Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Kwasan and Hida Observatories, Kyoto University
Kwasan and Hida Observatory, Kyoto University
Kwasan and Hida Observatoires, Kyoto, Japan
Kwasan and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto 607-8471
Kwasan and Hida Observatoires, Kyoto University, Yamashina, Kyoto 607-8471, Japan.
Kwasan and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto 607-8471, Japan.
Kwasan and Hida Observatoires, Kyoto University
Kwasan and Hida Observatoires, Kyoto University, Sakyo-ku, Kyoto, 606-8502 Japan
Hida Observatory, Gifu, Japan
Kwasan Observatory, Kyoto University, Yamashina-Ku, Kyoto 607-8471
Kwasan Observatory, Kyoto University, Yamashina-ku, Kyoto 607-8471
Kwasan and Hida Observatoires, University of Kyoto Kamitakara
Kwasan and Hida Observatoires, Kamitakara, Japan
Hida Observatory, Kyoto University, Kamitakara, Gifu 506-13
Kyoto University, Gifu, Japan
Kwasan and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto 607-8471, Japan and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto 607-8471, Japan and Hida Observatoires, Yamashina, Japan
Yamashina, Kyoto, 604-8471, Japan Univ.
Kwasan and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto, Japan
Kwasan and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto, 607-8471, Japan
Kwasan Observatory, Yamashina, Kyoto, Japan
Kwasan and Hida Observatoires, Kyoto University, Gifu 506-13, Japan
Kwasan and Hida Observatoires, Kyoto University, Kyoto 606-01, Japan
Kwasan and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto, Japan Observatory, Kyoto University, Yamashina-Ku, Kyoto 607-8471, Japan
Kwasan and Hida Observatoires, Gifu, Japan
Kwasan an
A coronal condensation observed at the total solar eclipse of June 11, 1983 and a related transient prominence
A Filament Eruption and Accompanying Coronal Field Changes on November 5, 1992
A Method for the Determination of 3-D Velocity Fields of Disappearing Solar Filaments
A Morphological Study of Magnetic Shear Development in a Flare-Productive Region NOAA 7270
A Multiple Flare Scenario where the Classic Long-Duration Flare Was Not the Source of a CME
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