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Measurements of the relative abundances of high-energy cosmic-ray nuclei in the TeV/nucleon region
- Title
- Measurements of the relative abundances of high-energy cosmic-ray nuclei in the TeV/nucleon region
- Authors
- Ahn H.S.; Allison P.S.; Bagliesi M.G.; Barbier L.; Beatty J.J.; Bigongiari G.; Brandt T.J.; Childers J.T.; Conklin N.B.; Coutu S.; Duvernois M.A.; Ganel O.; Han J.H.; Jeon J.A.; Kim K.C.; Lee J.; Lee M.H.; Maestro P.; Malinin A.; Marrocchesi P.S.; Minnick S.; Mognet S.I.; Na G.W.; Nam J.; Nam S.; Nutter S.; Park I.H.; Park N.H.; Seo E.S.; Sina R.; Walpole P.; Wu J.; Yang J.; Yoon Y.S.; Zei R.; Zinn S.Y.
- Ewha Authors
- 양종만; 박일흥; 남신우
- SCOPUS Author ID
- 양종만; 박일흥; 남신우
- Issue Date
- 2010
- Journal Title
- Astrophysical Journal Letters
- ISSN
- 2041-8205
- Citation
- Astrophysical Journal Letters vol. 715, no. 2, pp. 1400 - 1407
- Indexed
- SCI; SCIE; SCOPUS
- Document Type
- Article
- Abstract
- We present measurements of the relative abundances of cosmic-ray nuclei in the energy range of 500-3980 GeV/nucleon from the second flight of the Cosmic Ray Energetics And Mass balloon-borne experiment. Particle energy was determined using a sampling tungsten/scintillating-fiber calorimeter, while particle charge was identified precisely with a dual-layer silicon charge detector installed for this flight. The resulting element ratios C/O, N/O, Ne/O, Mg/O, Si/O, and Fe/O at the top of atmosphere are 0.919 ± 0.123stat 0.030syst, 0.076 ± 0.019stat 0.013syst, 0.115 ± 0.031stat 0.004syst, 0.153 ± 0.039stat 0.005syst, 0.180 ± 0.045stat 0.006syst, and 0.139 ± 0.043stat 0.005 syst, respectively, which agree with measurements at lower energies. The source abundance of N/O is found to be 0.054 ± 0.013stat 0.009syst+0.010esc -0.017. The cosmic-ray source abundances are compared to local Galactic (LG) abundances as a function of first ionization potential and as a function of condensation temperature. At high energies the trend that the cosmic-ray source abundances at large ionization potential or low condensation temperature are suppressed compared to their LG abundances continues. Therefore, the injection mechanism must be the same at TeV/nucleon energies as at the lower energies measured by HEAO-3, CRN, and TRACER. Furthermore, the cosmic-ray source abundances are compared to a mixture of 80% solar system abundances and 20% massive stellar outflow (MSO) as a function of atomic mass. The good agreement with TIGER measurements at lower energies confirms the existence of a substantial fraction of MSO material required in the TeV per nucleon region. © 2010. The American Astronomical Society. All rights reserved.
- DOI
- 10.1088/0004-637X/715/2/1400
- Appears in Collections:
- 자연과학대학 > 물리학전공 > Journal papers
- Files in This Item:
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Measurements of the relative abundances of high-energy cosmic-ray nuclei in the TeV nucleon region.pdf(1.28 MB)
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