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Cosmic Ray Sources

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Composition and Origin of Cosmic Rays

Part of the book series: NATO ASI Series ((ASIC,volume 107))

Abstract

Galactic Cosmic Ray Source (GCRS) abundances show, in general, strong similarities with the abundances measured in the Solar Energetic Particles, the Solar Corona and the Solar Wind, indicating (i) a common nucleosynthetic origin and history of the most common nuclides in these 4 samples, and (ii) that stellar coronae are probably the orimeval extraction site of galactic cosmic rays. 12C and 22Ne are remarkable exceptions, their overabundance in GCRS suggest an extra source for these nuclides, the carbon-rich Wolf-Rayet stars.

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  1. Section d’Astrophysique, Centre d’Etudes Nucléaires de Saclay, France

    Michel Casse

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  1. Michel Casse
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  1. Department of Physics and Astronomy, University of Iowa, USA

    Maurice M. Shapiro

  2. Institute for Astrophysics, University of Bonn, Germany

    Maurice M. Shapiro

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© 1983 D. Reidel Publishing Company

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Casse, M. (1983). Cosmic Ray Sources. In: Shapiro, M.M. (eds) Composition and Origin of Cosmic Rays. NATO ASI Series, vol 107. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7166-0_14

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  • DOI: https://doi.org/10.1007/978-94-009-7166-0_14

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