[J] Oral

M (Multidisciplinary and Interdisciplinary) » M-GI General Geosciences, Information Geosciences & Simulations

[M-GI40] Development of computational sciences on planetary formation, evolution and surface environment

convener:Yoshi-Yuki Hayashi(Department of Planetology/CPS, Graduate School of Science, Kobe University), Masaki Ogawa(Division of General Systems Studies, Graduate School of Arts and Sciences, University of Tokyo), Shigeru Ida(Earth-Life Science Institute, Tokyo Institute of Technology), Kanya Kusano(Institute for Space-Earth Environmental Research, Nagoya University)

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[MGI40-01] A calculation for the formation of sunspots in an unprecedentedly deep domain

*Hideyuki Hotta¹, Haruhisa Iijima² (1.Graduate School of Science, Chiba University, 2.Institute for Space-Earth Environmental Research, Nagoya University)

[MGI40-02] Dependence of sunspot appearance on the deep structure

*Akito Ishikura¹, Hideyuki Hotta² (1.Graduate School of Science and Engineering, Chiba University, 2.Graduate School of Science, Chiba University)

[MGI40-03] Influence of large-scale flow in the solar interior on the surface small-scale magnetic field

*Ken Takahata¹, Yusuke Iida², Hideyuki Hotta³ (1.Chiba University, 2.Niigada University, 3.Graduate School of Science, Chiba University)

[MGI40-04] Dust lifting and advection simulated by a non-hydrostatic general circulation model in a Mars-like atmosphere

*Hiroki Kashimura¹, Hisashi Yashiro², Seiya Nishizawa³, Hirofumi Tomita³, Kensuke Nakajima⁴, Masaki Ishiwatari⁵, Yoshiyuki O. Takahashi¹, Yoshi-Yuki Hayashi¹ (1.Department of Planetology, Graduate School of Science, Kobe University, 2.Center for Global Environmental Research, National Institute for Environmental Studies, 3.RIKEN Center for Computational Science , 4.Department of Earth and Planetary Sciences, Flculty of Sciences, Kyushu University, 5.Department of Cosmosciences, Graduate school of Science, Hokkaido University)

[MGI40-05] Attempts at numerical modeling of mantle convection of terrestrial bodies: from Moon, Earth, to super-Earths

*Masanori Kameyama^1,2, Masaki Ogawa^3,2, Takehiro Miyagoshi², Takatoshi Yanagisawa² (1.Geodynamics Research Center, Ehime University, 2.Japan Agency for Marine-Earth Science and Technology, 3.The University of Tokyo at Komaba)

[MGI40-06] A semi-Lagrangian advection model on the sphere using radial basis functions

*Takeshi Enomoto¹ (1.Disaster Prevention Research Institute, Kyoto University)