Fig. 28From: 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 fieldMotion \({\bf{V}}_{{\bf{IGM}}}^{\bf{S}}\) of the interstellar gaseous matter (IGM) relative to the neighboring stars (S) inferred from the motion \({\bf{V}}_{{\bf{HMS}}}^{{\bf{CS}}}\) of HMS relative to S observed by CRs and the motion \({\bf{V}}_{{\bf{np}}}^{{\bf{HMS}}}\) of the neutral particles (np) relative to the HMS.Back to article page