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  1. 極地研刊行誌
  2. 英文誌
  3. 極域宙空圏
  4. Advances in polar upper atmosphere research (ISSN 1345-1065)
  5. No.13 (Sep. 1999)

Measurement of high-energy cosmic-ray electrons with a Polar Patrol Balloon

https://doi.org/10.15094/00006289
https://doi.org/10.15094/00006289
c91d4e11-838b-45b5-8291-c993432e58cf
名前 / ファイル ライセンス アクション
KJ00000048029.pdf KJ00000048029 (718.1 kB)
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Item type 紀要論文(ELS) / Departmental Bulletin Paper(1)
公開日 1999-09-01
タイトル
タイトル Measurement of high-energy cosmic-ray electrons with a Polar Patrol Balloon
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 departmental bulletin paper
ID登録
ID登録 10.15094/00006289
ID登録タイプ JaLC
ページ属性
内容記述タイプ Other
内容記述 P(論文)
著者名(英) Torii, Shoji

× Torii, Shoji

en Torii, Shoji

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Yamagami, Takamasa

× Yamagami, Takamasa

en Yamagami, Takamasa

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Yuda, Toshinori

× Yuda, Toshinori

en Yuda, Toshinori

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Kasahara, Katsuaki

× Kasahara, Katsuaki

en Kasahara, Katsuaki

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著者所属(英)
言語 en
値 Institute of Physics, Kanagawa University
著者所属(英)
言語 en
値 Institute of Space and Astronautical Science
著者所属(英)
言語 en
値 Institute for Cosmic Ray Research, University of Tokyo
著者所属(英)
言語 en
値 Department of System Engineering, Shibaura Institute of Technology
抄録(英)
内容記述タイプ Other
内容記述 One of the major purpose of recent cosmic-ray studies is to know the origin, acceleration mechanism and propagation properties inside the Galaxy. Along this line many efforts have been spent to observe a precise spectrum of the electron component of cosmic-rays. The main difficulty to study high-energy electrons is the detection of these electrons. The flux is much lower than the abundant proton component, and we need an observation of long duration and a detector with a high rejection power against the background protons. We propose to carry a newly developed scintillating-fiber detector on the Polar Patrol Balloon (PPB) and to expose it for 30 days. The goal of this observation is to determine a definite electron energy-spectrum ranging from 10 GeV to TeV region based on a high statistical accuracy with a long exposure by the PPB. In the result, we can expect to obtain direct evidence for the origin of high-energy electrons and a precise knowledge of their propagation in the Galaxy including solar modulation effects on the electron flux.
雑誌書誌ID
収録物識別子タイプ NCID
収録物識別子 AA11397422
書誌情報 Advances in polar upper atmosphere research

巻 13, p. 176-181, 発行日 1999-09
出版者
出版者 National Institute of Polar Research
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