Title of article :
Calorimetric electron telescope (CALET) for the Japanese Exposure Facility on the ISS Original Research Article
Author/Authors :
K. Yoshida، نويسنده , , S. Torii، نويسنده , , N. Tateyama، نويسنده , , T. Tamura، نويسنده , , T. Ouchi، نويسنده , , T. Kashiwagi، نويسنده , , K. Hibino، نويسنده , , J. Nishimura، نويسنده , , T. Yamagami، نويسنده , , Y. Saito، نويسنده , , H. Murakami، نويسنده , , T. Kobayashi، نويسنده , , Y. Komori، نويسنده , , K. Kasahara، نويسنده , , T. Yuda، نويسنده , , M. Ohnishi، نويسنده , , M. Shibata، نويسنده , , F. Makino، نويسنده ,
Issue Information :
دوهفته نامه با شماره پیاپی سال 2001
Pages :
6
From page :
681
To page :
686
Abstract :
The CALET (CALorimetric Electron Telescope) instrument is proposed for the observation of TeV electrons at the Japanese Experiment Module Exposure Facility (JEM/EF) on the ISS, which is composed of an imaging calorimeter with scintillating fibers and lead plates, and a total absorption calorimeter with BGO logs. Since TeV electrons could reach only from the nearby sources within a distance less than 1 kpc, we can expect that the energy spectrum has a structural component and the arrival directions show an anisotropy. Therefore, we should be able to localize and identify the nearby cosmic-ray sources by the TeV electron observation. We report the status of development of the CALET instrument, which has a capability to observe electrons up to 10 TeV and a proton rejection power of ∼ 106. We expect to observe ∼ 103 events over 1 TeV during the 3 years observation. By using the excellent imaging capability of the CALET, gamma-rays over the GeV region and the nuclear components up to 1015 eV might also be observed.
Journal title :
Advances in Space Research
Serial Year :
2001
Journal title :
Advances in Space Research
Record number :
1127355
Link To Document :
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