Cosmic-ray flux distribution in interplanetary-magnetic-field sectors

Details Cosmic-ray flux distribution in interplanetary-magnetic-field sectors Cosmic-ray flux distribution in interplanetary-magnetic-field sectors

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978izyak..42.1067k&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, June 1977.) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheska

Computer Science

Cosmic Rays, Galactic Radiation, Interplanetary Magnetic Fields, Particle Flux Density, Adiabatic Conditions, Convection, Deceleration, Solar Wind

Scientific paper

The behavior of galactic-cosmic-ray fluxes and flux density within an interplanetary-magnetic-field (IMF) sector is examined using data on the cosmic-ray neutron component. The observed effects are explained in the framework of the diffusion model of cosmic-ray propagation with allowance for convection and adiabatic deceleration. It is shown that the degree of IMF irregularity may depend in an arbitrary manner on the heliocentric longitude of a magnetic sector and that the cosmic-ray flux distribution in such a sector is governed by both the presence of high-speed solar-wind streams and the behavior of the cosmic-ray diffusion coefficients.

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