Large-scale cosmic ray fluctuations inferred from the ground-based neutron and ionizing component observations and their relevance to cosmic ray anisotropy

The work treats with the behavior of the cosmic ray fluctuation power spectrum in the frequency range below 10 -4 Hz inferred from ground-based observations of the neutron and ionizing components. An attempt is made to describe the observed rearrangement of the fluctuation spectrum using changes in the value of the cosmic ray anisotropy and the rearrangement of the IMF inhomogeneity spectrum.