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Elemental abundances in the local cosmic rays at high energies
The Astrophysical Journal1993Vol. 403, pp. 658–658
Citations Over TimeTop 10% of 1993 papers
Abstract
The heavy-nuclei energy spectra measured aboard the Space Shuttle and on HEAO 3 are presently discussed in the framework of a leaky-box model; the source energy spectrum required for a fit, at E exp -2.2 for all nuclear species, is slightly steeper than a previous estimate. These data are presented in terms of total energy/particle, in order to allow direct comparison with the observed all-particle spectrum of cosmic rays.
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