Japan Geoscience Union Meeting 2014

Presentation information

International Session (Oral)

Symbol S (Solid Earth Sciences) » S-IT Science of the Earth's Interior & Techtonophysics

[S-IT03_29AM1] Structure and dynamics of Earth and Planetary deep interiors

Tue. Apr 29, 2014 9:00 AM - 10:45 AM 418 (4F)

Convener:*Satoru Tanaka(Institute for Research on Earth Evolution Japan Agency for Marine-Earth Science and Technology), Takashi Yoshino(Institute for Study of the Earth's Interior, Okayama University), Masanori Kameyama(Geodynamics Research Center, Ehime University), Dapeng Zhao(Department of Geophysics, Tohoku University), John Hernlund(ELSI, Tokyo TECH), Chair:Dapeng Zhao(Department of Geophysics, Tohoku University), Takashi Yoshino(Institute for Study of the Earth's Interior, Okayama University)

9:00 AM - 9:15 AM

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

*Robert TENZER1, Wenjin CHEN1 (1.School of Geodesy and Geomatics, Wuhan University)

Keywords: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.