A model of propagation of solar flare particles and its application to cosmic ray ground level events

Details A model of propagation of solar flare particles and its application to cosmic ray ground level events A model of propagation of solar flare particles and its application to cosmic ray ground level events

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982jgr....87.4338l&link_type=abstract

Journal of Geophysical Research, vol. 87, June 1, 1982, p. 4338-4344. Swiss National Science Foundation

Physics

20

Cosmic Rays, Interplanetary Magnetic Fields, Particle Flux Density, Relativistic Particles, Solar Flares, Solar Protons, Mean Free Path, Monte Carlo Method, Propagation Modes, Proton Scattering, Solar X-Rays

Scientific paper

A Monte Carlo simulation of the propagation of relativistic solar flare protons in the interplanetary magnetic field was used to understand the intensity-time profiles and anisotropies for the GLEs on Nov. 22, 1977 and May 7, 1978. Mean free paths for pitch angle scattering of 0.5 AU and 5 AU, respectively, were deduced. The injection of the solar flare protons had an extended time structure that was found to be of similar shape as the X ray burst profiles in the bands 1-8 A and 0.5-4 A, respectively.

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