JpGU-AGU Joint Meeting 2017

講演情報

[JJ] ポスター発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS23] [JJ] 古気候・古海洋変動

2017年5月23日(火) 15:30 〜 17:00 ポスター会場 (国際展示場 7ホール)

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)、岡 顕(東京大学大気海洋研究所)、北場 育子(立命館大学古気候学研究センター)、佐野 雅規(総合地球環境学研究所)

[MIS23-P17] Winter monsoon intensification during the last geomagnetic reversal in the Chinese Loess Plateau

*上野 友輔1兵頭 政幸2楊 天水3加藤 茂弘4 (1.神戸大学大学院惑星学専攻、2.神戸大学内海域環境教育研究センター、3.中国地質大学、4.兵庫県立人と自然の博物館)

キーワード:冬季モンスーン、マツヤマ―ブリュンヌ境界、中国黄土高原

A link between geomagnetic field and climate is an unresolved long life research subject. Correlation between galactic cosmic rays (GCR) flux and low cloud cover can provide a theoretical rationale to this subject. Namely, the geomagnetic field intensity can change low cloud cover through GCR, and finally change the climate. The East Asian Monsoon (EAM) system significantly affects the climate in East Asia, including Japan. In order to clarify whether the EAM was influenced by geomagnetic field changes in the past, we analyzed loess paleosol deposits of the Chinese Loess Plateau (CLP) for the Marine Isotope Stage (MIS) 19 interglacial, during which the Matuyama-Brunhes magnetic polarity transition (MBT) accompanying a large field intensity decrease occurred.
For Chinese loess-paleosol deposits, magnetic susceptibility and frequency dependence are regarded as proxies of summer monsoon (SM) intensity, and grain size as a proxy of winter monsoon (WM) intensity. We collected samples from sections of about 7 m thick in Xifeng and 8 m thick in Lingtai, about 100 km south of Xifeng, in the CLP. Magnetic and grain size analyses were conducted at about 2.5~20-cm depth intervals. In both sites, the high-resolution paleomagnetic data reveal the detailed MBT with multiple polarity swings.
The SM and WM proxy curves, obtained from magnetic susceptibility and grain size data, show consistent variations well correlated the precessional sea level changes. The correlation shows that our data have an average resolution of about 120 yr. The SM intensity increases and WM intensity decreases during the MISs 19.3 and 19.1 seal-level highstands, and the opposite changes occur during the MIS 19.2 lowstand. This variation pattern is the same with the results of a number of previous studies. However, our high-resolution data reveal that the WM briefly strengthens around highstand MIS 19.3 which should be warm. The WM strengthening interval is partly overlapped with the MBT. According to the paleomagnetic intensity stack for the last 800 kyr (S-int 800), the WM strengthened when the geomagnetic field intensity decreased below one third of the present intensity, and also when the GCR flux increased to above 1.4 times, and about 2 times at maximum. The temporary WM strengthening occurred around highstand MIS 19.3 may be related to the climatic cooling observed in Osaka Bay, Lake Baikal, Israel, and Italy, probably caused by an increase in GCR due to the significant geomagnetic field decrease.