  Using the simple model for the description of the GCR modulation in the
heliosphere and the sets of parameters discussed in the accompanying paper we
model some features of the time and energy behavior of the GCR intensity near
the Earth observed during periods of low solar activity around three last solar
minima. In order to understand the mechanisms underlying these features in the
GCR behavior, we use the suggested earlier decomposition of the calculated
intensity into the partial intensities corresponding to the main processes
(diffusion, adiabatic losses, convection and drifts).
