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  1. 原著論文

Estimation method of planetary fast neutron flux by a Ge gamma-ray spectrometer

https://repo.qst.go.jp/records/47625
https://repo.qst.go.jp/records/47625
c27115b8-f2fb-45d1-9d60-c38dde65a938
Item type 学術雑誌論文 / Journal Article(1)
公開日 2017-01-30
タイトル
タイトル Estimation method of planetary fast neutron flux by a Ge gamma-ray spectrometer
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 Hareyama, M.

× Hareyama, M.

WEKO 477448

Hareyama, M.

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Fujibayashi, Y.

× Fujibayashi, Y.

WEKO 477449

Fujibayashi, Y.

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Yamashita, N.

× Yamashita, N.

WEKO 477450

Yamashita, N.

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Karouji, Y.

× Karouji, Y.

WEKO 477451

Karouji, Y.

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Nagaoka, H.

× Nagaoka, H.

WEKO 477452

Nagaoka, H.

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Kobayashi, S.

× Kobayashi, S.

WEKO 477453

Kobayashi, S.

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C., Reedy R.

× C., Reedy R.

WEKO 477454

C., Reedy R.

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Gasnault, O.

× Gasnault, O.

WEKO 477455

Gasnault, O.

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Forni, O.

× Forni, O.

WEKO 477456

Forni, O.

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d'Uston, C.

× d'Uston, C.

WEKO 477457

d'Uston, C.

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Kim, K.J.

× Kim, K.J.

WEKO 477458

Kim, K.J.

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小林 進悟

× 小林 進悟

WEKO 477459

en 小林 進悟

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抄録
内容記述タイプ Abstract
内容記述 An intensity map of lunar fast neutrons (LFNs) and their temporal variation has been estimated by fitting “sawtooth” peaks in the energy spectra of lunar gamma rays observed by the Kaguya (SELENE) Gamma Ray Spectrometer (GRS) consisting of a high-purity germanium (HPGe) detector with a BGO scintillator. While an ordinary peak in the spectrum is produced by only gamma ray lines, the sawtooth peak is produced by gamma ray lines and recoil nuclei in the detector by Ge(n,n′γ)Ge(n,n′γ) reaction. We develop a model for the shape of the sawtooth peak and apply it to fit sawtooth peaks together with ordinary peaks in actual observed spectra on the Moon. The temporal variation of LFNs is synchronous with that of galactic cosmic rays (GCRs), and the global distribution of fast neutrons on the lunar surface agrees well with the past observation reported by the Neutron Spectrometer aboard Lunar Prospector. Based on these results, a new method is established to estimate the flux of fast neutrons by fitting sawtooth peaks on the gamma ray spectrum observed by the HPGe detector.
書誌情報 Nuclear Instruments and Methods in Physics Research A

巻 828, p. 145-155, 発行日 2016-08
出版者
出版者 Elsevier Science
ISSN
収録物識別子タイプ ISSN
収録物識別子 0168-9002
DOI
識別子タイプ DOI
関連識別子 10.1016/j.nima.2016.05.045
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