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Fig. 22 | Earth, Planets and Space

Fig. 22

From: 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

Fig. 22

(a) Latitude dependence of \({{\rm{S}}_{\rm{i}}}{\rm{D}}({{\rm{t}}_{{{\rm{S}}_{\rm{i}}}}})\) observed by muon telescopes (S3, S2, S, N) at Nagoya in the period of 1971–2003 to show the existence of \({\rm{H(}}{{\rm{t}}_{{{\rm{S}}_{\rm{i}}}}}{\rm{)}}\) with the maximum phase at 18 hr, and (b) the modulation pattern of \({{\rm{S}}_{\rm{i}}}{\rm{D}}({{\rm{t}}_{{{\rm{S}}_{\rm{i}}}}})\) of S-component in (a) which shows clearly the existence of

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