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Fokker-Planck simulation of runaway electron generation in disruptions with the hot-tail effect
https://repo.qst.go.jp/records/48265
https://repo.qst.go.jp/records/48265e03c833b-92dc-4deb-8874-67cb74083fa2
| Item type | 学術雑誌論文 / Journal Article(1) | |||||
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| 公開日 | 2017-08-07 | |||||
| タイトル | ||||||
| タイトル | Fokker-Planck simulation of runaway electron generation in disruptions with the hot-tail effect | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| 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 | journal article | |||||
| アクセス権 | ||||||
| アクセス権 | metadata only access | |||||
| アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
| 著者 |
奴賀, 秀男
× 奴賀, 秀男× 矢木, 雅敏× 福山, 淳× 矢木 雅敏 |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | To study runaway electron generation in disruptions, we have extended the three-dimensional (3D) (2D in momentum space; 1D in the radial direction) Fokker-Planck code, which describes the evolution of the relativistic momentum distribution function of electrons and the induced toroidal electric field in a self-consistent manner. A particular focus is placed on the hot-tail effect in 2D momentum space. The effect appears if the drop of the background plasma temperature is sufficiently rapid compared with the electron-electron slowing down time for a few times of the pre-quench thermal velocity. It contributes to not only the enhancement of the primary runaway electron generation but also the broadening of the runaway electron distribution in the pitch angle direction. | |||||
| 書誌情報 |
PHYSICS OF PLASMAS 巻 23, 号 6, p. 062506-1-062506-8, 発行日 2016-06 |
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| 出版者 | ||||||
| 出版者 | AIP | |||||
| DOI | ||||||
| 識別子タイプ | DOI | |||||
| 関連識別子 | 10.1063/1.4953606 | |||||
| 関連サイト | ||||||
| 識別子タイプ | DOI | |||||
| 関連識別子 | http://dx.doi.org/10.1063/1.4953606 | |||||
| 関連名称 | http://dx.doi.org/10.1063/1.4953606 | |||||