Art

J-GLOBAL ID：201802241788879365   Reference number：18A2080961

Onset mechanism of solar eruptions

太陽噴火の開始機構【JST・京大機械翻訳】

Author (4)： Inoue Satoshi (Max-Planck-Institut Fuer Sonnensystemforschung, Justus-von-Liebig 3, 337077, Gottingen, Germany) ,  Inoue Satoshi (Institute for Space-Earth Environmental Research, Nagoya University, Furo-Cho Chikusa-ku, Nagoya, 464-8601, Japan) ,  Bamba Yumi (Institute of Space and Astronautical Science (ISAS) / Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa, 252-5210, Japan) ,  Kusano Kanya (Institute for Space-Earth Environmental Research, Nagoya University, Furo-Cho Chikusa-ku, Nagoya, 464-8601, Japan)
Material： Journal of Atmospheric and Solar-Terrestrial Physics  (J Atmos Sol-Terr Phys)
Volume： 180  Page： 3-8  Publication year： 2018 
JST Material Number： C0269A  ISSN： 1364-6826  Document type： Article
Article type： 原著論文  Country of issue： Netherlands (NLD)  Language： ENGLISH (EN)

Abstract/Point： Solar eruptions are the most e...

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Thesaurus term： *eruptive activity ,  numerical analysis ,  simulation ,  energy ,  geomagnetism ,  filament ,  magnetic field ,  interplanetary space ,  *sun ,  plasma ,  solar flare ,  magnetosphere ,  reconnection of magnetic field lines ,  space weather ,  space weather forecast

Author keywords (5)： Sun:magnetic fields ,  Sun:solar flares ,  Sun:coronal mass ejections (CMEs) ,  Magnetohydrodynamics ,  Space weather

JST classification (1)： Solar system in general  (DB04010T)

Terms in the title (2)： 太陽 ,  噴火