GENERAL MAGNETIC FIELD OF THE SUN AS A ST AR AS INDICA TOR OF MASSIVE STREAMS FLOWING ON THE SUN

GENERAL MAGNETIC FIELD OF THE SUN AS A ST AR AS INDICA TOR OF MASSIVE STREAMS FLOWING ON THE SUN

The behaviour of the General Magnetic Field of the Sun as a Star (GMFSS) is characterized by the change of amplitude of oscillations with the eleven-year cycle of activity. In maximum of activity GMFSS reaches its maximal values, and in a minimum reaches minimal values. The values of active frequenc...

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Bibliographic Details
Main Authors: S. Plachinda, D. Baklanova, I. Han, K. M. Kim, P. Reegen, G. Valyavin, W. Weiss
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2008-12-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/86869

Internet

http://oap.onu.edu.ua/article/view/86869

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