日本地球惑星科学連合2015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-IS34] 古気候・古海洋変動

2015年5月28日(木) 11:00 〜 12:45 301A (3F)

コンビーナ:*山田 和芳(静岡県 文化・観光部 文化学術局 ふじのくに地球環境史ミュージアム整備課)、池原 実(高知大学海洋コア総合研究センター)、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)、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)、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:山田 和芳(静岡県 文化・観光部 文化学術局 ふじのくに地球環境史ミュージアム整備課)

11:45 〜 12:00

[MIS34-08] 西部赤道太平洋の生物生産量と底層流への地球軌道要素の影響:環境岩石磁気学による考察

*山崎 俊嗣1堀内 一穂2七山 太3 (1.東京大学大気海洋研究所、2.弘前大学大学院理工学研究科、3.産業技術総合研究所地質情報研究部門)

The Western Pacific Warm Pool (WPWP) has highest water temperature in the global ocean, and its spatiotemporal variations have significant impacts on large-scale atmospheric circulation and global hydrology. An environmental magnetic study was conducted on sediment cores of late Pleistocene age taken from water depths of 2500 to 4500m in the West Caroline Basin (WCB) offshore northern New Guinea to understand better the paleoceanography in WPWP. Sediments in the southern part of WCB are deposited under the influence of relatively strong bottom water currents parallel to the New Guinea Trench; this is evidenced by sediment grain-size spectra, anisotropy of magnetic susceptibility, and 3.5 kHz sub-bottom profiling records.
Magnetite dominates magnetic mineral assemblages of the sediments. This is evidenced by that isothermal remanent magnetization (IRM) acquisition curves are mostly explained by a low-coercivity component, and that the Verwey transition is obvious in low-temperature measurements. Existence of the sharp central ridges on first-order reversal curve (FORC) diagrams and transmission electron microscopy indicate the occurrence of biogenic magnetite, in addition to magnetostatically interacting pseudo-single-domain and multi-domain magnetites of probably terrigenous origin.
The ratio of anhysteretic remanent magnetization susceptibility to saturation IRM (kARM/SIRM, a proxy of biogenic to terrigenous magnetic mineral component) and acid solvable component (~carbonate content) are synchronous with northern-hemisphere summer insolation; peaks of the former two correspond to the insolation maxima. This suggests that in WCB ocean productivity and then population of magnetotactic bacteria are higher when the Australia-Indonesian summer monsoon is stronger at the insolation maxima. The precessional frequency is visible in volumetric magnetic susceptibility (k) variations at sites shallower than the carbonate compensation depth (CCD), but the eccentricity frequency becomes dominant in carbonate-free mass susceptibility (χcf). Sediment redistribution by bottom water currents, whose strength and paths may vary with glacial/interglacial changes, may be responsible for the eccentricity frequency in χcf.
On the Ontong-Java Plateau (OJP) to the east of WCB, on the other hand, the precessional frequency appears in k, but the eccentricity frequency dominates kARM/SIRM variations. This suggests that the kARM/SIRM ratio at OJP could be influenced by a terrigenous supply via the Equatorial Undercurrent, but not by the strength of the monsoon.