The formation of the sunspot and magnetic cycles in the GCR intensity in the heliosphere

We compare the different approaches (observational and theoretical) to the definition and separation of the GCR intensity variations due to the changing number and area of sunspots (the sunspot cycle) and the changing polarity of the high-latitude solar magnetic fields (the magnetic cycle). Using the theoretical approach we can consider how both types of the GCR intensity variations change with energy in different parts of the heliosphere during the minima of the sunspot cycle and their relative weights in the calculated intensity.