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Depth dependency of neutron density produced by cosmic rays in the lunar subsurface
https://repo.qst.go.jp/records/47204
https://repo.qst.go.jp/records/472041b2f96a5-6b55-4c02-bf35-dd4c469adf0b
Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2015-08-06 | |||||
タイトル | ||||||
タイトル | Depth dependency of neutron density produced by cosmic rays in the lunar subsurface | |||||
言語 | ||||||
言語 | jpn | |||||
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 |
Ota, S.
× Ota, S.× Sihver, L.× 小林, 進悟× Hasebe, N.× 小林 進悟 |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | Depth dependency of neutrons produced by cosmic rays (CRs) in the lunar subsurface was estimated using the three-dimensional Monte Carlo particle and heavy ion transport simulation code, PHITS, incorporating the latest high energy nuclear data, JENDL/ HE-2007. The PHITS simulations of equilibrium neutron density profiles in the lunar subsurface were compared with the measurement by Apollo 17 Lunar Neutron Probe Experiment (LNPE). Our calculations reproduced the LNPE data except for the 350–400 mg/cm2 region under the improved condition using the CR spectra model based on the latest observations, well-tested nuclear interaction models with systematic cross section data, and JENDL/HE-2007. |
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書誌情報 |
Advances in Space Research 巻 54, 号 10, p. 2114-2121, 発行日 2014-12 |
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出版者 | ||||||
出版者 | Elsevier | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0273-1177 |