UH nuclei - implications for acceleration theory

Details UH nuclei - implications for acceleration theory UH nuclei - implications for acceleration theory

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995adspr..15...65d&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 15, no. 6, p. (6)65-(6)70

Computer Science

Anomalies, Chemical Composition, Galactic Cosmic Rays, Heavy Nuclei, Particle Acceleration, Shock Fronts, Supernovae, Abundance, Diffusion Length, Diffusion Theory, Propagation Velocity, Shock Wave Propagation

Scientific paper

The significance of ultra-heavy compositional anomalies in the cosmic rays is discussed in the context of current ideas on cosmic ray acceleration. The diffusive shock acceleration process, operating at the shocks produced by supernova explosions, is thought to be responsible for the bulk of the Galactic cosmic rays. The status of the so-called 'injection problem' for this acceleration process is reviewed as is the pattern of shocks and compositional variations expected from supernova explosions.

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