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We consider the long-term behavior of the solar and heliospheric parametersand the GCR intensity in the periods of high solar activity and the inversionsof heliospheric magnetic field (HMF). The classification of the HMF polaritystructures and the meaning of the HMF inversion are discussed. The procedure isconsidered how to use the known HMF polarity distribution for the GCR intensitymodeling during the periods of high solar activity. We also briefly discuss thedevelopment and the nearest future of the sunspot activity and the GCRintensity in the current unusual solar cycle 24.

On the GCR intensity and the inversion of the heliospheric magnetic field during the periods of the high solar activity