日本地球惑星科学連合2016年大会

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セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS17] 古気候・古海洋変動

2016年5月24日(火) 10:45 〜 12:15 A04 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*入野 智久(北海道大学 大学院地球環境科学研究院)、池原 実(高知大学海洋コア総合研究センター)、岡 顕(東京大学大気海洋研究所)、岡崎 裕典(九州大学大学院理学研究院地球惑星科学部門)、北場 育子(立命館大学古気候学研究センター)、北村 晃寿(静岡大学理学部地球科学教室)、佐野 雅規(総合地球環境学研究所)、多田 隆治(東京大学大学院理学系研究科地球惑星科学専攻)、中川 毅(立命館大学)、林田 明(同志社大学理工学部環境システム学科)、座長:岡 顕(東京大学大気海洋研究所)

11:45 〜 12:00

[MIS17-23] 40万年間の東シナ海のMg/Ca水温および酸素同位体比に基づく東アジア夏季モンスーン変動

*久保田 好美1脇坂 恵都子2Clemens Steven3Holbourn Ann4Lee Kyung Eun6Ziegler Martin7堀川 恵司2木元 克典5 (1.国立科学博物館、2.富山大学、3.Brown University、4.Christian-Albrechts-University、5.海洋研究開発機構、6.Korea Maritime University、7.Utrecht University)

キーワード:モンスーン、東シナ海、ミランコビッチ サイクル、Mg/Ca古水温、酸素同位体比

The East Asian summer monsoon (EASM) system is involved in the hydrological cycle and in latent heat and energy transport, and thus plays a crucial role in the regional and global climate system. Modern summer sea surface salinity in the northern part of the East China Sea (ECS) is mainly controlled by the discharge of the Yangtze River, which reflects East Asian summer monsoon (EASM) precipitation in the drainage area of the Yangtze River. Site U1429 was drilled by Integrated Ocean Drilling Program (IODP) Expedition 346 in the northern part of the ECS to reconstruct the Yangtze River discharge in high temporal resolution (~100 year resolution). A ~200 m long sediment succession was recovered, which covers the last 400 ky based on a benthic foraminiferal oxygen isotope. A record of oxygen isotope of seawater (δ18Ow) was reconstructed, based on high-resolution Mg/Ca and oxygen isotope measurements of the planktic foraminifera Globigerinoides ruber. The δ18Ow shows variations that have been in concert with Chinese spleothem oxygen isotope records on millennial to orbital scales. However, comparison with a global mean δ18Ow reveals that the δ18Ow of U1429 follows the global mean except from MIS 7.3 to MIS 6.4 and from MIS 5.4 to MIS 4, when the δ18Ow of U1429 was higher than the global mean during MIS 7.2, 6.4, 5.4, 5.2, 4 and lower during MIS 7.3, 7.1, 6.5, 5.3, 5.1. These intervals correspond to higher eccentricity periods during the last 400 ky. During these time periods, the amplitude variations of the regional δ18Ow increased, suggesting that the 23 ky amplitude of the EASM precipitation was also enhanced. These results suggest that the 23 ky amplitude of the EASM precipitation has been modulated by the eccentricity.