日本地球惑星科学連合2014年大会

講演情報

インターナショナルセッション(ポスター発表)

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-IT03_29PO1] Structure and dynamics of Earth and Planetary deep interiors

2014年4月29日(火) 18:15 〜 19:30 3階ポスター会場 (3F)

コンビーナ:*田中 聡(海洋研究開発機構 地球内部ダイナミクス領域)、芳野 極(岡山大学地球物質科学研究センター)、亀山 真典(国立大学法人愛媛大学地球深部ダイナミクス研究センター)、趙 大鵬(東北大学大学院理学研究科附属地震・噴火予知研究観測センター)、ヘルンランド ジョン(東京工業大学 地球生命研究所)

18:15 〜 19:30

[SIT03-P05] CMB 電気伝導度不均質と非双極子磁場

*清水 久芳1 (1.東京大学地震研究所)

キーワード:地磁気, CMB

The effects of electromagnetic induction in the heterogeneous mantle on the observed electromagnetic fields have been studied numerically to investigate possible causes of short time-scale variation known as the geomagnetic jerk. We found previously that the jerk-like magnetic and electric field variations observed at the surface of Earth can be explained by an input of a sudden variation of the toroidal field at the top of the core and large-scale conductivity heterogeneity of which conductivity is about 100 times higher than the background electrical conductivity. In this study, the effect of the heterogeneity on the flow in the core and magnetic field is evaluated by using a simple plane model of a heterogeneous mantle. Preliminary results suggest that the signature of the magnetic field may be detected as a stationary field at the Earth's surface if the heterogeneity is planetary scale, but the penetration length of its effect in the core is much shorter than the length scale of the heterogeneity.