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
Link To Document :
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