Search for singularities of proton events in solar cycle 22 from ground-based observation data

Physics

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Solar Protons, Solar Activity, Solar Terrestrial Interactions, Solar Cosmic Rays, Radiation Distribution, Solar Neutrinos, Proton Flux Density

Scientific paper

The characteristics of the increases in solar cosmic rays detected on the earth surface during solar cycle 22 are investigated using data of neutron monitors with a high time resolution. The event frequency in 1989-1991 exceeded the mean annual frequency (about 1/yr) for the entire period of solar cosmic ray observations by a factor of 4. The shape of the time profiles for a number of events is characterized by a two-hump structure, indicating the possibility of dual emission of solar cosmic rays from two different coronal sources.

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