| Project/Area Number |
25257203
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| Research Category |
Grant-in-Aid for Scientific Research (A)
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| Allocation Type | Single-year Grants |
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| Section | 海外学術 |
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| Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
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| Research Institution | Kanagawa University |
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Principal Investigator |
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| Co-Investigator(Kenkyū-buntansha) |
日比野 欣也 神奈川大学, 工学部, 教授 (80260991)
鳥居 祥二 早稲田大学, 理工学術院, 教授 (90167536)
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| Co-Investigator(Renkei-kenkyūsha) |
TORII Shoji 早稲田大学, 理工学術院, 教授 (90167536)
KASAHARA Katsuaki 早稲田大学, 理工学術院, 招聘研究員 (00013425)
YOSHIDA Kenji 芝浦工業大学, システム工学部, 教授 (90260984)
KATAYOSE Yusaku 横浜国立大学, 工学研究科, 准教授 (90323930)
OZAWA Shunsuke 早稲田大学, 理工学術院, 研究員 (60506715)
SHIMIZU Yuki 神奈川大学, 工学部, 准教授 (60434320)
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| Research Collaborator |
Mitchell John William NASA Goddard Space Flight Center
Marrocchesi Pier Simone University of Siena and INFN Pisa
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| Project Period (FY) |
2013-04-01 – 2017-03-31
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| Project Status |
Completed (Fiscal Year 2016)
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| Budget Amount *help |
¥44,590,000 (Direct Cost: ¥34,300,000、Indirect Cost: ¥10,290,000)
Fiscal Year 2016: ¥8,970,000 (Direct Cost: ¥6,900,000、Indirect Cost: ¥2,070,000)
Fiscal Year 2015: ¥5,720,000 (Direct Cost: ¥4,400,000、Indirect Cost: ¥1,320,000)
Fiscal Year 2014: ¥11,570,000 (Direct Cost: ¥8,900,000、Indirect Cost: ¥2,670,000)
Fiscal Year 2013: ¥18,330,000 (Direct Cost: ¥14,100,000、Indirect Cost: ¥4,230,000)
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| Keywords | 宇宙線 / 宇宙物理 / 宇宙科学 / 国際宇宙ステーション / 加速器 |
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| Outline of Final Research Achievements |
A cosmic-ray detector, CALET, was launched in August 2015. It is successfully observing cosmic-ray electrons, gamma-rays, and nuclei on the International Space Station. Performances of the detector for the high energy cosmic rays are estimated by simulations for interactions of particles in the detector. Thus, it is very important to verify the simulations by beam tests. Therefore, we carried out heavy ion beam tests at CERN-SPS with a ground verification model which we assembled with Structure Thermal Models, Bread Board Models of readout electronics, and self-made electronics circuits equivalent to Flight Models. We could confirm that the simulations were consistent with the beam data.
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