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
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