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Cited by 334

The DOI matches its Crossref record; 18 of the 18 references it cites were found in a registry or an index.

COSMIC-RAY PROTON AND HELIUM SPECTRA FROM THE FIRST CREAM FLIGHT

Open access
Yoon, Y. S., Ahn, H. S., Allison, P. S., Bagliesi, M. G., Beatty, J. J., Bigongiari, G., Boyle, P. J., Childers, J. T., Conklin, N. B., Coutu, S., DuVernois, M. A., Ganel, O., Han, J. H., Jeon, J. A., Kim, K. C., Lee, M. H., Lutz, L., Maestro, P., Malinine, A., Marrocchesi, P. S., Minnick, S. A., Mognet, S. I., Nam, S., Nutter, S., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Swordy, S., Wakely, S. P., Wu, J., Yang, J., Zei, R., Zinn, S. Y.·2011·The Astrophysical Journal

Abstract

Cosmic-ray proton and helium spectra have been measured with the balloon-borne Cosmic Ray Energetics And Mass experiment flown for 42 days in Antarctica in the 2004–2005 austral summer season. High-energy cosmic-ray data were collected at an average altitude of ∼38.5 km with an average atmospheric overburden of ∼3.9 g cm −2 . Individual elements are clearly separated with a charge resolution of ∼0.15 e (in charge units) and ∼0.2 e for protons and helium nuclei, respectively. The measured spectra at the top of the atmosphere are represented by power laws with a spectral index of −2.66 ± 0.02 for protons from 2.5 TeV to 250 TeV and −2.58 ± 0.02 for helium nuclei from 630 GeV nucleon −1 to 63 TeV nucleon −1 . They are harder than previous measurements at a few tens of GeV nucleon −1 . The helium flux is higher than that expected from the extrapolation of the power law fitted to the lower-energy data. The relative abundance of protons to helium nuclei is 9.1 ± 0.5 for the range from 2.5 TeV nucleon −1 to 63 TeV nucleon −1 . This ratio is considerably smaller than the previous measurements at a few tens of GeV nucleon −1 .

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Metadata

Authors
Yoon, Y. S., Ahn, H. S., Allison, P. S., Bagliesi, M. G., Beatty, J. J., Bigongiari, G., Boyle, P. J., Childers, J. T., Conklin, N. B., Coutu, S., DuVernois, M. A., Ganel, O., Han, J. H., Jeon, J. A., Kim, K. C., Lee, M. H., Lutz, L., Maestro, P., Malinine, A., Marrocchesi, P. S., Minnick, S. A., Mognet, S. I., Nam, S., Nutter, S., Park, I. H., Park, N. H., Seo, E. S., Sina, R., Swordy, S., Wakely, S. P., Wu, J., Yang, J., Zei, R., & Zinn, S. Y.
Venue
The Astrophysical Journal
Published
2011-01-28
Volume
728
Issue
2
Pages
122
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2131730920
Cited by
334
References
18
FWCI
13.10
Type
journal article
Language
en
Open access
green

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The paper
Yoon, Y. S., Ahn, H. S., Allison, P. S., Bagliesi, M. G., Beatty, J. J., Bigongiari, G., Boyle, P. J., Childers, J. T., Conklin, N. B., Coutu, S., DuVernois, M. A., Ganel, O., Han, J. H., Jeon, J. A., Kim, K. C., Lee, M. H., Lutz, L., Maestro, P., Malinine, A., . . . Zinn, S. Y. (2011). COSMIC-RAY PROTON AND HELIUM SPECTRA FROM THE FIRST CREAM FLIGHT. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/728/2/122

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.