A Simple Model of Cosmic Ray Modulation in the Heliosphere

Physics

Scientific paper

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Scientific paper

The cosmic ray modulation by the interplanetary magnetic field of simple geometry is considered. The turbulent component of field is assumed to be proportional to the total field intensity with a proportional coefficient indep ending on the coordinates but varying with the 11-year cycle. The expected variations are compared with the ground-based results for many years.

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