日本地球惑星科学連合2018年大会

講演情報

[EJ] ポスター発表

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

[A-CG39] 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

2018年5月21日(月) 15:30 〜 17:00 ポスター会場 (幕張メッセ国際展示場 7ホール)

コンビーナ:今田 由紀子(気象庁気象研究所)、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)、時長 宏樹(京都大学防災研究所、共同)、小坂 優(東京大学先端科学技術研究センター)

[ACG39-P03] Effects of the Australian monsoon on the duration of La Niña longer than that of El Niño

*白井 大雅1冨田 智彦2 (1.熊本大学大学院 自然科学研究科、2.熊本大学大学院 先端科学研究部)

キーワード:La Niñaの持続、オーストラリアモンスーン

In general, La Niña has longer duration than El Niño. That is, La Niña tends to remain for one year or longer, while El Niño decays within a year. The Australian monsoon plays an essential role for this long duration of La Niña. In spring after the mature phase of La Niña, the precipitation anomaly around the Indonesian maritime continent (IMC) is positive with the upward branch of Walker circulation. The positive precipitation anomalies further remain due to the temperature difference between IMC and northern Australia (NA). When La Niña occurs, the sea surface temperature (SST) is barely high around IMC, while land cooling is strong over NA due to the positive precipitation anomalies there, both of which make the large temperature difference between IMC and NA (IMC > NA). From boreal spring to summer, i.e., from austral fall to winter, the temperature of NA seasonally decreases. Such seasonal and anomalous temperature decreases over NA give rise to the substantial large-scale land breeze from NA to IMC, i.e., the stronger-than-normal Australian “winter” monsoon forcing positively large precipitation anomalies over IMC and to the south through the activation of vertical instability near the surface. The positive precipitation anomalies retain the upward branch of Walker circulation around IMC and overcome the effects of Kelvin wave from the tropical Indian Ocean and others inducing the transition from La Niña to El Niño. Thus, La Niña continues until boreal fall or winter, while El Niño decays by boreal spring or summer without such self-maintenance mechanism.