Item type |
紀要論文(ELS) / Departmental Bulletin Paper(1) |
公開日 |
1999-09-01 |
タイトル |
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タイトル |
Measurement of high-energy cosmic-ray electrons with a Polar Patrol Balloon |
言語 |
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言語 |
eng |
資源タイプ |
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資源タイプ識別子 |
http://purl.org/coar/resource_type/c_6501 |
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資源タイプ |
departmental bulletin paper |
ID登録 |
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ID登録 |
10.15094/00006289 |
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ID登録タイプ |
JaLC |
ページ属性 |
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内容記述タイプ |
Other |
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内容記述 |
P(論文) |
著者名(英) |
Torii, Shoji
Yamagami, Takamasa
Yuda, Toshinori
Kasahara, Katsuaki
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著者所属(英) |
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言語 |
en |
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値 |
Institute of Physics, Kanagawa University |
著者所属(英) |
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言語 |
en |
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値 |
Institute of Space and Astronautical Science |
著者所属(英) |
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言語 |
en |
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値 |
Institute for Cosmic Ray Research, University of Tokyo |
著者所属(英) |
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言語 |
en |
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値 |
Department of System Engineering, Shibaura Institute of Technology |
抄録(英) |
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内容記述タイプ |
Other |
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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 |
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収録物識別子タイプ |
NCID |
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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 |
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出版者 |
National Institute of Polar Research |