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  1. 原著論文

High energy electron observation by Polar Patrol Balloon flight in Antarctica

https://repo.qst.go.jp/records/44954
https://repo.qst.go.jp/records/44954
756a2a67-e23a-49be-ab29-56ecf36c6877
Item type 学術雑誌論文 / Journal Article(1)
公開日 2007-08-24
タイトル
タイトル High energy electron observation by Polar Patrol Balloon flight in Antarctica
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 Torii, Syoji

× Torii, Syoji

WEKO 446433

Torii, Syoji

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Tamura, Tadahisa

× Tamura, Tadahisa

WEKO 446434

Tamura, Tadahisa

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Yoshida, Kenji

× Yoshida, Kenji

WEKO 446435

Yoshida, Kenji

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Kitamura, Hisashi

× Kitamura, Hisashi

WEKO 446436

Kitamura, Hisashi

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Katayose, Yusaku

× Katayose, Yusaku

WEKO 446437

Katayose, Yusaku

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et.al

× et.al

WEKO 446438

et.al

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鳥居 祥二

× 鳥居 祥二

WEKO 446439

en 鳥居 祥二

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田村 忠久

× 田村 忠久

WEKO 446440

en 田村 忠久

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吉田 賢二

× 吉田 賢二

WEKO 446441

en 吉田 賢二

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北村 尚

× 北村 尚

WEKO 446442

en 北村 尚

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片寄 祐作

× 片寄 祐作

WEKO 446443

en 片寄 祐作

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抄録
内容記述タイプ Abstract
内容記述 We accomplished a balloon observation of the high-energy cosmic-ray electrons
in 10-1000 GeV to reveal the origin and the acceleration mechanism. The
observation was carried out for 15 days at an average altitude of 35 km by the Polar
Patrol Balloon (PPB) around Antarctica in January ,2004. The detector is an imaging
calorimeter composed of scintillating-fiber belts and plastic scintillation counters
sandwiched between lead plates. The geometrical factor is about 600 cm^2sr, and the
total thickness of lead absorber is 9 radiation lengths. The performance of the
detector has been confirmed by a test flight at the Sanriku Balloon Center and by an
accelerator beam test using the CERN-SPS (Super Proton Synchrotron at CERN).
The new telemetry system using the Iridium satellite, the power system supplied by
solar panels and the automatic flight level control operated successfully during the
flight. We collected 5.7*10^3 events over 100 GeV, and selected the electron candidates
by a preliminary data analysis of the shower images. We report here an outline
of both detector and observation, and the first result of the electron energy spectrum
over 100 GeV obtained by an electronic counter.
書誌情報 Advances in Polar Upper Atmosphere Research

巻 20, p. 52-62, 発行日 2006
ISSN
収録物識別子タイプ ISSN
収録物識別子 1345-1065
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