Charge composition and energy spectra of cosmic-ray nuclei for elements from Be to NI - Results from HEAO-3-C2

Details Charge composition and energy spectra of cosmic-ray nuclei for elements from Be to NI - Results from HEAO-3-C2 Charge composition and energy spectra of cosmic-ray nuclei for elements from Be to NI - Results from HEAO-3-C2

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...233...96e&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 233, no. 1, July 1990, p. 96-111.

Astronomy and Astrophysics

Astrophysics

307

Abundance, Cosmic Rays, Heao 3, Nuclear Astrophysics, Spectral Energy Distribution, Astronomical Models, Cerenkov Counters, Charged Particles, Stellar Composition

Scientific paper

Final results of the HEAO-C2 data on the elemental composition of cosmic rays up to Z = 28 are presented. A new table of elemental abundances and absolute energy spectra of cosmic ray nuclei with Z = 4 to 28 in the 0.6-35 GeV/n range, as measured in 1980, is presented. The source spectrum for all species is reasonably well fit by a power law in momentum, with a spectral index of 2.23 + or - 0.05, but only up to 16 GeV/n.

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