Fig. 10.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 HMSThe seasonal variation of D(j, y)TSO in Eq. (8) on the solar harmonic diagram (X′, Y′) on the left side and its on the right. The X′-axis is in the direction of D(j, 0)TSO whose magnitude is normalized to unity.Back to article page