Three-Dimensional Simulation of Solar Emerging Flux Using the Earth Simulator : I. Magnetic Rayleigh-Taylor Instability at the Top of the Emerging Flux as the Origin of Filamentary Structure
スポンサーリンク
概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 2006-04-25
著者
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ISOBE Hiroaki
Department of Pathology, Tama-Nagayama Hospital, Nippon Medical School
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Isobe Hiroaki
Department Of Earth And Planetary Science The University Of Tokyo
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横山 央明
Department Of Earth And Planetary Science The University Of Tokyo
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Isobe Hiroaki
Univ. Tokyo Tokyo
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SHIBATA Kazunari
Kwasan and Hida Observatories, Department of Astronomy, Kyoto University
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YOKOYAMA Takaaki
Department of Earth and Planetary Science, The University of Tokyo
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Isobe Hiroaki
Unit Of Synergetic Studies For Space Kwasan Observatory Kyoto University
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MIYAGOSHI Takehiro
Kwasan and Hida Observatories, Kyoto University
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Shibata K
Kwasan And Hida Observatory Kyoto University
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Shibata Kazunari
Kwasan And Hida Observatories Kyoto University
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Miyagoshi Takehiro
Kwasan And Hida Observatories Kyoto University
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Yokoyama Takaaki
Department Of Earth And Planetary Science The University Of Tokyo
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Shibata Kazunari
Kwasan And Hida Observatories Department Of Astronomy Kyoto University
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