日本地球惑星科学連合2018年大会

講演情報

[EE] 口頭発表

セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT22] 核-マントルの相互作用と共進化

2018年5月24日(木) 10:45 〜 12:15 国際会議室(IC) (幕張メッセ国際会議場 2F)

コンビーナ:飯塚 毅(東京大学)、渋谷 秀敏(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)、土屋 卓久(愛媛大学地球深部ダイナミクス研究センター、共同)、太田 健二(東京工業大学大学院理工学研究科地球惑星科学専攻)、座長:福間 浩司(同志社大学)、佐藤 雅彦(東京大学大学院理学研究科地球惑星科学専攻)

12:00 〜 12:15

[SIT22-42] Paleomagnetic Directions of 3-5ka Basaltic Volcanoes in the Aso Central Cone, Kyushu Japan: Further Extension of the Paleosecular Variation Curve.

*渋谷 秀敏1治田 有里紗4望月 伸竜2宮縁 育夫3 (1.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、2.熊本大学大学院先導機構、3.熊本大学大学院先端科学研究部基礎科学部門総合理学分野、4.熊本大学理学部)

キーワード:古地磁気学、古地磁気永年変化、阿蘇火山

In the central cone of Aso volcano, Kyushu Japan, there are several basaltic activities of 3-5 ka in age. The lava flows from those cones spread on the northwestern flank of the central cones, and they were classified in the relation to the cones. The composition and lithology of those lavas are, however, often difficult to distinguish each other. We have carried out the paleomagnetic direction measurements to draw the paleomagnetic secular variation curve of the duration to extend it back to pre-historic ages. It also shows that the classification of the lavas should be revised.

The samples were collected from 35 sites, one from a scoria cone and others were from lavas, and they were measured their paleomagnetism. The magnetization of those samples is quite simple, as expected, and alternating field demagnetization well defines the primary component. The site mean directions align well on a couple of arcs, which define the paleosecular variation of those ages, 3-5ka. The lava flows and a welded scoria classified as of three centers (Komezuka, Akase and Nakadake) are well clustered and confirmed to a single or erupted very closely in time for each center. On the other hand, lava flows related to the other two centers (Ojo and Kishima) have multiple clusters in the paleomagnetic directions, and their ages estimated from the paleosecular variation curve interfinger to the classification.

It is also very interesting that there seems to be a stagnant point in secular variation just before 3ka, whose direction is similar to the known stagnant point in archeomagnetic secular variation at around 800CE. If there is tendency to stop the SV at the direction, it may be related to the core dynamo processes.