Coronal propagation of flare associated electrons and protons

Details Coronal propagation of flare associated electrons and protons Coronal propagation of flare associated electrons and protons

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..305s&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 305-308 (SEE N85-34729 23-92)

Physics

Electrons, Solar Corona, Solar Cosmic Rays, Solar Flares, Solar Protons, Helios 1, Helios 2, Interplanetary Medium, Magnitude, Particle Motion, Radiative Transfer

Scientific paper

A statistical study of characteristic times and intensities of 36 solar particle events observed between 1977 and 1979 by the Kiel Cosmic Ray Experiment on board HELIOS-1 and -2 has been carried out. For approx. 0.5 MeV electrons we order the times of maximum and the absolute intensities with respect to angular distance from the parent flare. Discussion of coronal parameters in terms of Reid's model leads to typical time constants for coronal diffusion and escape.

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