*Kuriki Murahashi1, Seiya Nishizawa2, Masaki Ishiwatari1, Masatsugu Odaka1, Kensuke Nakajima3, Shin-ichi Takehiro4, Ko-ichiro Sugiyama5, Yoshiyuki O. Takahashi6, Yoshi-Yuki Hayashi6 (1.Hokkaido University, 2.RIKEN Advanced Institute for Computational Science, 3.Kyushu University, 4.Research Institute for Mathematical Sciences, Kyoto University , 5.National Institute of Technology, Matsue College, 6.Kobe University / CPS)
M (Multidisciplinary and Interdisciplinary) » M-GI General Geosciences, Information Geosciences & Simulations
[M-GI32] [JJ] Development of computational sciences on planetary formation, evolution and surface environment
Mon. May 22, 2017 5:15 PM - 6:30 PM Poster Hall (International Exhibition Hall HALL7)
Computer simulations have been recognized as one of the fundamental tools in understanding planetary formation, evolution and diversity of surface environment.
However, is may be notified that the continuous development of computational abilities in recent years does not seem to be well utilized in improving numerical simulations in those fields; computational efficiency has been improved by 6 orders of magnitude compared from the early 90's, many of our simulations do not seem to catch up qualitatively and quantitatively such improvement.
We propose here in this session to ask those who are interested in computational sciences of various fields not only of planetary formation and evolution but also of earth and planetary sciences in general to join. The aim is to discuss various scientific and technical aspects of our numerical simulations to improve our skills to fully utilize those development of computational resources that is realized or will be realized in near future as "K" to "post-K".
*Yuta Kawai1,2, Yoshiyuki O. Takahashi1,6, Masaki Ishiwatari5, Seiya Nishizawa2, Shin-ichi Takehiro4, Kensuke Nakajima3, Hirofumi Tomita2, Yoshi-Yuki Hayashi1,6 (1.Kobe Univ., 2.RIKEN AICS., 3.Kyusyu Univ., 4.Kyoto Univ., 5.Hokkaido Univ., 6.CPS)
*Youhei SASAKI1, Shin-ichi Takehiro3, Masaki Ishiwatari2, Michio Yamada3 (1.Department of Mathematics, Kyoto University, 2.Department of Cosmosciences, Graduate school of Science, Hokkaido University, 3.Research Institute for Mathematical Sciences, Kyoto University)
*Hirotaka Hohokabe1, Masahiro Machida2 (1.Department of Earth and Planetary Sciences, Graduate School of Science, Kyushu University, 2.Department of Earth and Planetary Sciences, Faculty of Science, Kyushu University)