The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.
Energy spectra of abundant nuclei of primary cosmic rays from the data of ATIC-2 experiment: Final results
Open accessAbstract
The final results of processing the data from the balloon-born experiment ATIC-2 (Antarctica, 2002–2003) for the energy spectra of protons and He, C, O, Ne, Mg, Si, and Fe nuclei, the spectrum of all particles, and the mean logarithm of atomic weight of primary cosmic rays as a function of energy are presented. The final results are based on improvement of the methods used earlier, in particular, considerably increased resolution of the charge spectrum. The preliminary conclusions on the significant difference in the spectra of protons and helium nuclei (the proton spectrum is steeper) and the non-power character of the spectra of protons and heavier nuclei (flattening of carbon spectrum at energies above 10 TeV) are confirmed. A complex structure of the energy dependence of the mean logarithm of atomic weight is found.
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Cites
Measurements of primary and atmospheric cosmic-ray spectra with the BESS-TeV spectrometer
Haino, S., Sanuki, T., Abe, K., Anraku, K., Asaoka, Y., Fuke, H., Imori, M., Itasaki, A., Maeno, T., Makida, Y., et al. (2004) · Physics Letters B · doi:10.1016/j.physletb.2004.05.019 · Cited by 268
Self-citationAlcaraz, J., Alpat, B., Ambrosi, G., Anderhub, H., Ao, L., Arefiev, A., Azzarello, P., Babucci, E., Baldini, L., Basile, M., et al. (2000) · Physics Letters B · doi:10.1016/s0370-2693(00)00970-9 · Cited by 264
Self-citationAlcaraz, J., Alpat, B., Ambrosi, G., Anderhub, H., Ao, L., Arefiev, A., Azzarello, P., Babucci, E., Baldini, L., Basile, M., et al. (2000) · Physics Letters B · doi:10.1016/s0370-2693(00)01193-x · Cited by 168
Self-citationThe cosmic-ray proton and helium spectra measured with the CAPRICE98 balloon experiment
Boezio, M., Bonvicini, V., Schiavon, P., Vacchi, A., Zampa, N., Bergström, D., Carlson, P., Francke, T., Hansen, P., Mocchiutti, E., et al. (2003) · Astroparticle Physics · doi:10.1016/s0927-6505(02)00267-0 · Cited by 130
Cited by
COSMIC-RAY PROTON AND HELIUM SPECTRA FROM THE FIRST CREAM FLIGHT
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., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/728/2/122 · Cited by 334
Self-citationAguilar, M., Ali Cavasonza, L., Alpat, B., Ambrosi, G., Arruda, L., Attig, N., Aupetit, S., Azzarello, P., Bachlechner, A., Barao, F., et al. (2017) · Physical Review Letters · doi:10.1103/physrevlett.119.251101 · Cited by 293
Self-citationThe Badhwar‐O'Neill 2020 GCR Model
Slaba, T. C., & Whitman, K. (2020) · Space Weather · doi:10.1029/2020sw002456 · Cited by 78
Metadata
- Authors
- Panov, A. D., Adams, J. H., Ahn, H. S., Bashinzhagyan, G. L., Watts, J. W., Wefel, J. P., Wu, J., Ganel, O., Guzik, T. G., Zatsepin, V. I., Isbert, I., Kim, K. C., Christl, M., Kouznetsov, E. N., Panasyuk, M. I., Seo, E. S., Sokolskaya, N. V., Chang, J., Schmidt, W. K. H., & Fazely, A. R.
- Venue
- Bulletin of the Russian Academy of Sciences: Physics
- Publisher
- Allerton Press
- Published
- 2009-05
- Volume
- 73
- Issue
- 5
- Pages
- 564-567
- ISSN
- 1062-8738 (ISSN-L)
- 1934-9432
- OpenAlex
- W2142385112
- Cited by
- 339
- References
- 4
- FWCI
- 5.31
- Type
- journal article
- Language
- en
- Open access
- green
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- Panov, A. D., Adams, J. H., Ahn, H. S., Bashinzhagyan, G. L., Watts, J. W., Wefel, J. P., Wu, J., Ganel, O., Guzik, T. G., Zatsepin, V. I., Isbert, I., Kim, K. C., Christl, M., Kouznetsov, E. N., Panasyuk, M. I., Seo, E. S., Sokolskaya, N. V., Chang, J., Schmidt, W. K. H., & Fazely, A. R. (2009). Energy spectra of abundant nuclei of primary cosmic rays from the data of ATIC-2 experiment: Final results. Bulletin of the Russian Academy of Sciences: Physics. https://doi.org/10.3103/s1062873809050098
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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