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A future plan in observing ultra-heavy nuclei (Z=30-110) of cosmic rays with large-scale collector at the lunar base

https://repo.qst.go.jp/records/45717
https://repo.qst.go.jp/records/45717
ac1fbc0c-feb7-4d57-bddf-aebbc337b324
Item type 学術雑誌論文 / Journal Article(1)
公開日 2010-01-05
タイトル
タイトル A future plan in observing ultra-heavy nuclei (Z=30-110) of cosmic rays with large-scale collector at the lunar base
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 Hasebe, Nobuyuki

× Hasebe, Nobuyuki

WEKO 454424

Hasebe, Nobuyuki

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Kodaira, Satoshi

× Kodaira, Satoshi

WEKO 454425

Kodaira, Satoshi

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Hareyama, Makoto

× Hareyama, Makoto

WEKO 454426

Hareyama, Makoto

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Yasuda, Nakahiro

× Yasuda, Nakahiro

WEKO 454427

Yasuda, Nakahiro

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小平 聡

× 小平 聡

WEKO 454428

en 小平 聡

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安田 仲宏

× 安田 仲宏

WEKO 454429

en 安田 仲宏

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抄録
内容記述タイプ Abstract
内容記述 Lunar-based measurement of galactic cosmic ray (GCR) nuclei with a high precision is a challenging approach in cosmic ray research for the coming 20 years. This approach focuses to measure the elemental composition of Pt- and Pb-groups, actinide and possibly trans-uranic nuclei of Pu and Cm. The observation covers a wide range of scientific themes including the study on the origin of GCR nuclei, the characteristic time, heating and acceleration mechanism of GCR particles. A large-scaled particle telescope is required in order to measure those nuclides with high precision. Solid state nuclear track detectors (SSTDs) with a geometric factor of about 1000 m2sr allow us to measure them easily. Fluorescent nuclear track detector such as Al2O3 doped with C and Mg is the best candidate at present among SSTDs for a lunar-based experiment which is currently the focus of an international program of scientific investigation. A permanent sunshine region near crater at lunar polar region is thought to be an excellent site. A two-year-exposure by the large-scaled telescope would result in the detection of about 30,000 actinides in GCRs.
書誌情報 Radiation Measurements

巻 44, 号 9-10, p. 913-916, 発行日 2009-10
ISSN
収録物識別子タイプ ISSN
収録物識別子 1350-4487
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