Fig. 3.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 HMSDistributions of on the -diagrams in the respective selected years during the period of 1970–2007, showing their dependence on the solar activity and the polarity of the solar polar magnetic field. The bold point is for the vertical (V) muon telescope at Nagoya (35°N).Back to article page