Energy spectrum of cosmic-ray electrons in 10 -1000 GeV observed with the PPB-BETS over Antarctica

We present preliminary results on the spectrum of high energycosmic-ray electrons as the measured in the flightof the Polar Patrol Balloon (PPB) which lasted for 13 days,in January,2004 with a launch from Syowa Station, Antarctica.The PPB-BETS (Balloon-borne Electron Telescope with ScintillatingFibe...

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Main Author: Kitamura Hisashi
Format: Conference Object
Language:English
Published: 2019
Subjects:
Online Access:https://repo.qst.go.jp/?action=repository_uri&item_id=60489
http://id.nii.ac.jp/1657/00060477/
id ftnirs:oai:repo.qst.go.jp:00060489
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spelling ftnirs:oai:repo.qst.go.jp:00060489 2023-05-15T13:52:37+02:00 Energy spectrum of cosmic-ray electrons in 10 -1000 GeV observed with the PPB-BETS over Antarctica Kitamura Hisashi 2019-02-18 https://repo.qst.go.jp/?action=repository_uri&item_id=60489 http://id.nii.ac.jp/1657/00060477/ en eng https://repo.qst.go.jp/?action=repository_uri&item_id=60489 http://id.nii.ac.jp/1657/00060477/ 2004-07-25 Presentation 2019 ftnirs 2021-12-30T07:53:54Z We present preliminary results on the spectrum of high energycosmic-ray electrons as the measured in the flightof the Polar Patrol Balloon (PPB) which lasted for 13 days,in January,2004 with a launch from Syowa Station, Antarctica.The PPB-BETS (Balloon-borne Electron Telescope with ScintillatingFiber) detector is designed to measure the cosmic-ray electron spectrumfrom 10 GeV to 1 TeV during a long balloon flight.It consists of 9 plates of plastic scinlater as a calorimeterand a scintillating fiber trackers for cascade showersinduced from high energy electrons and protonsbetween plates of lead with total 9 radiation length thickness.In this paper, we discuss the perfomance of the detectorand the preliminary results on the spectrum of cosmic-ray electrons. 35th COSPAR SCIENTIFIC ASSEMBLY Conference Object Antarc* Antarctica National Institute of Radiological Science: NIRS-Repository Syowa Station
institution Open Polar
collection National Institute of Radiological Science: NIRS-Repository
op_collection_id ftnirs
language English
description We present preliminary results on the spectrum of high energycosmic-ray electrons as the measured in the flightof the Polar Patrol Balloon (PPB) which lasted for 13 days,in January,2004 with a launch from Syowa Station, Antarctica.The PPB-BETS (Balloon-borne Electron Telescope with ScintillatingFiber) detector is designed to measure the cosmic-ray electron spectrumfrom 10 GeV to 1 TeV during a long balloon flight.It consists of 9 plates of plastic scinlater as a calorimeterand a scintillating fiber trackers for cascade showersinduced from high energy electrons and protonsbetween plates of lead with total 9 radiation length thickness.In this paper, we discuss the perfomance of the detectorand the preliminary results on the spectrum of cosmic-ray electrons. 35th COSPAR SCIENTIFIC ASSEMBLY
format Conference Object
author Kitamura Hisashi
spellingShingle Kitamura Hisashi
Energy spectrum of cosmic-ray electrons in 10 -1000 GeV observed with the PPB-BETS over Antarctica
author_facet Kitamura Hisashi
author_sort Kitamura Hisashi
title Energy spectrum of cosmic-ray electrons in 10 -1000 GeV observed with the PPB-BETS over Antarctica
title_short Energy spectrum of cosmic-ray electrons in 10 -1000 GeV observed with the PPB-BETS over Antarctica
title_full Energy spectrum of cosmic-ray electrons in 10 -1000 GeV observed with the PPB-BETS over Antarctica
title_fullStr Energy spectrum of cosmic-ray electrons in 10 -1000 GeV observed with the PPB-BETS over Antarctica
title_full_unstemmed Energy spectrum of cosmic-ray electrons in 10 -1000 GeV observed with the PPB-BETS over Antarctica
title_sort energy spectrum of cosmic-ray electrons in 10 -1000 gev observed with the ppb-bets over antarctica
publishDate 2019
url https://repo.qst.go.jp/?action=repository_uri&item_id=60489
http://id.nii.ac.jp/1657/00060477/
geographic Syowa Station
geographic_facet Syowa Station
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation https://repo.qst.go.jp/?action=repository_uri&item_id=60489
http://id.nii.ac.jp/1657/00060477/
2004-07-25
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