日本地球惑星科学連合2023年大会

講演情報

[J] オンラインポスター発表

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-EM15] 地磁気・古地磁気・岩石磁気

2023年5月24日(水) 10:45 〜 12:15 オンラインポスターZoom会場 (14) (オンラインポスター)

コンビーナ:吉村 由多加(九州大学大学院比較社会文化研究院)、臼井 洋一(金沢大学)


現地ポスター発表開催日時 (2023/5/23 17:15-18:45)

10:45 〜 12:15

[SEM15-P16] 阿蘇2/1溶岩の古地磁気学的研究

*望月 伸竜1、大西 優輝2石丸 聡子1 (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.熊本大学理学部)

キーワード:古地磁気方位、古地磁気永年変化、阿蘇2、秋田溶岩、岩戸溶岩、瀬田裏溶岩

We conducted a paleomagnetic study on lavas in the Aso caldera wall and out of the Aso caldera, called Aso-2/1 lavas. Stratigraphic levels of these lavas were recognized above Aso-1 pyroclastic flow deposit and below the Aso-2 pyroclastic flow deposit. We collected oriented samples from each of Hokamaki, Matoishi, Togawa, Tamaraigawa, Setaura, and Akita lavas, and the Aso-2 pyroclastic flow deposit. Paleomagnetic directional measurements using alternating field demagnetization were made on the samples. Our paleodirection results combined with the previous data indicate estimates on the temporal gaps between a lava and the Aso-2 pyroclastic flow deposit, and the temporal gaps between lava flows. The paleomagnetic direction of the Akita lava is indistinguishable from that of the Aso-2 pyroclastic flow deposit; this result indicates the Akita lava extruded just before the Aso-2 eruption. In contrast, the paleomagnetic direction of the Setaura lava differs by more than 15 degree from that of the Aso-2 pyroclastic flow deposit; this suggest a temporal gap of 300 year or longer. We will show a modified stratigraphic relationship of the Aso-2/1 lavas based on our paleomagnetic data.