Fig. 14From: The existence of cosmic ray sidereal anisotropies of galactic and solar origins with energies lower than 104 GeV and their modulation caused by the presumed behavior pattern of the heliomagnetosphere and of its neighboring gaseous matter in interstellar magnetic field(a) Latitude and Energy dependence of \({{\rm{S}}_{\rm{i}}}{\rm{D(}}{{\rm{t}}_{{{\rm{S}}_{\rm{i}}}}}{\rm{)}}\), suggesting the existence of two kinds of sidereal anisotropies \({\rm{G(}}{{\rm{t}}_{{{\rm{S}}_{\rm{i}}}}}{\rm{)}}\) and T\({\rm{T(}}{{\rm{t}}_{{{\rm{S}}_{\rm{i}}}}}{\rm{)}}\) respectively from α = 0 hr and 6 hr and (b) the three of them without CSSA, together with their associated \({\rm{A}}{{\rm{S}}_{\rm{i}}}{\rm{D(}}{{\rm{t}}_{{\rm{AS}}}}{\rm{)}}\), to show their influence on \({{\rm{S}}_{\rm{i}}}{\rm{D}}^\circ {\rm{(}}{{\rm{t}}_{{\rm{Si}}}}{\rm{)}}\).Back to article page