日本地球惑星科学連合2019年大会

講演情報

[J] ポスター発表

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-CG38] 熱帯インド洋・太平洋におけるマルチスケール大気海洋相互作用

2019年5月28日(火) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 8ホール)

コンビーナ:清木 亜矢子(海洋研究開発機構)、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)、名倉 元樹((独) 海洋研究開発機構)、釜江 陽一(筑波大学生命環境系)

[ACG38-P06] 熱帯太平洋からの海洋波動の伝播がニンガルー・ニーニョ現象の非対称性に与える影響について

*楠 秀大1木戸 晶一郎1東塚 知己1 (1.東京大学大学院理学系研究科地球惑星科学専攻)

キーワード:ニンガルー・ニーニョ現象、領域海洋モデル、エルニーニョ・南方振動、沿岸ケルビン波

Ningaloo Nino (Nina) is a climate mode associated with anomalously warm (cool) sea surface temperature (SST) off the Western Australian coast. Considering its large impacts on the local marine ecosystem and precipitation, better understanding of its mechanism and predictability is desirable. Existing studies suggest that both local air-sea interaction and remote forcing contribute to generation and amplification of the Ningaloo Nino/Nina. The latter forcing includes the atmospheric teleconnection and oceanic wave propagation through the Indonesian archipelago, mainly associated with the El Nino/Southern Oscillation (ENSO). One of the important characteristics of Ningaloo Nino/Nina is its asymmetry; the Ningaloo Nino is stronger than the Ningaloo Nina. This suggests the presence of some asymmetry in these processes. However, no studies to date focused on this topic.

Using a regional ocean modeling system (ROMS), the contribution of oceanic wave propagation to the amplitude and asymmetry of SST anomalies associated with the Ningaloo Nino/Nina is investigated. For these purposes, a sensitivity experiment in which oceanic lateral boundary conditions are replaced by the monthly climatology is conducted. The results suggest that downwelling (upwelling) Kelvin waves from the western tropical Pacific associated with La Nina (El Nino) that often co-occur with Ningaloo Nino (Nina) are stronger (weaker) and contribute to the asymmetry.