Fig. 15From: 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 in the N-state (1985–1987) at the nine high latitudes stations at the top (A) and those in the three low latitude stations at the bottom (B). The influences of D(j, y)TSO and D(j, y)HSO due to F(y)TSO and F(y)HSO are shown by the bold-faced symbols with the labels T and H in the respective AEP’s, (cf. text). Inu: Inuvik (68°N), Oul: Oulu (65°N), New: Newark (40°N), Yak: Yakutsk (62°N), Clim: Climax (39°N), Tsum: Tsumeb (19°S), Potchef: Potchefstroom (27°S), Herma: Hermanus (34°S), Mt. Wel: Mt. Wellington (43°S), Nag: Nagoya (35°N), Huan: Huancayo (12°S), Beij: Beijing (40°N).Back to article page