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Prompt Particle Acceleration to Relativistic Energies During Current Loop Coalescence in Solar Flares
https://doi.org/10.15099/00004392
https://doi.org/10.15099/00004392a1237463-4d28-4fce-bb5c-6b6465c43829
名前 / ファイル | ライセンス | アクション |
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Kokiyo_40_01_Page134to159.pdf (2.3 MB)
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Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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公開日 | 2012-10-10 | |||||
タイトル | ||||||
タイトル | Prompt Particle Acceleration to Relativistic Energies During Current Loop Coalescence in Solar Flares | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 太陽フレア | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | Solar Flares | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 電流ループ合体 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | Current Loop Coalescence | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 相対論的エネルギー | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | Relativistic Energies | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 速い粒子加速 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | Prompt Particle Acceleration | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | High energy particle acceleration | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | impulsive phase | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | SMM | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
ID登録 | ||||||
ID登録 | 10.15099/00004392 | |||||
ID登録タイプ | JaLC | |||||
著者 |
中野, 融
× 中野, 融× 坂井, 純一 |
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著者別名 | ||||||
姓名 | Nakano, Tohru | |||||
著者別名 | ||||||
姓名 | Sakai, Jun-ichi | |||||
その他(別言語等)のタイトル | ||||||
その他のタイトル | 太陽フレアの電流ループ合体中における相対論的エネルギーまでの速い粒子加速 | |||||
抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | High energy particle acceleration during the current loop coalescence in solar flares is investigated by numerical simulation, based on the theoretical model derived by Sakai and Tajima (1986). Simulation results show that during the current loop coalescence, both electrons and protons can be quasi-periodically accelerated to relativistic energies within very short time (≪1s). These results can give a good explanation for the prompt high energy particle acceleration during the impulsive phase of solar flares. | |||||
引用 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 富山大学工学部紀要,40 | |||||
書誌情報 |
富山大学工学部紀要 巻 40, p. 134-159, 発行日 1989-03 |
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ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 03871339 | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AN00175872 | |||||
著者版フラグ | ||||||
出版タイプ | VoR | |||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
国立国会図書館分類 | ||||||
主題Scheme | NDLC | |||||
主題 | ZM2 | |||||
出版者 | ||||||
出版者 | 富山大学工学部 | |||||
資源タイプ(DSpace) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Article |