Upper energy limit of particles accelerated in a solar flare

Details Upper energy limit of particles accelerated in a solar flare Upper energy limit of particles accelerated in a solar flare

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ge%26ae..28..197b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 28, Mar.-Apr. 1988, p. 197-201. In Russian.

Physics

2

Particle Acceleration, Particle Energy, Solar Flares, Solar Activity, Solar Cycles, Solar Protons, Statistical Analysis

Scientific paper

A statistical analysis is used to estimate the upper energy level for flare-accelerated particles, which does not exceed 500 MeV for the majority of proton events. In intense events recorded in the stratosphere and with neutron monitors, this limit, as a rule, is of the order of several GeV. Proton events with maximum particle energy are observed at the growth and decline phase of solar activity, not at the cycle maximum.

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