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   <subfield code="a">Variable anisotropy of cosmic rays with E 0 ⩽ 1018 eV from Yakutsk EAS array data</subfield>
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   <subfield code="a">Results of a harmonic analysis of the arrival directions for primary cosmic-ray particles with energies E 0 ⩾ 1017 eV and zenith angles θ ⩽ 45° recorded on the Yakutsk array over 29 years of its continuous operation (1983-2012) are presented. These events are shown to have different global anisotropies in different time intervals: the phase of the first harmonic φ 1 = 119° ± 18° and its amplitude A 1 = 0.030 ± 0.014 in the 1983-1994 samples changed into φ 1 = 284° ± 13° and A 1 = 0.033 ± 0.010 in 1998-2010. All of this could be caused by a considerably increased flux of heavy nuclei from the exit of the Galaxy's local arm after 1996.</subfield>
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