Radial and transverse gradients of cosmic rays in the 22-year solar cycle

Details Radial and transverse gradients of cosmic rays in the 22-year solar cycle Radial and transverse gradients of cosmic rays in the 22-year solar cycle

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2110a&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Physics

Cosmic Rays, Solar Cycles, Gradients, Interplanetary Space, Periodic Variations, Plasma-Electromagnetic Interaction, Radial Distribution, Radiant Flux Density, Solar Activity Effects, Solar Magnetic Field

Scientific paper

The transverse and radial gradients of cosmic rays in interplanetary space are determined from the expected heliolatitudinal and heliocentric radial distributions of the relative density of galactic cosmic rays. An analysis is made of the dependence of the radial gradient for particles with a rigidity of 10 GV on distance for different periods and different orientations of the solar magnetic field; and of the distribution of the transverse gradient for different epochs in relation to solar latitude at a distance of 1 AU for particles with a rigidity of 10 GV for different orientations of the solar magnetic field.

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