Fig. 11.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 HMSSimulation of produced by D(j, y) TD in Eq. (9) for various combinations of β0 and ϕ0 in Eq. (10).Back to article page