Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
The Earth Simulator Center, JAMSTEC, 3173-25 Showa-machi, Kanazawa-ku, Yokohama, 236-0001 Japan Simulator Center, 3173-25 Showa-machi, Kanazawa-ku, Yokohama, 236-0001 Japan Simulator Center, Japan Agency for Marine-Earth Science and Technology, Kanagawa, Japan
Solar Terrestrial Environment Lab, Nagoya university, Nagoya, Japan;
STELAB, Nagoya University, Nagoya, Japan;
STEL, Nagoya Univ., Nagoya, Japan;
Hiroshima Univ., Hiroshima, Japan
Earth Simulator Center, JAMSTEC, Showa-machi 3173-25, Yokohama, 236-0001 Japan Earth Simulator Center, 3173-25 Showa-machi, Kanazawa-ku, Yokohama, 236- 0001 Japan Simulator Center, JAMSTEC, 3173-25 Showa-machi, Kanazawa-ku, Yokohama, 236-0001 Japan School of Advanced Sciences of Matter, Hiroshima University, Japan
Graduate School of Advanced Sciences of Matter, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8530, Japan 3173-25 Showa-machi, Kanazawa-ku, Yokohama, 236-0001, Japan Earth Simulator Center, JAMSTEC, 3173-25 Showa-machi, Yokohama, 236-0001, Japan School of Advanced Sciences of Matter, Hiroshima University, Higashi-Hiroshima 739-8526, Japan
Earth Simulator Center, Japan Agency for Marine-Earth Science and Technology, 3173-25 Showa-machi, Kanazawa-ku, Yokohama 236-0001, Japan
Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya 464-8601, Japan; Japan Agency for Marine-Earth Science and Technology, Yokohama, Kanagawa 236-0001, Japan
The Earth Simulator Center, JAMSTEC, 3173-25, Showa-machi, Kanazawa-ku, Yokohama, 236-0001, Japan Syowa-machi, Kanazawa-ku, Yokohama, 236-0001, Japan of Materials Science, Faculty of Science, Hiroshima Uni
A comparative study of the evolving morphology of 2.5-D simulated CMEs to Earth's magnetosphere
A global MHD simulation of the Jovian magnetosphere interacting with/without the interplanetary magnetic field
A Positivity-Preserving Projection Method for Multi-Dimensional MHD Solvers
A quantitative MHD study of the relation among arcade shearing, flux rope formation, and eruption due to the tearing instability
A Robust MHD Scheme in Space Weather Modeling: A Carbuncle-Free HLL-type Solver
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