Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Nobeyama Solar Radio Observatory, Minamisaku, Nagano, 384-1305, Japan and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto 607-8471, Japa; Research Fellows of the Japan Society for the Promotion of Science; Nobeyama Radio Observatory, Minamisaku, Nagano 384-1305, Japan. and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto 607-8471, Japan; Research Fellows of the Japan Society for the Promotion of Science.
Nobeyama Solar Radio Observatory, Minamisaku, Nagano 384-1305
Nobeyama Solar Radio Observatory, National Astronomical Observatory, Minamimaki, Minamisaku, Nagano 384-1305
Nobeyama Solar Radio Observatory, National Astronomical Observatory of Japan, Minamimaki, Minamisaku, Nagano 384-1305 and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto 607-8471, Japan; Research Fellow of the Japan Society for the Promotion of Science.
Kwasan and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto 607-8471, Japan
USSS, Kyoto, Japan;
Hida Oberservatory, Kyoto Univ, Takayama, Japan;
Kwasan Observatory, Kyoto University, Yamashina, Kyoto 607-8471, Japan;
Nobeyama Solar Radio Observatory, National Astronomical Observatory of Japan, Minamimaki, Minamisaku, Nagano, 384-1305, Japan Solar Radio Observatory, National Astronomical Observatory of Japan, Minamisaku, Nagano 384-1305, Japan; Unit of Synergetic Studies for Space, Kyoto University, Yamashina, Kyoto 607-8471, Japan
Nobeyama Solar Radio Observatory, Minamisaku, Nagano 384-1305, Japan.
Nobeyama Solar Radio Observatory, NAOJ, Minamisaku, Nagano, 384-1305 Japan Solar Radio Observatory, NAOJ, Nagano, Japan
A Quantitative Study of the Homologous Flares on 2000 November 24
A Study on Red Asymmetry of H-alpha Flare Ribbons Using Narrowband Filtergram in the 2001 April 10 Solar Flare
Anemone structure of Active Region NOAA 10798 and related geo-effective flares/ CMEs
Asymmetric Prominence Eruption: A "Domino Effect"?
Center-to-Limb Variation of Microwave Emissions from Thermal-Rich and Thermal-Poor Solar Flares
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