日時: 2006(平成18)年11月14日 (火) 9:20~17日 (金) 17:00
場所: 海洋研究開発機構 横浜研究所 地球シミュレータセンター
主催者: (独)海洋研究開発機構 地球シミュレータセンター
申請代表者: 草野完也 ((独)海洋研究開発機構地球シミュレータセンター)
所内担当者: 大村善治 (京都大学生存圏研究所生存科学計算機実験分野)
生存圏である宇宙空間において、近未来に人類が安全に科学・経済活動を行うためには、宇宙環境の予報である「宇宙天気予報」は、重要な役割を果たし得る。本集会では、世界の指導的な研究者が一同に会して議論することにより、シミュレーションとモデリング研究の到達点を把握し、今後数年間の研究を先導する明確な指針を与えることを目指した。
生存科学計算機実験分野、生存圏電波応用分野。
November 14 | ||
(Chair: T. Sakurai) | ||
9:20– 9:30 |
Opening K. Kusano | |
9:30–10:00 |
S. Tsuneta (invited): “Hinode” A New Solar Observatory in Space —Current Status— | |
10:00–10:20 |
Y. Katsukawa: First Light of Solar Optical Telescope (SOT) on HINODE | |
10:20–10:40 |
H. Hara: Hinode X-ray Telescope and EUV Imaging Spectrometer | |
10:40–11:00 | break | |
(Chair: T. Obara) | ||
11:00–11:40 |
F. R. Toffoletto (invited): Magnetosphere-Ionosphere Coupling: A Modeler’s Perspective | |
11:40–12:00 |
H. Shinagawa: Development of the NICT real-time thermosphere-ionosphere simulator | |
12:00–12:40 |
H. Fujiwara (invited): GCM simulations of the thermaospherer/ionosphere | |
12:40–14:00 | lunch | |
(Chair: T. Yokoyama) | ||
14:00–14:40 |
V. Archontis (invited): Emergence and eruptions of magnetic flux in the solar atmosphere | |
14:40–15:00 |
H. Kurokawa: Observational Evidences of Emerging Twisted Magnetic Flux Ropes in Strong Flare Regions | |
15:00–15:20 |
N. Gopalswamy: Coronal Mass Ejections and Adverse Space Weather | |
15:20–15:40 |
S. Pohjolainen: Tracing CMEs from the corona to 1 AU in radio emission | |
Poster I (Chair: T. Yokoyama) | ||
15:40–16:10 | Short Oral Presentation | |
16:10–17:40 | Core Presentation Time | |
17:40–18:40 |
Virtual Conference I
| |
November 15 | ||
(Chair: T. Terasawa) | ||
9:00– 9:35 |
T. Wiegelmann (invited): Nonlinear force-free field modeling of the solar coronal magnetic field | |
9:35–10:00 |
Y. Yan (invited): Nonlinear Force-Free Field Modeling of Solar Coronal Magnetic Fields | |
10:00–10:20 |
H. He: Non-linear force-free magnetic field extrapolation scheme based on the direct boundary integral formulation | |
10:20–10:40 | break | |
(Chair: S. Machida) | ||
10:40–11:20 |
W. B. Manchester (invited): Simulations of the Sun-Earth System: Modeling the Halloween Events with SWMF | |
11:20–12:00 |
D. Odstrcil (invited): Numerical Modeling of May 1998 Interplanetary CME Events | |
12:00–12:20 |
K. Hayashi: MHD simulation of solar corona and solar wind and the sub-Alfvenic boundary treatments to utilize the measurement data | |
12:20–12:40 |
T. Miyoshi: A positively conservative scheme for MHD in space plasma simulations | |
12:40–14:00 | lunch | |
(Chair: K. Maezawa) | ||
14:00–14:40 |
G. Li (invited): Particle acceleration and transport in large SEP events | |
14:40–15:00 |
N. V. Nitta: SEP Properties and Magnetic Field Connection of the Source Region | |
15:00–15:20 |
M. Oka: Particle Acceleration by Shocks and the Whistler Critical Mach Number | |
15:20–15:40 |
I. Shinohara: Electron acceleration via magnetic island coalescence | |
15:40–16:00 | break | |
16:00–17:00 | “The Earth Simulator” Tour | |
17:00–18:00 | Bus Transportation | |
18:00–20:00 |
Banquet at China Town, Yokohama
| |
November 16 | ||
(Chair: M. Ugai) | ||
9:00– 9:40 |
T. Amari (invited): | |
9:40–10:20 |
B. Kliem (invited): Mechanisms and Kinematics of CoronalMass Ejections | |
10:20–10:40 |
D. Shiota: Three dimensional Magnetohydrodinamic modeling of Coronal Mass Ejections | |
10:40–11:00 | break | |
(Chair: M. Hoshino) | ||
11:00–11:40 |
T. G. Onsager (invited): Scientific Model Developments Needed to Mitigate Space Weather Impacts | |
11:40–12:20 |
J. Raeder (invited): Progress and Challenges Modeling the Geospace Environment | |
12:20–12:40 |
T. Ogino: An MHD Simulation of the Solar Wind-Magnetosphere Interaction on Substorms and Magnetospheric Storms | |
12:40–14:00 | lunch | |
(Chair: Y. Omura) | ||
14:00–14:40 |
M. Fok (invited): Modeling the Inner Magnetosphere | |
14:40–15:00 |
R. Kataoka: MHD and ring current simulations of a superstorm on 20 November 2003 | |
15:00–15:20 |
H. Shimazu: Real-time global MHD simulation of the solar wind interaction with the earth’s magnetosphere | |
15:20–15:40 |
S. Fujita: A numerical simulation of an overshielding effect of the magnetospheric convection electric field | |
Poster II (Chair: Y. Omura) | ||
15:40–16:10 | Short Oral Presentation | |
16:10–17:40 | Core Presentation Time | |
17:40–18:40 |
Virtual Conference II
| |
November 17 | ||
(Chair: TBD) | ||
9:00– 9:40 |
M. Rempel (invited): Modeling and predicting solar cycles using a flux-transport dynamo | |
9:40–10:00 |
T. Magara: Photospheric and coronal activities dynamically produced by flux emergence | |
10:00–10:20 |
H. Wang: Correlation between Solar Flare Procuntivity and Photospheric Magnetic Field Properties | |
10:20–10:40 |
A. Asai: Anemone Structure and Geo-Effective Flares/CMEs | |
10:40–11:00 | break | |
(Chair: T. Kikuchi) | ||
11:00–11:40 |
B. T. Welsch (invited): Forecasting Space Weather with Dynamic Coronal Models | |
11:40–12:00 |
T. K. Suzuki: Forecasting Solar Wind Speeds | |
12:00–12:20 |
D. Nagata: Solar wind control of plasma number density in the near-Earth plasma sheet: Coordinated study of WIND-ACE/GEOTAIL observations | |
12:20–12:40 |
Y. Katoh: Particle simulation of VLF triggered emissions —roles of the nonlinear cyclotron resonant interaction in the wave generation process | |
12:40–14:00 | lunch | |
(Chair: TBD) | ||
14:00–14:40 |
K. Kusano (invited): Predictability of Solar Flare Onset and Multi-scale Modelings for Space Weather Dynamics | |
14:40–15:00 |
T. Sugiyama: MHD-PIC Interlocked Simulation Model for Magnetic Reconnection | |
15:00–15:20 |
T. Umeda: Polynomial interpolation for hyperbolic conservation laws (PIC) scheme: Application to Vlasov Simulations | |
15:20–15:40 |
K. Fujimoto: Magnetic Reconnection in Large and Fully Kinetic System | |
15:40–16:00 | break | |
Summary (Chair: K. Shibata) | ||
16:00–16:30 |
Y. Kamide: Toward the success of space weather predictions | |
16:30–17:00 |
Discussion & Closing K. Shibata |
November 14
Short Oral Presentation: (15:40–16:10)
Core Presentation Time: (16:10–17:40)
November 16
Short Oral Presentation: (15:40–16:10)
Core Presentation Time: (16:10–17:40)
ポスター PDF ファイル (1 019 673 バイト) ポスター制作: 熨斗千華子 (京都大学) |