Fig. 9.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 HMSRigidity dependence of the geographic latitude of cosmic-ray asymptotic orbital direction in the geomagnetic field at j-station. The horizontal thick line (24° S) expresses the direction (δT = −24°) of the tail-in anisotropy.Back to article page