日本地球惑星科学連合2024年大会

講演情報

[J] ポスター発表

セッション記号 S (固体地球科学) » S-TT 計測技術・研究手法

[S-TT34] 空中からの地球計測とモニタリング

2024年5月27日(月) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

コンビーナ:小山 崇夫(東京大学地震研究所)、楠本 成寿(京都大学大学院理学研究科附属地球熱学研究施設)、光畑 裕司(独立行政法人 産業技術総合研究所)、上田 匠(早稲田大学)

17:15 〜 18:45

[STT34-P02] 伊豆大島におけるドローン繰り返し空中磁気測量

*小山 崇夫1金子 隆之1大湊 隆雄1渡邉 篤志1、八木 健夫1 (1.東京大学地震研究所)

キーワード:空中磁気測量、ドローン、伊豆大島

We've conducted aeromagnetic survey in the caldera of Izu Oshima volcano by using a multirotor drone.
Izu Oshima is a basaltic active volcano, and multidisciplinary surveys and monitoring measurements are being performed. Grounded-based geomagnetic continuous observation shows that remagnetization process in caldera is ceasing. It may indicate that heat cooling since the last eruption in 1986 almost stops and preparation for the next event is starting.
In order to reveal the present condition of the shallow subsurface in the caldera, we obtained a wide and dense magnetic field data at the low altitude above the surface by aeromagnetic survey. The target area is 3 km by 3 km including the A crater and the B fissure of the 1986 eruption. Measurement height and line interval was almost kept at 50 m. Measurement of the geomagnetic field was done by using the optical pumping total intensity magnetometer.
As the result of modeling of the subsurface structure, lineation of magnetization appeared in the NW-SE direction, which is identical to the regional stress field. Especially, the region beneath the B fissure shows very low magnetization. It shows that the NW-SE line beneath the B fissure is structurally weak, and has potential to erupt in the future.
Also, preliminary data processing detected that the magnetization change of the model benath the A crater in negative and the B fissure in positive. It may indicates that the A crater is getting some heat supply while the B fissure is still cooling.