JpGU Meeting 2019
Session outline| Multidisciplinary and Interdisciplinary (M) | ||
|---|---|---|
| Session Sub-category | General Geosciences, Information Geosciences & Simulations(GI) | |
| Session ID | M-GI35 | |
| Title | Development of computational sciences on planetary formation, evolution and surface environment | |
| Short Title | Computational Planets | |
| Main Convener | Name | Yoshi-Yuki Hayashi |
| Affiliation | Department of Planetology/CPS, Graduate School of Science, Kobe University | |
| Co-Convener 1 | Name | Masaki Ogawa |
| Affiliation | Division of General Systems Studies, Graduate School of Arts and Sciences, University of Tokyo | |
| Co-Convener 2 | Name | Shigeru Ida |
| Affiliation | Earth-Life Science Institute, Tokyo Institute of Technology | |
| Co-Convener 3 | Name | Kanya Kusano |
| Affiliation | Institute for Space-Earth Environmental Research, Nagoya University | |
| Session Language | J | |
| Scope | 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". | |
| Presentation Format | Oral and Poster presentation | |
| Time | Presentation No | Title | Presenter | Abstract |
|---|---|---|---|---|
| Oral Presentation May 28 PM1 | ||||
| 13:45 - 14:00 | MGI35-01 | Simulation Studies of Solar Activities as a Cause of Solar-Terrestrial Environment Variation | Kanya Kusano | |
| 14:00 - 14:15 | MGI35-02 | Development of a global non-hydrostatic Martian atmospheric model and its high-resolution simulation | Hiroki Kashimura | |
| 14:15 - 14:30 | MGI35-03 | Numerical simulations on the collision, adhesion, and growth of dust particles in turbulent gas in a protoplanetary disk | Takashi Ishihara | |
| 14:30 - 14:45 | MGI35-04 | Development of N-body Simulation Code for Planetary System Formation With Particle-Particle Particle-Tree Scheme | Yota Ishigaki | |
| 14:45 - 15:00 | MGI35-05 | Current status of post-K Exploratory Challenge, computational planetary science | Junichiro Makino | |
| Presentation No | Title | Presenter | Abstract |
|---|---|---|---|
| Poster Presentation May 28 PM2 | |||
| MGI35-P01 | Global N-body Simulation from Inner Region to Outer Region | Junko Kominami | |
| MGI35-P02 | Attempts at numerical modeling of 3-D mantle convection with magmatism and plate tectonics | Masanori Kameyama | |
| MGI35-P03 | Surface zonal flows induced by anelastic thermal convection in a rapidly rotating spherical shell | Youhei SASAKI | |
| MGI35-P04 | Protostellar flares driven by accretion in protoplanetary disks | Shinsuke Takasao | |
| MGI35-P05 | Cross-reference simulations by scalable communication library for the study of wave-particle interactions in planetary magnetospheres | Yuto Katoh | |
| MGI35-P06 | Radiative transfer calculation for various planetary atmospheres: Application to a general circulation model | Yoshi-Yuki Hayashi | |
| MGI35-P07 | Effect of the compressibility of turbulent flows on dust particle collision statistics in a protoplanetary disk | Yoshiki Sakurai | |
| MGI35-P08 | Algorithms to use accelerators effectively with FDPS and performance of applications | Daisuke Namekata | |