Cosmic ray intensity fluctuations of interplanetary and ionospheric origin

Details Cosmic ray intensity fluctuations of interplanetary and ionospheric origin Cosmic ray intensity fluctuations of interplanetary and ionospheric origin

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55.1975a&link_type=abstract

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

Computer Science

Earth Ionosphere, Solar Cosmic Rays, Solar Flares, Solar Terrestrial Interactions, Solar X-Rays, Particle Flux Density, Radiant Flux Density, Ultraviolet Radiation

Scientific paper

It is shown that variations caused by wave processes in the earth's ionosphere as well as spectral precursors of solar flares are observed in the frequency spectra of the intensity fluctuations of the neutron component of cosmic rays in frequency regions higher than 0.0001 Hz. If precursors of solar events exist in solar UV rays or X-rays, they can give, through the earth's ionosphere, the corresponding response in the spectral characteristics of cosmic ray intensity fluctuations.

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