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(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-IT03_29AM1] Structure and dynamics of Earth and Planetary deep interiors

2014年4月29日(火) 09:00 〜 10:45 418 (4F)

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)、座長: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)、芳野 極(岡山大学地球物質科学研究センター)

09:00 〜 09:15

[SIT03-01] Effect of the upper mantle structure on the Moho geometry

*TENZER Robert1CHEN Wenjin1 (1.School of Geodesy and Geomatics, Wuhan University)

キーワード:crust, density, gravity, mantle, Moho

We investigate the effect of the lateral density structure within the upper (most) mantle on the Moho geometry. The gravimetric forward and inverse modeling methods are applied to determine the Moho depths using the gravity data corrected for major known anomalous density structures within the Earth crust. In our numerical experiment we compute and compare the Moho geometry determined using uniform and laterally varying models of the Moho density contrast. The laterally varying model of the Moho density contrast incorporates the information on the upper mantle lateral density structure taken from the CRUST1.0 global crustal model. For the uniform density contrast model, the constant value of the Moho density contrast is determined based on minimizing the spatial correlation between the gravity data and the Moho geometry. Except for the upper (most) mantle, the deeper heterogeneous mantle density structures including the core-mantle boundary zone are not taken into consideration due to the absence of a reliable 3-D density model of the whole mantle. The numerical results revealed that the consideration of the upper mantle density structure improves the fit of the gravimetric solution with the seismic Moho model.