• Title of article

    α–ω Effect and peculiarities of the 27-day variations of the galactic cosmic rays intensity, solar wind and solar activity parameters Original Research Article

  • Author/Authors

    A. Gil، نويسنده , , M.V. Alania، نويسنده ,

  • Issue Information
    دوهفته نامه با شماره پیاپی سال 2013
  • Pages
    6
  • From page
    951
  • To page
    956
  • Abstract
    We show that the amplitudes of the 27-day variations of galactic cosmic ray (GCR) intensity, solar wind and solar activity parameters have a periodicity with duration of three to four Carrington rotation periods (3–4 CRP). We assume that the general reason for this phenomenon may be related to similar cyclicity of topological structure of the solar magnetic field lines created owing to the asymmetry of turbulent solar dynamo and solar differential rotation transforming the Sun’s poloidal magnetic field to the toroidal (α–ω effect), and vice versa.
  • Keywords
    Solar dynamo , Sun’s differential rotation , 27-day variation of GCR
  • Journal title
    Advances in Space Research
  • Serial Year
    2013
  • Journal title
    Advances in Space Research
  • Record number

    1134794