Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Univ. Cambridge
Kwasan and Hida Observatoires, Kyoto University, Yamashina, Kyoto 607-8471, Japan.
Kwasan and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto 607-8471, Japan and Hida Observatoires, Kyoto University
Kwasan and Hida Observatoires, Kyoto University, Kyoto 607-8471, Japan
Department of Earth and Planetary Science, University of Tokyo, Tokyo 113-0033, Japan
Department of Earth and Planetary Science, The University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033; Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK; Kwasan and Hida Observatoires, Kyoto University, Yamashina-ku, Kyoto 607-8471 and Hida Observatoires, Kyoto University, Yamashina, Kyoto 607-8471, Japan; Department of Astronomy, Kyoto University, Kyoto 606-8502, Japan.
Faculty of Science, Kumamoto Univ., Kurokami, Kumamoto, 860-8555 Japan of Earth and Planetary Science, University of Tokyo, Hongo, Bunkyo-ku, Tokyo, Japan univ, Kumamoto, Japan; of synergetic studies for Space, Kyoto University, Kyoto, Japan;
Kwasan Observatory, Kyoto University, Yamashina, Kyoto 607-8471, Japan;
Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Wilberforce Road, Cambridge, CB3 0WA, UK; Department of Earth and Planetary Science, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033, Japan University Graduate School of Science and Technology, 2-39-1 Kurokami, Kumamoto 860-8555, Japan, KUMAMOTO, 860-8555, Japan School of Sci. and Tech., Kumamoto Univ., 2-39-1, Kurokami, Kumamoto, 860-8555, Japan Observatory, Kyoto Univ., 17 Ohmine-cho Kita Kazan, Yamashina-ku, Kyoto
A Reexamination of the Evidence for Reconnection Inflow
A Study of a Tiny Two-Ribbon Flare Driven by Emerging Flux
Active Region Microflares From Hinode and RHESSI
An active region jet observed with Hinode
Analysis of the Temperature and Emission Measure of Solar Coronal Arcades and Test of a Scaling Law of Flare/Arcade Loop Length
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