENSO and well-known precursors in tropical ocean basins(Li et al., 2020), particularly in the Indian Ocean(Han and Wang, 2021). Here we show that the Southern Indian Ocean Dipole (SIOD), which is characterized by east-west oriented sea surface temperature (SST) dipole pattern over the southern Indian Ocean, becomes a key precursor of the Central Pacific El Niño events since the 2000s at a 14-month lead. Interestingly, the previously revealed precursors accelerate the transition of ENSO phase(Izumo et al., 2010; Ham et al., 2013), while the SIOD prolongs the ENSO period. Anomalous westerlies over the equatorial western Pacific led by the positive SIOD result in the development of a Central Pacific El Niño event in the subsequent year. The SIOD after the 2000s persists longer due to the westward shifted ENSO events, which eventually intensifies the impact of the SIOD on the subsequent ENSO evolution.