Abstract
The CALET space experiment, currently under development by Japan in collaboration with Italy and the United States, will measure the flux of Cosmic Ray electrons (including positrons) to 20 TeV, gamma rays to 10 TeV and nuclei with Z=1 to 40 up to 1,000 TeV during a five year mission. These measurements are essential to investigate possible nearby astrophysical sources of high energy electrons, study the details of galactic particle propagation and search for dark matter signatures. The instrument consists of a module to identify the particle charge, a thin imaging calorimeter (3 radiation lengths) with tungsten plates interleaving scintillating fiber planes, and a thick calorimeter (27 radiation lengths) composed of lead tungstate logs. CALET has the depth, imaging capabilities and energy resolution necessary for excellent separation between hadrons, electrons and gamma rays. The instrument is currently being prepared for launch, during the 2014 time frame, to the International Space Station (ISS) for installation on the Japanese Experiment Module - Exposed Facility (JEM-EF).
Original language | English |
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Title of host publication | Proceedings of the 33rd International Cosmic Rays Conference, ICRC 2013 |
Publisher | Sociedade Brasileira de Fisica |
Volume | 2013-October |
ISBN (Electronic) | 9788589064293 |
Publication status | Published - 2013 Jan 1 |
Event | 33rd International Cosmic Rays Conference, ICRC 2013 - Rio de Janeiro, Brazil Duration: 2013 Jul 2 → 2013 Jul 9 |
Other
Other | 33rd International Cosmic Rays Conference, ICRC 2013 |
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Country/Territory | Brazil |
City | Rio de Janeiro |
Period | 13/7/2 → 13/7/9 |
Keywords
- Calorimeter
- Dark matter
- Electrons
- ISS
- Neraby sources
ASJC Scopus subject areas
- Nuclear and High Energy Physics