Fig. 4.From: The influence of the sidereal cosmic-ray anisotropies originated on the tail- and nose-boundaries of the heliomagnetosphere (HMS) upon the solar cosmic-ray anisotropy produced inside the HMS-diagrams showing the distributions of the theoretical due to the diffusion-convection of cosmic rays for various combinations of parameters γ and pu of the rigidity spectrum. The stations in these figures are not always the same as those in Fig. 3. The bold point is for the vertical (V) muon telescope at Nagoya (35°N).Back to article page