Fig. 25From: 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 fieldThe averages of \({{\rm{S}}_{\rm{i}}}{\rm{D}}({{\rm{t}}_{{{\rm{S}}_{\rm{i}}}}})\) for 6 years (1981, ’83, ’84, ’87, ’88, ’89) in AN and QN periods, selected from those in Fig. 22(a). \({\rm{G}}({{\rm{t}}_{{{\rm{S}}_{\rm{i}}}}})\) can be clearly seen, especially in the low latitude region.Back to article page