日本地球惑星科学連合2025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-EM16] 地磁気・古地磁気・岩石磁気・環境磁気

2025年5月25日(日) 09:00 〜 10:30 302 (幕張メッセ国際会議場)

コンビーナ:川村 紀子(海上保安大学校 基礎教育講座)、加藤 千恵(九州大学比較社会文化研究院)、座長:望月 伸竜(熊本大学大学院先端科学研究部 基礎科学部門 地球環境科学分野)

10:15 〜 10:30

[SEM16-06] Microscopic observation of iron oxide grains in basalts from the Agulhas Plateau drilled during IODP Expedition 392

*加藤 千恵1藤井 昌和2,3吉村 由多加2、Sprain Courtney J.4、Dallanave Edoardo5 (1.九州大学比較社会文化研究院、2.国立極地研究所、3.総合研究大学院大学、4.フロリダ大学、5.ミラノ大学)

Basaltic units drilled at the Agulhas Plateau during IODP Expedition 392 are expected to record the absolute paleointensity at the time of the Cretaceous Normal Superchron. We have been conducting paleointensity experiments by the Tsunakawa-Shaw method on samples taken from three of the six basaltic sills from Site U1580. However, the rate of samples that passed the standard acceptance criteria for reliable paleointensity estimate is only about 25%, even though the samples used in the experiments were preselected based on paleomagnetic and rock-magnetic analyses such as alternating field demagnetization (AFD) of the natural remanent magnetization (NRM) by the on-board superconducting rock magnetometer (SRM), magnetic hysteresis measurements, and thermomagnetic analysis. Therefore, we performed scanning electron microscope (SEM) and reflection microscope observations of polished sections of the sister samples used in paleointensity experiments, in order to clarify the characteristics of magnetic minerals in samples that passed or were rejected and to obtain a guideline for sample selection. In the rejected samples, euhedral or dendritic iron oxides with grain sizes ranging from a few hundred micrometers to over 1 mm were observed, and many of them showed Ti-rich fine lamellae. On the other hand, the passed samples did not show such coarse-grained iron oxides; instead they contained fine particles with grain sizes less than 10 micrometers. These results indicate that cooling rate is a key factor controlling the stability of the magnetic carriers. Indeed, all of the passed samples were collected within 80 cm from the upper or lower margin of a sill, while most of the rejected samples were taken from the middle of a sill. Therefore, we conclude that rapidly cooled areas near the margin of a sill should be selected for paleointensity experiments.