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- W3046939052 abstract "Institute of Geophysics, Georgian Academy of Sciences, Tbilisi, Georgiagila@ap.siedlce.plrenatam@ap.siedlce.plalania@ap.siedlce.pl(Received January 29, 2007)We study features of the 27-day variations of the galactic cosmic ray(GCR) intensity and anisotropy using data of neutron monitors and solarwind (SW) velocity. We found that the larger amplitudes of the 27-dayvariations of the galactic cosmic ray anisotropy and intensity for the posi-tive polarity period (A > 0) of solar magnetic cycle than for the negativepolarity period (A 0 period. Also, we demonstrate an existence of the clear stable 27-daywaves of the GCR intensity and anisotropy with the amplitudes larger inthe A > 0 than in the A 0 are related with the superposition oftwo effects: (1) the existence of the more regular heliolongitudinal asym-metry of the solar wind velocity, and (2) a coincidence of convective anddrift streams of the GCR particles in comparison with the A < 0.PACS numbers: 96.50.Ci, 94.20.Wq, 96.50.–s" @default.
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- W3046939052 date "2008-05-01" @default.
- W3046939052 modified "2023-09-27" @default.
- W3046939052 title "FEATURES OF THE 27-DAY VARIATIONS OF THE GALACTIC COSMIC RAY INTENSITY AND ANISOTROPY" @default.
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