Time and spectral characteristics of particles near the sun for the proton events of Dec. 8, 1982 and Nov. 19, 1949

Details Time and spectral characteristics of particles near the sun for the proton events of Dec. 8, 1982 and Nov. 19, 1949 Time and spectral characteristics of particles near the sun for the proton events of Dec. 8, 1982 and Nov. 19, 1949

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..309m&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, Mar.-Apr. 1989, p. 309-311. In Russian.

Computer Science

1

Energy Spectra, Relativistic Particles, Solar Cosmic Rays, Temporal Distribution, Particle Acceleration, Solar Corona, Solar Flares, Solar Protons

Scientific paper

The energy spectra near the sun and the time profiles of the emission of relativistic protons in the events of Dec. 8, 1982 and Nov. 19, 1949 are determined by solving the inverse problem of solar-cosmic-ray propagation. A comparison of time profiles of emission for three events (including the flare of Feb. 23, 1956) indicates that accelerated particles are delayed in the solar corona.

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