Azimuthal distribution and escape of accelerated particles from the solar corona

Details Azimuthal distribution and escape of accelerated particles from the solar corona Azimuthal distribution and escape of accelerated particles from the solar corona

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26..187b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, Mar.-Apr. 1986, p. 187-190. In Russian.

Physics

6

Azimuth, Particle Acceleration, Particle Emission, Solar Corona, Solar Cosmic Rays, Solar Protons, Distribution (Property), Escape Velocity, Propagation Velocity, Statistical Analysis

Scientific paper

Coronal effects of solar cosmic rays are examined on the basis of a statistical analysis of the parameters of solar proton events. Calculations are made of the azimuthal-propagation velocity of accelerated particles in the corona and of delays in their escape into interplanetary space. Attention is given to the relationship between the dimensions of regions of fast coronal propagation of fast escape.

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