Abstract
The mechanism of cosmic-ray acceleration by diffusive shock waves (1–4) is now very popular, especially for galactic cosmic-ray acceleration. First, we briefly summarize the main features of the mechanism. For more details the reader is referred to the second lecture by C. Cesarsky.
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References
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© 1983 D. Reidel Publishing Company
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Lagage, P.O. (1983). Cosmic-Ray Acceleration by Diffusive Shocks: Cut-Off Energy. 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_12
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DOI: https://doi.org/10.1007/978-94-009-7166-0_12
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