Spectrum and composition of galactic cosmic rays accelerated in supernova remnants

Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena

Scientific paper

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4 pages, 4 figures, talk presented at 31st ICRC, Lodz, Poland, July 2009

Scientific paper

The spectra of high-energy protons and nuclei accelerated by supernova
remnant shocks are calculated taking into account magnetic field amplification
and Alfvenic drift for different types of SNRs during their evolution. The
overall energy spectrum and elemental composition of cosmic rays after
propagation through the Galaxy are found.

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