[M-GI36] Computational sciences on the universe, galaxies, stars, planets and their environments

[MGI36-P06] Stable plate motion and its features reproduced in a 3D spherical model of mantle convection with stress history dependent rheology

*Takehiro Miyagoshi¹, Masanori Kameyama², Masaki Ogawa³ (1. Japan Agency for Marine-Earth Science and Technology, 2. Ehime University, 3. The University of Tokyo (retired) )

Keywords:plate motion, 3D spherical mantle convection, stress history dependent rheology, numerical model