Cosmic-ray density gradients during solar flares and Forbush effects

Details Cosmic-ray density gradients during solar flares and Forbush effects Cosmic-ray density gradients during solar flares and Forbush effects

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roizf..57...55b&link_type=abstract

Rossijskaya Akademiya Nauk, Izvestiya, Seriya Fizicheskaya (ISSN 0367-6765), vol. 57, no. 7, p. 55-58.

Physics

Forbush Decreases, Galactic Cosmic Rays, Particle Flux Density, Solar Cosmic Rays, Solar Flares, Neutron Counters, Solar Protons

Scientific paper

Neutron-monitor data for cases of solar flares are used to calculate
radial gradients of cosmic-ray density based on the N-S asymmetry. It is
shown that the density gradients, during both flares and Forbush
effects, amount to several tens of percent per AU and experience
significant variations.

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