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富士山頂における宇宙線中性子測定

https://repo.qst.go.jp/records/54196
https://repo.qst.go.jp/records/54196
bd613180-2fa2-47df-80bc-28b00de1bc8a
Item type 会議発表論文 / Conference Paper(1)
公開日 2010-02-01
タイトル
タイトル 富士山頂における宇宙線中性子測定
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_5794
資源タイプ conference paper
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 矢島, 千秋

× 矢島, 千秋

WEKO 553315

矢島, 千秋

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保田, 浩志

× 保田, 浩志

WEKO 553316

保田, 浩志

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矢島 千秋

× 矢島 千秋

WEKO 553317

en 矢島 千秋

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保田 浩志

× 保田 浩志

WEKO 553318

en 保田 浩志

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内容記述タイプ Abstract
内容記述 To evaluate the model calculation, the measurement of cosmic neutron was performed in the Mt. Fuji Weather Station built at the summit of Mt. Fuji (3,776 m above see level) from July to August, 2008. Two types of detector were used. One was an extended energy-range rem counter, named WENDI-II, with a tungsten-mixed moderator covering almost a whole energy range of cosmic neutrons. The other was a phoswich detector developed by us for high-energy neutron measurement up to hundreds of MeV, which has a $phi$ 160 mm x 160 mm probe consisting of liquid scintillator and plastic scintillator. The averaged neutron ambient dose equivalent rate at the summit of Mt. Fuji obtained using the WENDI-II was about 0.1 [micro Sv/h], which is about 10 times greater than that at sea level. The signals of neutron obtained using the phoswich detector were discriminated from those of other particles, such as protons, electrons, muons, and photons, analyzed based on the difference of the decay time between the liquid scintillator and the plastic scintillator. It is the next task to obtain the cosmic neutron energy spectrum to unfold the discriminated neutron signals.
書誌情報 Proceedings of the Workshop on Environmental Radioactivity (KEK Proceedings)

号 2009-8, p. 31-35, 発行日 2009-11
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