Journal
SPACE SCIENCE REVIEWS
Volume 99, Issue 1-4, Pages 329-352Publisher
SPRINGER
DOI: 10.1023/A:1013825905795
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The main features of cosmic-ray source models and acceleration processes are reviewed, with special emphasis on the possible observational tests, through both composition analysis and multi-wavelength studies of supernova remnants. Non-linear effects in the context of supernova-induced diffusive shock acceleration are discussed, as well as collective acceleration effects induced by multiple supernova explosions inside superbubbles.
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