Multidisciplinary and Interdisciplinary (M) | ||
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Session Sub-category | General Geosciences, Information Geosciences & Simulations(GI) | |
Session ID | M-GI30 | |
Title | Computational sciences on the universe, galaxies, stars, planets and their environments | |
Short Title | Computational universe and planets | |
Main Convener | Name | Wataru Ohfuchi |
Affiliation | Kobe University | |
Co-Convener 1 | Name | Junichiro Makino |
Affiliation | Kobe University | |
Co-Convener 2 | Name | Masanori Kameyama |
Affiliation | Geodynamics Research Center, Ehime University | |
Co-Convener 3 | Name | Hideyuki Hotta |
Affiliation | Nagoya University | |
Session Language |
J |
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Scope |
Computer simulations have played critical roles in elucidating and understanding the planetary formation and evolution, planetary surface environments and their diversity, the solar and stellar dynamics, and the structure formation and evolution of the universe. While computer performance has increased by seven orders of magnitude over the past 30 years, this has not necessarily improved simulation outcomes. In this session, we aim to explore how to exploit these improvements in computing performance to the quantitative and qualitative advancement of space, planet, and earth sciences with the current "Fugaku" and the coming post "Fugaku" computers. We invite presentations from theoretical, observational, numerical simulation and AI studies and will hold a session for comprehensive discussions on the future direction of the fields. We welcome cross-disciplinary participation from all fields of the Japan Geoscience Union, not limited to space, planet, and earth science. |
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Presentation Format | Oral and Poster presentation |
Time | Presentation No | Title | Presenter |
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Oral Presentation May 27 PM1 | |||
13:45 - 14:00 | MGI30-01 | Progress and Future Plans of the Program for Promoting Researches on the Supercomputer Fugaku: Structure and Evolution of the Universe Unraveled by Fusion of Simulation and AI | Ken Ohsuga |
14:00 - 14:15 | MGI30-02 | Jupiter's moist and thermal convection modulated by torsional oscillation | Kumiko Hori |
14:15 - 14:30 | MGI30-03 | Linear stability analysis of Boussinesq convection with explicit methods and its verification using a high-precision particle scheme | Kensuke Shobuzako |
14:30 - 14:45 | MGI30-04 | Unified N-body simulation of planet formation from planetesimal disk: The dynamic planet formation with planetary migration | Tenri Jinno |
14:45 - 15:00 | MGI30-05 | A Tracer Advection Scheme Based on the Particle-in-Cell Method on the 2-Sphere | Toshiki Matsushima |
15:00 - 15:15 | MGI30-06 | Collisional growth of dust in a turbulent protoplanetary disk | Takashi Ishihara |
Oral Presentation May 27 PM2 | |||
15:30 - 15:45 | MGI30-07 | Shallow-water models using cubed-sphere projection and radial basis functions | Takeshi Enomoto |
15:45 - 16:00 | MGI30-08 | Time evolution of spiral structures in the Moon-forming disk | Yoichi Yoshimura |
16:00 - 16:15 | MGI30-09 | Interfaces and Programming of OpenACC for MN-Core | Ryuta Tsunashima |
16:15 - 16:30 | MGI30-10 | Oligarchic growth of protoplanets in an expanding planetesimal ring | Yuki Kambara |
16:30 - 16:45 | MGI30-11 | Attempts for direct solution of flow fields of 3-D mantle convection on coarse Yin-Yang grids | Masanori Kameyama |
16:45 - 17:00 | MGI30-12 | Post-Fugaku Feasibility Study and Computational Astrophysics and Planetary Science | Junichiro Makino |
Presentation No | Title | Presenter |
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Poster Presentation May 27 PM3 | ||
MGI30-P01 | Experiment of Physics-Informed Neural Networks for Nonlinear Force-Free Field Extrapolation and its applicability | Chihiro Mitsuda |
MGI30-P02 | Fourier transform on the sphere starting from the latitudinal direction | Suzune Nomura |
MGI30-P03 | Temperature dependence of head-on collisions between dust monomers explored by molecular dynamics simulations | Yuki Yoshida |
MGI30-P04 | Attempt to estimate initial guesses for iterative solvers using polynomial extrapolation: Toward improving convergence of 3-D simulations of mantle convection | SOTO MIZUTANI |
MGI30-P05 | Introduction of moist process to an global atmospheric dynamical core using discontinuous Galerkin method and validation with a moist Held-Suarez test | Yuta Kawai |
MGI30-P06 | Machine Learning Model Predicting Planetary Formation in the Giant Impact Stage | Yuichiro Ishida |
MGI30-P07 | The adjustment of the horizontal diffusion coefficient to changes in the resolution of a general circulation model of the atmosphere | Wataru Ohfuchi |
MGI30-P08 | Mechanism of Magma Ascent from a Partially Molten Layer by a Coupled Magmatism-Mantle Convection System | Kenyo U |
MGI30-P09 | Anelastic thermal convection in a rapidly rotating spherical shell and surface banded structures of the Jovian planets | Youhei SASAKI |
MGI30-P10 | A formulation of a three-dimensional spectral atmospheric dynamical core using new vertical basis functions. | Shun Fujita |
MGI30-P11 | Plate motion reproduced in a spherical shell mantle convection model with stress-history-dependent viscosity and its characteristics | Takehiro Miyagoshi |