The acceleration of charged particles in interplanetary shock waves

Details The acceleration of charged particles in interplanetary shock waves The acceleration of charged particles in interplanetary shock waves

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ssrv...32..185p&link_type=abstract

(Slovenska Akademia Vied, IAU, and COSPAR, Study of Travelling Interplanetary Phenomena Workshop on Shock Waves in the Solar Cor

Physics

49

Interplanetary Space, Ion Motion, Particle Acceleration, Shock Wave Interaction, Solar Wind, Energy Spectra, Particle Diffusion, Pitch (Inclination)

Scientific paper

Consideration of the theoretical and observational literature on energetic ion acceleration in interplanetary shock waves is the basis for the present discussion of the shock acceleration of the solar wind plasma and particle transport effects. It is suggested that ISEE data be used to construct data sets for shock events that extend continuously from solar wind to galactic cosmic ray energies, including data for electrons, protons, alphas and ions with Z values greater than 2.0, and that the temporal and spatial evolution of two- and three-dimensional particle distribution functions be studied by means of two or more spacecraft.

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