The balloon-borne Cosmic Ray Energetics And Mass experiment launched five times from Antarctica has achieved a cumulative flight duration of about 156 days above 99.5% of the atmosphere. The instrument is configured with complementary and redundant particle detectors designed to extend direct measurements of cosmic-ray composition to the highest energies practical with balloon flights. All elements from protons to iron nuclei are separated with excellent charge resolution. Here, we report results from the first two flights of ∼70 days, which indicate hardening of the elemental spectra above ∼200 GeV/nucleon and a spectral difference between the two most abundant species, protons and helium nuclei. These results challenge the view that cosmic-ray spectra are simple power laws below the so-called knee at ∼10^15 eV. This discrepant hardening may result from a relatively nearby source, or it could represent spectral concavity caused by interactions of cosmic rays with the accelerating shock. Other possible explanations should also be investigated.

H. S., A., P., A., Bagliesi, M.G., J. J., B., Bigongiari, G., J. T., C., et al. (2010). Discrepant hardening observed in cosmic-ray elemental spectra. THE ASTROPHYSICAL JOURNAL LETTERS, 714(1, part 2), L89-L93 [10.1088/2041-8205/714/1/L89].

Discrepant hardening observed in cosmic-ray elemental spectra

BAGLIESI, MARIA GRAZIA;BIGONGIARI, GABRIELE;MAESTRO, PAOLO;MARROCCHESI, PIER SIMONE;ZEI, RICCARDO;
2010-01-01

Abstract

The balloon-borne Cosmic Ray Energetics And Mass experiment launched five times from Antarctica has achieved a cumulative flight duration of about 156 days above 99.5% of the atmosphere. The instrument is configured with complementary and redundant particle detectors designed to extend direct measurements of cosmic-ray composition to the highest energies practical with balloon flights. All elements from protons to iron nuclei are separated with excellent charge resolution. Here, we report results from the first two flights of ∼70 days, which indicate hardening of the elemental spectra above ∼200 GeV/nucleon and a spectral difference between the two most abundant species, protons and helium nuclei. These results challenge the view that cosmic-ray spectra are simple power laws below the so-called knee at ∼10^15 eV. This discrepant hardening may result from a relatively nearby source, or it could represent spectral concavity caused by interactions of cosmic rays with the accelerating shock. Other possible explanations should also be investigated.
H. S., A., P., A., Bagliesi, M.G., J. J., B., Bigongiari, G., J. T., C., et al. (2010). Discrepant hardening observed in cosmic-ray elemental spectra. THE ASTROPHYSICAL JOURNAL LETTERS, 714(1, part 2), L89-L93 [10.1088/2041-8205/714/1/L89].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11365/20546
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