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Measurement of high-energy cosmic-ray electrons with a Polar Patrol Balloon
https://doi.org/10.15094/00006289
https://doi.org/10.15094/00006289c91d4e11-838b-45b5-8291-c993432e58cf
名前 / ファイル | ライセンス | アクション |
---|---|---|
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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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× Yamagami, Takamasa× Yuda, Toshinori× Kasahara, Katsuaki |
|||||
著者所属(英) | ||||||
en | ||||||
Institute of Physics, Kanagawa University | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
Institute for Cosmic Ray Research, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
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 |
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出版者 | ||||||
出版者 | National Institute of Polar Research |