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Capability of the CALET experiment for measuring elemental abundances of galactic cosmic ray nuclei heavier than nickel (Z=28)
B. F. Rauch
, W. R. Binns
, M. H. Israel
, P. S. Marrocchesi
, Y. Shimizu
, S. Torii
Department of Physics
Research output
:
Contribution to conference
›
Paper
›
peer-review
7
Scopus citations
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Keyphrases
International Space Station
100%
Elemental Abundances
100%
Imaging Calorimeter
100%
Cosmic Ray nuclei
100%
Galactic Cosmic Rays
100%
Radiation Length
100%
Dynamic Range
50%
Tungsten
50%
Proton
50%
Energy Spectrum
50%
Number of Events
50%
Spaceflight
50%
Maximum Charge
50%
Energy Range
50%
Lead Tungstate
50%
Gamma Rays
50%
Charge Resolution
50%
Scintillating Fibers
50%
Total Absorption Calorimeter
50%
Electron Energy Spectrum
50%
Segmented Plastic Scintillator
50%
Measuring Module
50%
Physics
Calorimeter
100%
Heavy Nuclei
100%
Galactic Cosmic Ray
100%
Particle Telescopes
100%
Elemental Abundance
100%
Energy Spectra
66%
Scintillating Fiber
33%
Electron Energy
33%
Dynamic Range
33%
Gamma Radiation
33%
Iron
33%