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 S (固体地球科学) » S-EM 固体地球電磁気学

[S-EM34] 地磁気・古地磁気・岩石磁気

2016年5月24日(火) 10:45 〜 12:15 コンベンションホールA (2F)

コンビーナ:*松島 政貴(東京工業大学大学院理工学研究科地球惑星科学専攻)、菅沼 悠介(国立極地研究所)、座長:菅沼 悠介(国立極地研究所)、畠山 唯達(岡山理科大学情報処理センター)

12:00 〜 12:15

[SEM34-06] 西部赤道太平洋の海底堆積物における堆積残留磁化獲得深度の検討

櫻本 晋洋1、*山崎 俊嗣1木元 克典2宮入 陽介1横山 祐典1 (1.東京大学大気海洋研究所、2.海洋研究開発機構)

キーワード:古地磁気強度、堆積残留磁化獲得深度、ベリリウム同位体

On reconstructing past geomagnetic-field variations from marine sediments, lock-in depth of post-depositional remanent magnetization (pDRM) acquisition has been controversial for a long time. By direct comparison of relative paleointensity (RPI) and 10Be flux, Suganuma et al. (2010, 2011) proposed a lock-in depth of ~15 cm, whereas Valet et al. (2014) reported ~0 cm. We studied lock-in depth of pDRM using a marine sediment core obtained from the West Caroline Basin in the equatorial Pacific Ocean (R/V “MIRAI” MR14-02 cruise, core PC01). RPI and 10Be flux did not show obvious constant shift around the onset of the Olduvai subchron and the Gauss-Matuyama transition. This implies a negligibly small lock-in depth for the studied core. We also examined the lock-in depth of the PC01 core by comparing δ18O based ages of recorded polarity boundaries and GPTS ages, and by comparisons of RPI records among PC01, MD982187 (Yamazaki and Oda, 2005) and IODP Site U1314 (Ohno et al., 2012), which have different sedimentation rates. The results were consistent with the negligibly small lock-in depth of the PC01 core. This contrasts to the ~15 cm lock-in depth of the MD982187 core (Suganuma et al, 2010, 2011), which was obtained from the same area. Furthermore, Horiuchi et al. (in press) obtained lock-in depths of ~6 cm and ~10 cm from two cores in the same area. Lock-in depth may depend on lithology and depositional processes of each core.