Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Kwasan and Hida Observatoires, Kyoto University, Yamashina, Kyoto 607-8471, Japan.
Kwasan and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto 607-8471, Japan; Department of Astronomy, Kyoto University, Sakyo-ku, Kyoto 606-8502, Japan. and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto 607-8417
Kwasan and Hida Observatoires / Department of Astronomy, Faculty of Science, Kyoto University
Center for Computational Astrophysics, National Astronomical Observatory of Japan, Tokyo, Japan
Computational Astrophysics Lab, RIKEN, Tokyo, Japan; Saitama, Japan; 3173-25 Showa-machi, Kanazawa-ku, Yokohama, 236-0001, Japan Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan.
Computational Astrophysics Laboratory, Advanced Science Institute, RIKEN, 2-1, Hirosawa, Wako, Saitama 351-0198, Japan
The Earth Simulator Center, JAMSTEC, 3173-25, Showa-machi, Kanazawa-ku, Yokohama, 236-0001, Japan 3173-25, Showa-Cho, Kanazawa-ku, Yokohama, 236-0001, Japan Wako, Japan for Research on Earth Evolution, Japan Agency for Marine-Earth Science and Technology, Yokosuka, Japan
Computational Astrophysics Laboratory, Advanced Science Institute, RIKEN, Wako, Japan
National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo, 181-8588, Japan Nagoya University, Nagoya, Japan
A comparative study of the evolving morphology of 2.5-D simulated CMEs to Earth's magnetosphere
A quantitative MHD study of the relation among arcade shearing, flux rope formation, and eruption due to the tearing instability
A Study of a Tiny Two-Ribbon Flare Driven by Emerging Flux
Alfvén Wave and Nanoflare Reconnection Heating: How to Distinguish Them Observationally?
An MHD Model of the Major Solar Flare on 2006 December 13
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