The structure and evolution of interplanetary shocks and the relevance for particle acceleration.

Details The structure and evolution of interplanetary shocks and the relevance for particle acceleration. The structure and evolution of interplanetary shocks and the relevance for particle acceleration.

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995nuphs..39...35c&link_type=abstract

Nuclear Physics B - Proceedings Supplements, vol. 39, issue 1, pp. 35-44

Physics

Nuclear Physics

2

Interplanetary Shock Waves: Solar Cosmic Rays, Interplanetary Shock Waves: Particle Acceleration

Scientific paper

It is now widely accepted that interplanetary shocks initiated by coronal mass ejections play a dominant role in the generation of the vast majority of large solar energetic particle events. However, our understanding of the details of the acceleration process is far from complete. It is important to better understand the large-scale properties of shocks and how these properties change with distance from the Sun. The author summarizes shock and particle observations and indicates where the problems lie.

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