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Study of first orbit losses of 1 MeV tritons using the Lorentz orbit code in the LHD
http://hdl.handle.net/10655/00012563
http://hdl.handle.net/10655/0001256341b13f44-8082-4b77-a013-8420e25da032
名前 / ファイル | ライセンス | アクション |
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Plasma_Sci.Techn21(2)_pp025102 (1.0 MB)
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Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2021-07-13 | |||||
タイトル | ||||||
タイトル | Study of first orbit losses of 1 MeV tritons using the Lorentz orbit code in the LHD | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | the Large Helical Device | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | tritons | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | energetic ion | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | first orbit loss | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | Lorentz orbit code | |||||
キーワード | ||||||
主題Scheme | Other | |||||
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 | |||||
著者 |
OGAWA, Kunihoro
× OGAWA, Kunihoro× ISOBE, Mitsutaka× Nishitani, T.× MURAKAMI, Sadayoshi× SEKI, Ryosuke× NUGA, Hideo× PU, Neng× OSAKABE, Masaki× LHD, Experiment Group |
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著者ID | ||||||
内容記述タイプ | Other | |||||
内容記述 | 0000-0003-4555-1837 | |||||
抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | Shot-integrated measurement of the triton burnup ratio has been performed in the Large Helical Device. It was reported that the triton burnup ratio, defined as total DT neutron yield divided by total DD neutron yield, increases significantly in inward shifted configurations. To understand the magnetic configuration dependence of the triton burnup ratio, the first orbit loss fraction of 1 MeV tritons is evaluated by means of the Lorentz orbit code for various magnetic configurations. The first orbit loss of 1 MeV tritons is seen at t of less than 10−5 s and loss points of the triton are concentrated on the side of the helical coil case where the magnetic field is relatively weak. The significant decrease of the first orbit loss fraction by 15% is obtained with the inward shift of the magnetic axis position from 3.90 to 3.55 m. It is found that the decrease of first orbit loss is due to the reduction of the first orbit loss of transition and helically trapped tritons. | |||||
書誌情報 |
Plasma Science and Technology 巻 21, 号 2, p. 025102, 発行日 2019-01-11 |
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出版者 | ||||||
出版者 | IOP Publishing | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA12472636 | |||||
DOI | ||||||
識別子タイプ | DOI | |||||
関連識別子 | 10.1088/2058-6272/aaeba8 | |||||
権利 | ||||||
権利情報 | (c) 2019 Hefei Institutes of Physical Science, Chinese Academy of Sciences and IOP Publishing. | |||||
権利 | ||||||
権利情報 | This is the Accepted Manuscript version of an article accepted for publication in Plasma Science and Technology. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at https://doi.org/10.1088/2058-6272/aaeba8. | |||||
情報源 | ||||||
関連名称 | Kunihiro OGAWA et al 2019 Plasma Sci. Technol. 21 025102 | |||||
関連サイト | ||||||
識別子タイプ | DOI | |||||
関連識別子 | https://doi.org/10.1088/2058-6272/aaeba8 | |||||
関連名称 | Publisher version | |||||
NAIS | ||||||
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