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Earth, Planets and Space
Fig. 12 | Earth, Planets and Space

Fig. 12

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. 12

Energy dependence of the phase of the observed SiD1 cited from Ref. 3. All the SiD1’s except several in the high-energy region are those of the vertical intensities corrected by the CSSA method, or those for the equatorially directed telescopes which do not require the above correction owing to a negligible influence. BO, Bolivia; SO, Socorro (Swinson and Nagashima, 1985); MI, Misato; HO, Hobart; BU, Budapest; YA, Yakutsk; LO, London (Nagashima et al., 1985 and references therein); SA, Sakashita (Ueno et al., 1990); LS, London (Thambyahpillai, 1983); LP, Laipootah; MV, Matsushiro (Mori et al., 1993); OT, Ottawa (Bercovitch and Agrawal, 1981); MS, Matsushiro (Mori et al., 1989); UT, Utah (Cutler and Groom, 1991); PO, Poatina (Fenton and Fenton, 1975;Humble et al., 1985); HK, Hong Kong (Lee and Ng, 1987); BM, Baksan (Andreyev et al., 1987); BA, Baksan (Alexeenko et al., 1981); NO, Norikura (Nagashima et al., 1989); DA, Norikura, directional air showers (Nagashima et al., 1989) and MU, Musala (Gombosi et al., 1975).

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