Features of the ground-level increase of solar cosmic rays on September 29, 1989, from neutron monitor data

Details Features of the ground-level increase of solar cosmic rays on September 29, 1989, from neutron monitor data Features of the ground-level increase of solar cosmic rays on September 29, 1989, from neutron monitor data

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55.1877b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, Russia, Nov. 1-3, 1990, Materialy. A92-40776 16-93) Akademiia Nauk

Computer Science

Energy Spectra, Solar Cosmic Rays, Solar Neutrons, Solar Terrestrial Interactions, Energetic Particles, Geomagnetic Pulsations, Magnetospheric Instability, Radiation Spectra

Scientific paper

Absolute values and variations of the energy spectrum of solar cosmic rays are obtained from the ground-level increase in solar cosmic ray intensity on September 29, 1989, as evidenced by neutron monitor data. The specifics of this event are discussed. The event makes it possible to study the anisotropy and gradients of solar cosmic rays, to obtain diffusion characteristics of the interplanetary medium, and to determine the integral multiplicity of the neutron component for energies less than 2 GeV.

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