日本地球惑星科学連合2018年大会

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[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-IT27] 地球内部での液体の特性とその役割

2018年5月22日(火) 09:00 〜 10:30 A11 (東京ベイ幕張ホール)

コンビーナ:坂巻 竜也(東北大学大学院理学研究科)、中島 陽一(熊本大学大学院先導機構)、座長:坂巻 竜也(東北大学)、中島 陽一(熊本大学)

09:00 〜 09:15

[SIT27-01] Understanding of low velocity anomaly in the asthenosphere inferred from elastic wave velocity measurement of partially molten rocks

*大橋 智典1坂巻 竜也1久野 直毅1肥後 祐司2柴崎 裕樹3鈴木 昭夫1 (1.東北大学大学院理学系研究科、2.(財)高輝度光科学センター、3.東北大学 学際科学フロンティア研究所)

キーワード:部分溶融、弾性波速度、アセノスフェア

The low velocity anomaly at the top of asthenosphere is one of important seismological features, and expected to be formed by carbon dioxide (CO2)-induced partial melting of mantle rock. For better constraint on the melt fraction and distribution in the low-velocity zone, a comparison between experimental velocity and geophysical observation is a straightforward approach. Here we have measured the elastic wave velocity of olivine + carbonate melt using in-situ ultrasonic technique under conditions relevant to the top of asthenosphere. Both of compressional (VP) and shear (VS) wave velocities became smaller with increasing the volume fraction of melt in the sample, and we found quantitatively the velocity attenuation as a function of melt fraction. Comparing with the low-velocity zone, we succeeded in understanding a suitable amount of melt in the asthenosphere. The presence of magmas below the lithosphere could serve as a lubricant for the dynamics of plate tectonics and be a magma source of petit-spot volcanoes located at the outer rise of the oceanic plate.