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Fig. 4 | Earth, Planets and Space

Fig. 4

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. 4

Elimination of \({{\bf{S}}_{\bf{i}}}{\bf{D}}_{\bf{1}}^{\bf{f}}\) from \({{\bf{S}}_{\bf{i}}}{\bf{D}}_{\bf{1}}^{\bf{o}}\) by using \({\bf{A}}{{\bf{S}}_{\bf{i}}}{\bf{D}}_{\bf{1}}^{\bf{f}}\) according to the CSSA method. The corrected vector \({{\bf{S}}_{\bf{i}}}{{\bf{D}}_{\bf{1}}}\) is on the right. (a) Underground CR intensities at London (L) and Hobart (H), (Nagashima et al., 1985); (b) those at Sakashita (S), Misato (M) and Nagoya (N) at sea level; (c) those at Embudo (E), Socorro (S) and Bolivia (B). The telescopes point vertical (V), North (N) and South (S) at each location and only the observed vectors and, on the right, the corrected vectors, as shown. The amplitude scale is in percent.

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