The influence of nonstationarity of the solar activity and general solar field on modulation of cosmic rays

Computer Science – Numerical Analysis

Scientific paper

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Diffusion Coefficient, Drift Rate, Galactic Cosmic Rays, Interplanetary Space, Models, Modulation, Numerical Analysis, Particles, Solar Magnetic Field, Electron Emission, Proton Beams, Rates (Per Time), Solar Activity

Scientific paper

A numerical model is presented of the propagation of galactic cosmic rays in the interplanetary space for the case when the modulation depth determined by the level of the solar activity changed in time. The contribution of the particle drift in the regular field was also calculated and the agreement with experimental data is shown about the ratio of protons and electrons in two solar activity minima.

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