Physics
Scientific paper
Feb 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980p%26ss...28..177n&link_type=abstract
Planetary and Space Science, vol. 28, Feb. 1980, p. 177-194.
Physics
25
Electromagnetic Fields, Long Term Effects, Solar Activity Effects, Solar Cosmic Rays, Solar Wind, Diffusion Coefficient, Integral Equations, Life (Durability), Radial Distribution, Solar Magnetic Field, Time Lag
Scientific paper
It is demonstrated that the long term variation in cosmic ray intensity can be described by an integral equation derived from a generalization of Simpson's (1963) coasting solar wind model. Moreover, the equation can be derived from the general diffusion-convection theory and as a result, the source and characteristic functions can be related to the diffusion coefficient and its transition in space. Based on the theory, one can obtain the transition and life time of solar disturbances, boundary of the modulating region, radial and time dependences of the diffusion coefficient, radial density gradient, and modulated intensity of cosmic rays.
Morishita I.
Nagashima Kana
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