Elemental energy spectra of cosmic rays from the data of the ATIC-2 experiment
Document Type
Conference Proceeding
Publication Date
4-1-2007
Abstract
This paper reports on the results of measurements performed in the course of the ATIC-2 balloon experiment (2002-2003) for the energy spectra of particles (such as protons; He, C, O, Ne, Mg, Si, and Fe nuclei; and some groups of nuclei) and the all-particle energy spectrum in primary cosmic rays at energies ranging from 50 GeV to 200 TeV. The conclusion is drawn that the energy spectra of protons and helium nuclei differ substantially (the spectrum of protons is steeper) and that the shape of the energy spectra of protons and heavy nuclei cannot be described by a power function. © Allerton Press, Inc. 2007.
Publication Source (Journal or Book title)
Bulletin of the Russian Academy of Sciences: Physics
First Page
494
Last Page
497
Recommended Citation
Panov, A., Adams, J., Ahn, H., Batkov, K., Bashindzhagyan, G., Watts, J., Wefel, J., Wu, J., Ganel, O., Guzik, T., Gunashingha, R., Zatsepin, V., Isbert, J., Kim, K., Christl, M., Kouznetsov, E., Panasyuk, M., Seo, E., Sokolskaya, N., Chang, J., Schmidt, W., & Fazely, A. (2007). Elemental energy spectra of cosmic rays from the data of the ATIC-2 experiment. Bulletin of the Russian Academy of Sciences: Physics, 71 (4), 494-497. https://doi.org/10.3103/S1062873807040168