کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
1764630 1020065 2013 6 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
α-ω Effect and peculiarities of the 27-day variations of the galactic cosmic rays intensity, solar wind and solar activity parameters
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات علوم فضا و نجوم
پیش نمایش صفحه اول مقاله
α-ω Effect and peculiarities of the 27-day variations of the galactic cosmic rays intensity, solar wind and solar activity parameters
چکیده انگلیسی
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.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Advances in Space Research - Volume 52, Issue 5, 1 September 2013, Pages 951-956
نویسندگان
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