A periodical analysis of the cosmic-ray diffusion coefficient and the high-speed solar-wind streams

Details A periodical analysis of the cosmic-ray diffusion coefficient and the high-speed solar-wind streams A periodical analysis of the cosmic-ray diffusion coefficient and the high-speed solar-wind streams

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988em%26p...43..165x&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 43, Nov. 1988, p. 165-179.

Physics

Diffusion Coefficient, Solar Cosmic Rays, Solar Cycles, Solar Wind, Interplanetary Magnetic Fields, Power Spectra, Three Dimensional Models

Scientific paper

A three-dimensional model has been applied to monthly data obtained by the Inuvik neuton-monitor station in order to study the long-term modulation of cosmic-ray intensity in solar cycles 20 and 21. The K coefficient is used to determine sunspot numbers in terms of high-speed solar-wind streams, and the coefficient is shown to be related to the diffusion process of cosmic rays. Similar periods are obtained for the data of the two solar cycles.

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