Cosmic-ray intensity related to solar and terrestrial activity indices in solar cycle No. 20

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Cosmic Rays, Geomagnetism, Magnetic Variations, Particle Flux Density, Solar Activity Effects, Solar Cycles, Annual Variations, Indexes (Ratios), Interplanetary Space, Solar Protons, Solar Wind, Sunspot Cycle, Sunspots

Scientific paper

The existence of an 11-year modulation of cosmic-ray intensity in the 20th solar cycle is found using data from nine neutron monitoring stations over the period 1965-1975. A fundamental equation which describes the long-term modulation of cosmic-ray intensity is obtained. According to this relation, the modulated intensity measured by the ground stations is equal to the galactic cosmic-ray intensity (unmodulated) at a finite distance (corrected by a few appropriate solar and terrestrial activity indices) which causes disturbances in interplanetary space. The relation is explained by a generalization of the Simpson solar wind model (1963).

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